ICODE-ADC/lammps
4
0
Fork 0
Code Issues Pull Requests Actions Packages Projects Releases Wiki Activity

Merge branch 'upstream' into dielectric-updates

Browse Source
This commit is contained in:
Trung Nguyen
2022-12-25 15:13:46 -06:00
parent f091233d7d 07fe2fa29d
commit 652c237b5e
4218 changed files with 188014 additions and 28904 deletions
Download Patch File Download Diff File Expand all files Collapse all files

63
.github/CODEOWNERS vendored
View File

@ -13,40 +13,45 @@ lib/kim/* @ellio167
lib/mesont/* @iafoss
# whole packages
src/ADIOS/* @pnorbert
src/AMOEBA/* @sjplimp
src/COMPRESS/* @rbberger
src/GPU/* @ndtrung81
src/KOKKOS/* @stanmoore1
src/KIM/* @ellio167
src/LATTE/* @cnegre
src/MLIAP/* @athomps
src/SNAP/* @athomps
src/SPIN/* @julient31
src/BPM/* @jtclemm
src/BROWNIAN/* @samueljmcameron
src/CG-DNA/* @ohenrich
src/CG-SPICA/* @yskmiyazaki
src/COLVARS/* @giacomofiorin
src/COMPRESS/* @rbberger
src/DIELECTRIC/* @ndtrung81
src/ELECTRODE/* @ludwig-ahrens
src/FEP/* @agiliopadua
src/ML-HDNNP/* @singraber
src/GPU/* @ndtrung81
src/GRANULAR/* @jtclemm @dsbolin
src/INTEL/* @wmbrownintel
src/KIM/* @ellio167
src/KOKKOS/* @stanmoore1
src/LATTE/* @cnegre
src/MANIFOLD/* @Pakketeretet2
src/MDI/* @taylor-a-barnes
src/MDI/* @taylor-a-barnes @sjplimp
src/MEAM/* @martok
src/MESONT/* @iafoss
src/ML-HDNNP/* @singraber
src/ML-IAP/* @athomps
src/ML-PACE/* @yury-lysogorskiy
src/ML-POD/* @exapde @rohskopf
src/MOFFF/* @hheenen
src/MOLFILE/* @akohlmey
src/NETCDF/* @pastewka
src/ML-PACE/* @yury-lysogorskiy
src/PLUMED/* @gtribello
src/PHONON/* @lingtikong
src/PTM/* @pmla
src/OPENMP/* @akohlmey
src/PHONON/* @lingtikong
src/PLUGIN/* @akohlmey
src/PLUMED/* @gtribello
src/PTM/* @pmla
src/QMMM/* @akohlmey
src/REAXFF/* @hasanmetin @stanmoore1
src/REACTION/* @jrgissing
src/REAXFF/* @hasanmetin @stanmoore1
src/SCAFACOS/* @rhalver
src/SNAP/* @athomps
src/SPIN/* @julient31
src/TALLY/* @akohlmey
src/UEF/* @danicholson
src/VTK/* @rbberger
@ -59,6 +64,8 @@ src/MANYBODY/pair_atm.* @sergeylishchuk
src/REPLICA/*_grem.* @dstelter92
src/EXTRA-COMPUTE/compute_stress_mop*.* @RomainVermorel
src/MISC/*_tracker.* @jtclemm
src/MC/fix_gcmc.* @athomps
src/MC/fix_sgcmc.* @athomps
# core LAMMPS classes
src/lammps.* @sjplimp
@ -120,27 +127,32 @@ src/dump_movie.* @akohlmey
src/exceptions.h @rbberger
src/fix_nh.* @athomps
src/info.* @akohlmey @rbberger
src/timer.* @akohlmey
src/min* @sjplimp @stanmoore1
src/platform.* @akohlmey
src/timer.* @akohlmey
src/utils.* @akohlmey @rbberger
src/verlet.* @sjplimp @stanmoore1
src/math_eigen_impl.h @jewettaij
# tools
tools/msi2lmp/* @akohlmey
tools/coding_standard/* @akohlmey @rbberger
tools/emacs/* @HaoZeke
tools/singularity/* @akohlmey @rbberger
tools/coding_standard/* @rbberger
tools/valgrind/* @akohlmey
tools/swig/* @akohlmey
tools/lammps-shell/* @akohlmey
tools/msi2lmp/* @akohlmey
tools/offline/* @rbberger
tools/singularity/* @akohlmey @rbberger
tools/swig/* @akohlmey
tools/valgrind/* @akohlmey
tools/vim/* @hammondkd
# tests
unittest/* @akohlmey @rbberger
unittest/* @akohlmey
# cmake
cmake/* @junghans @rbberger
cmake/Modules/LAMMPSInterfacePlugin.cmake @akohlmey
cmake/Modules/MPI4WIN.cmake @akohlmey
cmake/Modules/OpenCLLoader.cmake @akohlmey
cmake/Modules/Packages/COLVARS.cmake @junghans @rbberger @giacomofiorin
cmake/Modules/Packages/KIM.cmake @junghans @rbberger @ellio167
cmake/presets/*.cmake @akohlmey
@ -149,13 +161,12 @@ cmake/presets/*.cmake @akohlmey
python/* @rbberger
# fortran
fortran/* @akohlmey
fortran/* @akohlmey @hammondkd
# docs
doc/utils/*/* @rbberger
doc/Makefile @rbberger
doc/README @rbberger
doc/* @akohlmey
examples/plugin/* @akohlmey
examples/PACKAGES/pace/plugin/* @akohlmey
# for releases
src/version.h @sjplimp

7
.github/ISSUE_TEMPLATE/help_request.md vendored
View File

@ -1,6 +1,6 @@
---
name: Request for Help
about: "Don't post help requests here, email the lammps-users mailing list"
about: "Don't post help requests here, post in the LAMMPS forum"
title: ""
labels: invalid
assignees: ''
@ -8,8 +8,9 @@ assignees: ''
---
Please **do not** post requests for help (e.g. with installing or using LAMMPS) here.
Instead send an e-mail to the lammps-users mailing list.
Instead, you can post to the LAMMPS category in the Materials Science Community
Discourse forum at: https://matsci.org/lammps/
This issue tracker is for tracking LAMMPS development related issues only.
Thanks for your cooperation.
Thank you in advance for your cooperation.

8
.github/workflows/compile-msvc.yml vendored
View File

@ -26,15 +26,19 @@ jobs:
- name: Select Python version
uses: actions/setup-python@v4
with:
python-version: '3.10'
python-version: '3.11'
- name: Building LAMMPS via CMake
shell: bash
run: |
python3 -m pip install numpy
python3 -m pip install pyyaml
nuget install MSMPIsdk
nuget install MSMPIDIST
cmake -C cmake/presets/windows.cmake \
-D PKG_PYTHON=on \
-D WITH_PNG=off \
-D WITH_JPEG=off \
-S cmake -B build \
-D BUILD_SHARED_LIBS=on \
-D LAMMPS_EXCEPTIONS=on \
@ -50,4 +54,4 @@ jobs:
- name: Run Unit Tests
working-directory: build
shell: bash
run: ctest -V -C Release
run: ctest -V -C Release -E FixTimestep:python_move_nve

4
README
View File

@ -16,8 +16,8 @@ National Laboratories, a US Department of Energy facility, with
funding from the DOE. It is an open-source code, distributed freely
under the terms of the GNU Public License (GPL) version 2.
The primary author of the code is Steve Plimpton, who can be emailed
at sjplimp@sandia.gov. The LAMMPS WWW Site at www.lammps.org has
The code is maintained by the LAMMPS development team who can be emailed
at developers@lammps.org. The LAMMPS WWW Site at www.lammps.org has
more information about the code and its uses.
The LAMMPS distribution includes the following files and directories:

54
cmake/CMakeLists.txt
View File

@ -7,6 +7,10 @@ cmake_minimum_required(VERSION 3.10)
if(POLICY CMP0074)
cmake_policy(SET CMP0074 NEW)
endif()
# set policy to silence warnings about ignoring ${CMAKE_REQUIRED_LIBRARIES} but use it
if(POLICY CMP0075)
cmake_policy(SET CMP0075 NEW)
endif()
# set policy to silence warnings about missing executable permissions in
# pythonx.y-config when cross-compiling. review occasionally if it may be set to NEW
if(POLICY CMP0109)
@ -262,6 +266,7 @@ set(STANDARD_PACKAGES
ML-QUIP
ML-RANN
ML-SNAP
ML-POD
MOFFF
MOLECULE
MOLFILE
@ -312,6 +317,15 @@ if(PKG_ADIOS)
# script that defines the MPI::MPI_C target
enable_language(C)
find_package(ADIOS2 REQUIRED)
if(BUILD_MPI)
if(NOT ADIOS2_HAVE_MPI)
message(FATAL_ERROR "ADIOS2 must be built with MPI support when LAMMPS has MPI enabled")
endif()
else()
if(ADIOS2_HAVE_MPI)
message(FATAL_ERROR "ADIOS2 must be built without MPI support when LAMMPS has MPI disabled")
endif()
endif()
target_link_libraries(lammps PRIVATE adios2::adios2)
endif()
@ -385,9 +399,9 @@ pkg_depends(EXTRA-MOLECULE MOLECULE)
# detect if we may enable OpenMP support by default
set(BUILD_OMP_DEFAULT OFF)
find_package(OpenMP QUIET)
if(OpenMP_FOUND)
check_include_file_cxx(omp.h HAVE_OMP_H_INCLUDE)
find_package(OpenMP COMPONENTS CXX QUIET)
if(OpenMP_CXX_FOUND)
check_omp_h_include()
if(HAVE_OMP_H_INCLUDE)
set(BUILD_OMP_DEFAULT ON)
endif()
@ -396,8 +410,8 @@ endif()
option(BUILD_OMP "Build with OpenMP support" ${BUILD_OMP_DEFAULT})
if(BUILD_OMP)
find_package(OpenMP REQUIRED)
check_include_file_cxx(omp.h HAVE_OMP_H_INCLUDE)
find_package(OpenMP COMPONENTS CXX REQUIRED)
check_omp_h_include()
if(NOT HAVE_OMP_H_INCLUDE)
message(FATAL_ERROR "Cannot find the 'omp.h' header file required for full OpenMP support")
endif()
@ -419,7 +433,7 @@ if(BUILD_OMP)
target_link_libraries(lmp PRIVATE OpenMP::OpenMP_CXX)
endif()
if(PKG_MSCG OR PKG_ATC OR PKG_AWPMD OR PKG_ML-QUIP OR PKG_LATTE OR PKG_ELECTRODE)
if(PKG_MSCG OR PKG_ATC OR PKG_AWPMD OR PKG_ML-QUIP OR PKG_ML-POD OR PKG_LATTE OR PKG_ELECTRODE)
enable_language(C)
if (NOT USE_INTERNAL_LINALG)
find_package(LAPACK)
@ -625,7 +639,7 @@ foreach(PKG_LIB POEMS ATC AWPMD H5MD MESONT)
endif()
endforeach()
if(PKG_ELECTRODE)
if(PKG_ELECTRODE OR PKG_ML-POD)
target_link_libraries(lammps PRIVATE ${LAPACK_LIBRARIES})
endif()
@ -654,7 +668,7 @@ endif()
# packages which selectively include variants based on enabled styles
# e.g. accelerator packages
######################################################################
foreach(PKG_WITH_INCL CORESHELL DPD-SMOOTH MISC PHONON QEQ OPENMP KOKKOS OPT INTEL GPU)
foreach(PKG_WITH_INCL CORESHELL DPD-SMOOTH MC MISC PHONON QEQ OPENMP KOKKOS OPT INTEL GPU)
if(PKG_${PKG_WITH_INCL})
include(Packages/${PKG_WITH_INCL})
endif()
@ -727,18 +741,17 @@ list(FIND LANGUAGES "Fortran" _index)
if(_index GREATER -1)
target_link_libraries(lammps PRIVATE ${CMAKE_Fortran_IMPLICIT_LINK_LIBRARIES})
endif()
set(LAMMPS_CXX_HEADERS angle.h atom.h bond.h citeme.h comm.h compute.h dihedral.h domain.h error.h fix.h force.h group.h improper.h
input.h info.h kspace.h lammps.h lattice.h library.h lmppython.h lmptype.h memory.h modify.h neighbor.h neigh_list.h output.h
pair.h pointers.h region.h timer.h universe.h update.h utils.h variable.h)
if(LAMMPS_EXCEPTIONS)
list(APPEND LAMMPS_CXX_HEADERS exceptions.h)
endif()
set(LAMMPS_CXX_HEADERS angle.h atom.h bond.h citeme.h comm.h command.h compute.h dihedral.h domain.h
error.h exceptions.h fix.h force.h group.h improper.h input.h info.h kspace.h lammps.h lattice.h
library.h lmppython.h lmptype.h memory.h modify.h neighbor.h neigh_list.h output.h pair.h
platform.h pointers.h region.h timer.h universe.h update.h utils.h variable.h)
set(LAMMPS_FMT_HEADERS core.h format.h)
set_target_properties(lammps PROPERTIES OUTPUT_NAME lammps${LAMMPS_MACHINE})
set_target_properties(lammps PROPERTIES SOVERSION ${SOVERSION})
set_target_properties(lammps PROPERTIES PREFIX "lib")
target_include_directories(lammps PUBLIC $<INSTALL_INTERFACE:${CMAKE_INSTALL_INCLUDEDIR}/lammps>)
file(MAKE_DIRECTORY ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps)
file(MAKE_DIRECTORY ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/fmt)
foreach(_HEADER ${LAMMPS_CXX_HEADERS})
add_custom_command(OUTPUT ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/${_HEADER} COMMAND ${CMAKE_COMMAND} -E copy_if_different ${LAMMPS_SOURCE_DIR}/${_HEADER} ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/${_HEADER} DEPENDS ${LAMMPS_SOURCE_DIR}/${_HEADER})
add_custom_target(${_HEADER} DEPENDS ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/${_HEADER})
@ -747,6 +760,14 @@ foreach(_HEADER ${LAMMPS_CXX_HEADERS})
install(FILES ${LAMMPS_SOURCE_DIR}/${_HEADER} DESTINATION ${CMAKE_INSTALL_INCLUDEDIR}/lammps)
endif()
endforeach()
foreach(_HEADER ${LAMMPS_FMT_HEADERS})
add_custom_command(OUTPUT ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/fmt/${_HEADER} COMMAND ${CMAKE_COMMAND} -E copy_if_different ${LAMMPS_SOURCE_DIR}/fmt/${_HEADER} ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/fmt/${_HEADER} DEPENDS ${LAMMPS_SOURCE_DIR}/fmt/${_HEADER})
add_custom_target(fmt_${_HEADER} DEPENDS ${CMAKE_CURRENT_BINARY_DIR}/includes/lammps/fmt/${_HEADER})
add_dependencies(lammps fmt_${_HEADER})
if(BUILD_SHARED_LIBS)
install(FILES ${LAMMPS_SOURCE_DIR}/fmt/${_HEADER} DESTINATION ${CMAKE_INSTALL_INCLUDEDIR}/lammps/fmt)
endif()
endforeach()
target_include_directories(lammps INTERFACE $<BUILD_INTERFACE:${CMAKE_CURRENT_BINARY_DIR}/includes>)
add_library(LAMMPS::lammps ALIAS lammps)
get_target_property(LAMMPS_DEFINES lammps INTERFACE_COMPILE_DEFINITIONS)
@ -969,9 +990,6 @@ if(PKG_GPU)
endif()
message(STATUS "GPU precision: ${GPU_PREC}")
endif()
if(PKG_KOKKOS)
message(STATUS "Kokkos Arch: ${KOKKOS_ARCH}")
endif()
if(PKG_KSPACE)
message(STATUS "<<< FFT settings >>>
-- Primary FFT lib: ${FFT}")

29
cmake/Modules/FindClangFormat.cmake
View File

@ -1,5 +1,10 @@
# Find clang-format
find_program(ClangFormat_EXECUTABLE NAMES clang-format
clang-format-15.0
clang-format-14.0
clang-format-13.0
clang-format-12.0
clang-format-11.0
clang-format-10.0
clang-format-9.0
clang-format-8.0
@ -14,19 +19,27 @@ if(ClangFormat_EXECUTABLE)
OUTPUT_VARIABLE clang_format_version
ERROR_QUIET OUTPUT_STRIP_TRAILING_WHITESPACE)
if(clang_format_version MATCHES "^clang-format version .*")
# Arch Linux
if(clang_format_version MATCHES "^(Ubuntu |)clang-format version .*")
# Arch Linux output:
# clang-format version 10.0.0
# Ubuntu 18.04 LTS Output
#
# Ubuntu 18.04 LTS output:
# clang-format version 6.0.0-1ubuntu2 (tags/RELEASE_600/final)
string(REGEX REPLACE "clang-format version ([0-9.]+).*"
"\\1"
#
# Ubuntu 20.04 LTS output:
# clang-format version 10.0.0-4ubuntu1
#
# Ubuntu 22.04 LTS output:
# Ubuntu clang-format version 14.0.0-1ubuntu1
#
# Fedora 36 output:
# clang-format version 14.0.5 (Fedora 14.0.5-1.fc36)
string(REGEX REPLACE "^(Ubuntu |)clang-format version ([0-9.]+).*"
"\\2"
ClangFormat_VERSION
"${clang_format_version}")
elseif(clang_format_version MATCHES ".*LLVM version .*")
# CentOS 7 Output
# CentOS 7 output:
# LLVM (http://llvm.org/):
# LLVM version 3.4.2
# Optimized build.

2
cmake/Modules/FindCythonize.cmake
View File

@ -22,7 +22,7 @@ endif()
if(Python_EXECUTABLE)
get_filename_component(_python_path ${Python_EXECUTABLE} PATH)
find_program(Cythonize_EXECUTABLE
NAMES cythonize3 cythonize cythonize.bat
NAMES cythonize-${Python_VERSION_MAJOR}.${Python_VERSION_MINOR} cythonize3 cythonize cythonize.bat
HINTS ${_python_path})
endif()

19
cmake/Modules/FindZMQ.cmake
View File

@ -1,19 +0,0 @@
find_path(ZMQ_INCLUDE_DIR zmq.h)
find_library(ZMQ_LIBRARY NAMES zmq)
include(FindPackageHandleStandardArgs)
find_package_handle_standard_args(ZMQ DEFAULT_MSG ZMQ_LIBRARY ZMQ_INCLUDE_DIR)
# Copy the results to the output variables and target.
if(ZMQ_FOUND)
set(ZMQ_LIBRARIES ${ZMQ_LIBRARY})
set(ZMQ_INCLUDE_DIRS ${ZMQ_INCLUDE_DIR})
if(NOT TARGET ZMQ::ZMQ)
add_library(ZMQ::ZMQ UNKNOWN IMPORTED)
set_target_properties(ZMQ::ZMQ PROPERTIES
IMPORTED_LINK_INTERFACE_LANGUAGES "C"
IMPORTED_LOCATION "${ZMQ_LIBRARY}"
INTERFACE_INCLUDE_DIRECTORIES "${ZMQ_INCLUDE_DIR}")
endif()
endif()

103
cmake/Modules/LAMMPSInterfacePlugin.cmake
View File

@ -112,45 +112,76 @@ if(BUILD_MPI)
set(MPI_CXX_SKIP_MPICXX TRUE)
# We use a non-standard procedure to cross-compile with MPI on Windows
if((CMAKE_SYSTEM_NAME STREQUAL "Windows") AND CMAKE_CROSSCOMPILING)
# Download and configure custom MPICH files for Windows
message(STATUS "Downloading and configuring MPICH-1.4.1 for Windows")
set(MPICH2_WIN64_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win64-devel.tar.gz" CACHE STRING "URL for MPICH2 (win64) tarball")
set(MPICH2_WIN32_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win32-devel.tar.gz" CACHE STRING "URL for MPICH2 (win32) tarball")
set(MPICH2_WIN64_DEVEL_MD5 "4939fdb59d13182fd5dd65211e469f14" CACHE STRING "MD5 checksum of MPICH2 (win64) tarball")
set(MPICH2_WIN32_DEVEL_MD5 "a61d153500dce44e21b755ee7257e031" CACHE STRING "MD5 checksum of MPICH2 (win32) tarball")
mark_as_advanced(MPICH2_WIN64_DEVEL_URL)
mark_as_advanced(MPICH2_WIN32_DEVEL_URL)
mark_as_advanced(MPICH2_WIN64_DEVEL_MD5)
mark_as_advanced(MPICH2_WIN32_DEVEL_MD5)
# Download and configure MinGW compatible MPICH development files for Windows
option(USE_MSMPI "Use Microsoft's MS-MPI SDK instead of MPICH2-1.4.1" OFF)
if(USE_MSMPI)
message(STATUS "Downloading and configuring MS-MPI 10.1 for Windows cross-compilation")
set(MPICH2_WIN64_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/msmpi-win64-devel.tar.gz" CACHE STRING "URL for MS-MPI (win64) tarball")
set(MPICH2_WIN64_DEVEL_MD5 "86314daf1bffb809f1fcbefb8a547490" CACHE STRING "MD5 checksum of MS-MPI (win64) tarball")
mark_as_advanced(MPICH2_WIN64_DEVEL_URL)
mark_as_advanced(MPICH2_WIN64_DEVEL_MD5)
include(ExternalProject)
if(CMAKE_SYSTEM_PROCESSOR STREQUAL "x86_64")
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN64_DEVEL_URL}
URL_MD5 ${MPICH2_WIN64_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
include(ExternalProject)
if(CMAKE_SYSTEM_PROCESSOR STREQUAL "x86_64")
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN64_DEVEL_URL}
URL_MD5 ${MPICH2_WIN64_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmsmpi.a)
else()
message(FATAL_ERROR "Only x86 64-bit builds are supported with MS-MPI")
endif()
ExternalProject_get_property(mpi4win_build SOURCE_DIR)
file(MAKE_DIRECTORY "${SOURCE_DIR}/include")
add_library(MPI::MPI_CXX UNKNOWN IMPORTED)
set_target_properties(MPI::MPI_CXX PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/lib/libmsmpi.a"
INTERFACE_INCLUDE_DIRECTORIES "${SOURCE_DIR}/include"
INTERFACE_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
add_dependencies(MPI::MPI_CXX mpi4win_build)
# set variables for status reporting at the end of CMake run
set(MPI_CXX_INCLUDE_PATH "${SOURCE_DIR}/include")
set(MPI_CXX_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
set(MPI_CXX_LIBRARIES "${SOURCE_DIR}/lib/libmsmpi.a")
else()
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN32_DEVEL_URL}
URL_MD5 ${MPICH2_WIN32_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
# Download and configure custom MPICH files for Windows
message(STATUS "Downloading and configuring MPICH-1.4.1 for Windows")
set(MPICH2_WIN64_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win64-devel.tar.gz" CACHE STRING "URL for MPICH2 (win64) tarball")
set(MPICH2_WIN64_DEVEL_MD5 "4939fdb59d13182fd5dd65211e469f14" CACHE STRING "MD5 checksum of MPICH2 (win64) tarball")
mark_as_advanced(MPICH2_WIN64_DEVEL_URL)
mark_as_advanced(MPICH2_WIN64_DEVEL_MD5)
include(ExternalProject)
if(CMAKE_SYSTEM_PROCESSOR STREQUAL "x86_64")
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN64_DEVEL_URL}
URL_MD5 ${MPICH2_WIN64_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
else()
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN32_DEVEL_URL}
URL_MD5 ${MPICH2_WIN32_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
endif()
ExternalProject_get_property(mpi4win_build SOURCE_DIR)
file(MAKE_DIRECTORY "${SOURCE_DIR}/include")
add_library(MPI::MPI_CXX UNKNOWN IMPORTED)
set_target_properties(MPI::MPI_CXX PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/lib/libmpi.a"
INTERFACE_INCLUDE_DIRECTORIES "${SOURCE_DIR}/include"
INTERFACE_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
add_dependencies(MPI::MPI_CXX mpi4win_build)
# set variables for status reporting at the end of CMake run
set(MPI_CXX_INCLUDE_PATH "${SOURCE_DIR}/include")
set(MPI_CXX_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
set(MPI_CXX_LIBRARIES "${SOURCE_DIR}/lib/libmpi.a")
endif()
ExternalProject_get_property(mpi4win_build SOURCE_DIR)
file(MAKE_DIRECTORY "${SOURCE_DIR}/include")
add_library(MPI::MPI_CXX UNKNOWN IMPORTED)
set_target_properties(MPI::MPI_CXX PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/lib/libmpi.a"
INTERFACE_INCLUDE_DIRECTORIES "${SOURCE_DIR}/include"
INTERFACE_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
add_dependencies(MPI::MPI_CXX mpi4win_build)
# set variables for status reporting at the end of CMake run
set(MPI_CXX_INCLUDE_PATH "${SOURCE_DIR}/include")
set(MPI_CXX_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
set(MPI_CXX_LIBRARIES "${SOURCE_DIR}/lib/libmpi.a")
else()
find_package(MPI REQUIRED)
option(LAMMPS_LONGLONG_TO_LONG "Workaround if your system or MPI version does not recognize 'long long' data types" OFF)

15
cmake/Modules/LAMMPSUtils.cmake
View File

@ -24,6 +24,21 @@ function(validate_option name values)
endif()
endfunction(validate_option)
# helper function to check for usable omp.h header
function(check_omp_h_include)
find_package(OpenMP COMPONENTS CXX QUIET)
if(OpenMP_CXX_FOUND)
set(CMAKE_REQUIRED_FLAGS ${OpenMP_CXX_FLAGS})
set(CMAKE_REQUIRED_INCLUDES ${OpenMP_CXX_INCLUDE_DIRS})
set(CMAKE_REQUIRED_LINK_OPTIONS ${OpenMP_CXX_FLAGS})
set(CMAKE_REQUIRED_LIBRARIES ${OpenMP_CXX_LIBRARIES})
check_include_file_cxx(omp.h _have_omp_h)
else()
set(_have_omp_h FALSE)
endif()
set(HAVE_OMP_H_INCLUDE ${_have_omp_h} PARENT_SCOPE)
endfunction()
# helper function for getting the most recently modified file or folder from a glob pattern
function(get_newest_file path variable)
file(GLOB _dirs ${path})

107
cmake/Modules/MPI4WIN.cmake
View File

@ -1,39 +1,74 @@
# Download and configure custom MPICH files for Windows
message(STATUS "Downloading and configuring MPICH-1.4.1 for Windows")
set(MPICH2_WIN64_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win64-devel.tar.gz" CACHE STRING "URL for MPICH2 (win64) tarball")
set(MPICH2_WIN32_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win32-devel.tar.gz" CACHE STRING "URL for MPICH2 (win32) tarball")
set(MPICH2_WIN64_DEVEL_MD5 "4939fdb59d13182fd5dd65211e469f14" CACHE STRING "MD5 checksum of MPICH2 (win64) tarball")
set(MPICH2_WIN32_DEVEL_MD5 "a61d153500dce44e21b755ee7257e031" CACHE STRING "MD5 checksum of MPICH2 (win32) tarball")
mark_as_advanced(MPICH2_WIN64_DEVEL_URL)
mark_as_advanced(MPICH2_WIN32_DEVEL_URL)
mark_as_advanced(MPICH2_WIN64_DEVEL_MD5)
mark_as_advanced(MPICH2_WIN32_DEVEL_MD5)
# Download and configure MinGW compatible MPICH development files for Windows
option(USE_MSMPI "Use Microsoft's MS-MPI SDK instead of MPICH2-1.4.1" OFF)
include(ExternalProject)
if(CMAKE_SYSTEM_PROCESSOR STREQUAL "x86_64")
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN64_DEVEL_URL}
URL_MD5 ${MPICH2_WIN64_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
if(USE_MSMPI)
message(STATUS "Downloading and configuring MS-MPI 10.1 for Windows cross-compilation")
set(MPICH2_WIN64_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/msmpi-win64-devel.tar.gz" CACHE STRING "URL for MS-MPI (win64) tarball")
set(MPICH2_WIN64_DEVEL_MD5 "86314daf1bffb809f1fcbefb8a547490" CACHE STRING "MD5 checksum of MS-MPI (win64) tarball")
mark_as_advanced(MPICH2_WIN64_DEVEL_URL)
mark_as_advanced(MPICH2_WIN64_DEVEL_MD5)
include(ExternalProject)
if(CMAKE_SYSTEM_PROCESSOR STREQUAL "x86_64")
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN64_DEVEL_URL}
URL_MD5 ${MPICH2_WIN64_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmsmpi.a)
else()
message(FATAL_ERROR "Only x86 64-bit builds are supported with MS-MPI")
endif()
ExternalProject_get_property(mpi4win_build SOURCE_DIR)
file(MAKE_DIRECTORY "${SOURCE_DIR}/include")
add_library(MPI::MPI_CXX UNKNOWN IMPORTED)
set_target_properties(MPI::MPI_CXX PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/lib/libmsmpi.a"
INTERFACE_INCLUDE_DIRECTORIES "${SOURCE_DIR}/include"
INTERFACE_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
add_dependencies(MPI::MPI_CXX mpi4win_build)
# set variables for status reporting at the end of CMake run
set(MPI_CXX_INCLUDE_PATH "${SOURCE_DIR}/include")
set(MPI_CXX_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
set(MPI_CXX_LIBRARIES "${SOURCE_DIR}/lib/libmsmpi.a")
else()
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN32_DEVEL_URL}
URL_MD5 ${MPICH2_WIN32_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
message(STATUS "Downloading and configuring MPICH2-1.4.1 for Windows cross-compilation")
set(MPICH2_WIN64_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win64-devel.tar.gz" CACHE STRING "URL for MPICH2 (win64) tarball")
set(MPICH2_WIN32_DEVEL_URL "${LAMMPS_THIRDPARTY_URL}/mpich2-win32-devel.tar.gz" CACHE STRING "URL for MPICH2 (win32) tarball")
set(MPICH2_WIN64_DEVEL_MD5 "4939fdb59d13182fd5dd65211e469f14" CACHE STRING "MD5 checksum of MPICH2 (win64) tarball")
set(MPICH2_WIN32_DEVEL_MD5 "a61d153500dce44e21b755ee7257e031" CACHE STRING "MD5 checksum of MPICH2 (win32) tarball")
mark_as_advanced(MPICH2_WIN64_DEVEL_URL)
mark_as_advanced(MPICH2_WIN32_DEVEL_URL)
mark_as_advanced(MPICH2_WIN64_DEVEL_MD5)
mark_as_advanced(MPICH2_WIN32_DEVEL_MD5)
include(ExternalProject)
if(CMAKE_SYSTEM_PROCESSOR STREQUAL "x86_64")
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN64_DEVEL_URL}
URL_MD5 ${MPICH2_WIN64_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
else()
ExternalProject_Add(mpi4win_build
URL ${MPICH2_WIN32_DEVEL_URL}
URL_MD5 ${MPICH2_WIN32_DEVEL_MD5}
CONFIGURE_COMMAND "" BUILD_COMMAND "" INSTALL_COMMAND ""
BUILD_BYPRODUCTS <SOURCE_DIR>/lib/libmpi.a)
endif()
ExternalProject_get_property(mpi4win_build SOURCE_DIR)
file(MAKE_DIRECTORY "${SOURCE_DIR}/include")
add_library(MPI::MPI_CXX UNKNOWN IMPORTED)
set_target_properties(MPI::MPI_CXX PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/lib/libmpi.a"
INTERFACE_INCLUDE_DIRECTORIES "${SOURCE_DIR}/include"
INTERFACE_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
add_dependencies(MPI::MPI_CXX mpi4win_build)
# set variables for status reporting at the end of CMake run
set(MPI_CXX_INCLUDE_PATH "${SOURCE_DIR}/include")
set(MPI_CXX_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
set(MPI_CXX_LIBRARIES "${SOURCE_DIR}/lib/libmpi.a")
endif()
ExternalProject_get_property(mpi4win_build SOURCE_DIR)
file(MAKE_DIRECTORY "${SOURCE_DIR}/include")
add_library(MPI::MPI_CXX UNKNOWN IMPORTED)
set_target_properties(MPI::MPI_CXX PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/lib/libmpi.a"
INTERFACE_INCLUDE_DIRECTORIES "${SOURCE_DIR}/include"
INTERFACE_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
add_dependencies(MPI::MPI_CXX mpi4win_build)
# set variables for status reporting at the end of CMake run
set(MPI_CXX_INCLUDE_PATH "${SOURCE_DIR}/include")
set(MPI_CXX_COMPILE_DEFINITIONS "MPICH_SKIP_MPICXX")
set(MPI_CXX_LIBRARIES "${SOURCE_DIR}/lib/libmpi.a")

13
cmake/Modules/Packages/KOKKOS.cmake
View File

@ -15,8 +15,9 @@ if(Kokkos_ENABLE_OPENMP)
if(NOT BUILD_OMP)
message(FATAL_ERROR "Must enable BUILD_OMP with Kokkos_ENABLE_OPENMP")
else()
if(LAMMPS_OMP_COMPAT_LEVEL LESS 4)
message(FATAL_ERROR "Compiler must support OpenMP 4.0 or later with Kokkos_ENABLE_OPENMP")
# NVHPC does not seem to provide a detectable OpenMP version, but is far beyond version 3.1
if((OpenMP_CXX_VERSION VERSION_LESS 3.1) AND NOT (CMAKE_CXX_COMPILER_ID STREQUAL "NVHPC"))
message(FATAL_ERROR "Compiler must support OpenMP 3.1 or later with Kokkos_ENABLE_OPENMP")
endif()
endif()
endif()
@ -123,7 +124,7 @@ set(KOKKOS_PKG_SOURCES ${KOKKOS_PKG_SOURCES_DIR}/kokkos.cpp
if(PKG_KSPACE)
list(APPEND KOKKOS_PKG_SOURCES ${KOKKOS_PKG_SOURCES_DIR}/fft3d_kokkos.cpp
${KOKKOS_PKG_SOURCES_DIR}/gridcomm_kokkos.cpp
${KOKKOS_PKG_SOURCES_DIR}/grid3d_kokkos.cpp
${KOKKOS_PKG_SOURCES_DIR}/remap_kokkos.cpp)
if(Kokkos_ENABLE_CUDA)
if(NOT (FFT STREQUAL "KISS"))
@ -138,6 +139,12 @@ if(PKG_KSPACE)
endif()
endif()
if(PKG_ML-IAP)
list(APPEND KOKKOS_PKG_SOURCES ${KOKKOS_PKG_SOURCES_DIR}/mliap_data_kokkos.cpp
${KOKKOS_PKG_SOURCES_DIR}/mliap_descriptor_so3_kokkos.cpp
${KOKKOS_PKG_SOURCES_DIR}/mliap_model_linear_kokkos.cpp
${KOKKOS_PKG_SOURCES_DIR}/mliap_so3_kokkos.cpp)
endif()
if(PKG_PHONON)
list(APPEND KOKKOS_PKG_SOURCES ${KOKKOS_PKG_SOURCES_DIR}/dynamical_matrix_kokkos.cpp)

9
cmake/Modules/Packages/MC.cmake Normal file
View File

@ -0,0 +1,9 @@
# fix sgcmc may only be installed if also the EAM pair style from MANYBODY is installed
if(NOT PKG_MANYBODY)
get_property(LAMMPS_FIX_HEADERS GLOBAL PROPERTY FIX)
list(REMOVE_ITEM LAMMPS_FIX_HEADERS ${LAMMPS_SOURCE_DIR}/MC/fix_sgcmc.h)
set_property(GLOBAL PROPERTY FIX "${LAMMPS_FIX_HEADERS}")
get_target_property(LAMMPS_SOURCES lammps SOURCES)
list(REMOVE_ITEM LAMMPS_SOURCES ${LAMMPS_SOURCE_DIR}/MC/fix_sgcmc.cpp)
set_property(TARGET lammps PROPERTY SOURCES "${LAMMPS_SOURCES}")
endif()

11
cmake/Modules/Packages/ML-IAP.cmake
View File

@ -2,7 +2,13 @@
set(MLIAP_ENABLE_PYTHON_DEFAULT OFF)
if(PKG_PYTHON)
find_package(Cythonize QUIET)
if(Cythonize_FOUND)
if (CMAKE_VERSION VERSION_GREATER_EQUAL 3.14)
find_package(Python COMPONENTS NumPy QUIET)
else()
# assume we have NumPy
set(Python_NumPy_FOUND ON)
endif()
if(Cythonize_FOUND AND Python_NumPy_FOUND)
set(MLIAP_ENABLE_PYTHON_DEFAULT ON)
endif()
endif()
@ -11,6 +17,9 @@ option(MLIAP_ENABLE_PYTHON "Build ML-IAP package with Python support" ${MLIAP_EN
if(MLIAP_ENABLE_PYTHON)
find_package(Cythonize REQUIRED)
if (CMAKE_VERSION VERSION_GREATER_EQUAL 3.14)
find_package(Python COMPONENTS NumPy REQUIRED)
endif()
if(NOT PKG_PYTHON)
message(FATAL_ERROR "Must enable PYTHON package for including Python support in ML-IAP")
endif()

4
cmake/Modules/Packages/ML-QUIP.cmake
View File

@ -58,12 +58,12 @@ if(DOWNLOAD_QUIP)
BUILD_COMMAND env QUIP_ARCH=lammps make libquip
INSTALL_COMMAND ""
BUILD_IN_SOURCE YES
BUILD_BYPRODUCTS <SOURCE_DIR>/build/lammps/libquip.a
BUILD_BYPRODUCTS <SOURCE_DIR>/build/lammps/${CMAKE_STATIC_LIBRARY_PREFIX}quip${CMAKE_STATIC_LIBRARY_SUFFIX}
)
ExternalProject_get_property(quip_build SOURCE_DIR)
add_library(LAMMPS::QUIP UNKNOWN IMPORTED)
set_target_properties(LAMMPS::QUIP PROPERTIES
IMPORTED_LOCATION "${SOURCE_DIR}/build/lammps/libquip.a"
IMPORTED_LOCATION "${SOURCE_DIR}/build/lammps/${CMAKE_STATIC_LIBRARY_PREFIX}quip${CMAKE_STATIC_LIBRARY_SUFFIX}"
INTERFACE_LINK_LIBRARIES "${LAPACK_LIBRARIES}")
target_link_libraries(lammps PRIVATE LAMMPS::QUIP)
add_dependencies(LAMMPS::QUIP quip_build)

20
cmake/Modules/Packages/PLUMED.cmake
View File

@ -47,15 +47,15 @@ if(DOWNLOAD_PLUMED)
endif()
message(STATUS "PLUMED download requested - we will build our own")
if(PLUMED_MODE STREQUAL "STATIC")
set(PLUMED_BUILD_BYPRODUCTS "<INSTALL_DIR>/lib/libplumed.a")
set(PLUMED_BUILD_BYPRODUCTS "<INSTALL_DIR>/lib/${CMAKE_STATIC_LIBRARY_PREFIX}plumed${CMAKE_STATIC_LIBRARY_SUFFIX}")
elseif(PLUMED_MODE STREQUAL "SHARED")
set(PLUMED_BUILD_BYPRODUCTS "<INSTALL_DIR>/lib/libplumed${CMAKE_SHARED_LIBRARY_SUFFIX};<INSTALL_DIR>/lib/libplumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX}")
set(PLUMED_BUILD_BYPRODUCTS "<INSTALL_DIR>/lib/${CMAKE_SHARED_LIBRARY_PREFIX}plumed${CMAKE_SHARED_LIBRARY_SUFFIX};<INSTALL_DIR>/lib/${CMAKE_SHARED_LIBRARY_PREFIX}plumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX}")
elseif(PLUMED_MODE STREQUAL "RUNTIME")
set(PLUMED_BUILD_BYPRODUCTS "<INSTALL_DIR>/lib/libplumedWrapper.a")
set(PLUMED_BUILD_BYPRODUCTS "<INSTALL_DIR>/lib/${CMAKE_STATIC_LIBRARY_PREFIX}plumedWrapper${CMAKE_STATIC_LIBRARY_PREFIX}")
endif()
set(PLUMED_URL "https://github.com/plumed/plumed2/releases/download/v2.7.4/plumed-src-2.7.4.tgz" CACHE STRING "URL for PLUMED tarball")
set(PLUMED_MD5 "858e0b6aed173748fc85b6bc8a9dcb3e" CACHE STRING "MD5 checksum of PLUMED tarball")
set(PLUMED_URL "https://github.com/plumed/plumed2/releases/download/v2.8.1/plumed-src-2.8.1.tgz" CACHE STRING "URL for PLUMED tarball")
set(PLUMED_MD5 "6bfe72ebdae63dc38a9ca27d9b0e08f8" CACHE STRING "MD5 checksum of PLUMED tarball")
mark_as_advanced(PLUMED_URL)
mark_as_advanced(PLUMED_MD5)
@ -78,12 +78,12 @@ if(DOWNLOAD_PLUMED)
add_library(LAMMPS::PLUMED UNKNOWN IMPORTED)
add_dependencies(LAMMPS::PLUMED plumed_build)
if(PLUMED_MODE STREQUAL "STATIC")
set_target_properties(LAMMPS::PLUMED PROPERTIES IMPORTED_LOCATION ${INSTALL_DIR}/lib/libplumed.a INTERFACE_LINK_LIBRARIES "${PLUMED_LINK_LIBS};${CMAKE_DL_LIBS}")
set_target_properties(LAMMPS::PLUMED PROPERTIES IMPORTED_LOCATION ${INSTALL_DIR}/lib/${CMAKE_STATIC_LIBRARY_PREFIX}plumed${CMAKE_STATIC_LIBRARY_SUFFIX} INTERFACE_LINK_LIBRARIES "${PLUMED_LINK_LIBS};${CMAKE_DL_LIBS}")
elseif(PLUMED_MODE STREQUAL "SHARED")
set_target_properties(LAMMPS::PLUMED PROPERTIES IMPORTED_LOCATION ${INSTALL_DIR}/lib/libplumed${CMAKE_SHARED_LIBRARY_SUFFIX} INTERFACE_LINK_LIBRARIES "${INSTALL_DIR}/lib/libplumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX};${CMAKE_DL_LIBS}")
set_target_properties(LAMMPS::PLUMED PROPERTIES IMPORTED_LOCATION ${INSTALL_DIR}/lib/${CMAKE_SHARED_LIBRARY_PREFIX}plumed${CMAKE_SHARED_LIBRARY_SUFFIX} INTERFACE_LINK_LIBRARIES "${INSTALL_DIR}/lib/${CMAKE_SHARED_LIBRARY_PREFIX}plumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX};${CMAKE_DL_LIBS}")
elseif(PLUMED_MODE STREQUAL "RUNTIME")
set_target_properties(LAMMPS::PLUMED PROPERTIES INTERFACE_COMPILE_DEFINITIONS "__PLUMED_DEFAULT_KERNEL=${INSTALL_DIR}/lib/libplumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX}")
set_target_properties(LAMMPS::PLUMED PROPERTIES IMPORTED_LOCATION ${INSTALL_DIR}/lib/libplumedWrapper.a INTERFACE_LINK_LIBRARIES "${CMAKE_DL_LIBS}")
set_target_properties(LAMMPS::PLUMED PROPERTIES INTERFACE_COMPILE_DEFINITIONS "__PLUMED_DEFAULT_KERNEL=${INSTALL_DIR}/lib/${CMAKE_SHARED_LIBRARY_PREFIX}plumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX}")
set_target_properties(LAMMPS::PLUMED PROPERTIES IMPORTED_LOCATION ${INSTALL_DIR}/lib/${CMAKE_STATIC_LIBRARY_PREFIX}plumedWrapper${CMAKE_STATIC_LIBRARY_SUFFIX} INTERFACE_LINK_LIBRARIES "${CMAKE_DL_LIBS}")
endif()
set_target_properties(LAMMPS::PLUMED PROPERTIES INTERFACE_INCLUDE_DIRECTORIES ${INSTALL_DIR}/include)
file(MAKE_DIRECTORY ${INSTALL_DIR}/include)
@ -96,7 +96,7 @@ else()
elseif(PLUMED_MODE STREQUAL "SHARED")
include(${PLUMED_LIBDIR}/plumed/src/lib/Plumed.cmake.shared)
elseif(PLUMED_MODE STREQUAL "RUNTIME")
set_target_properties(LAMMPS::PLUMED PROPERTIES INTERFACE_COMPILE_DEFINITIONS "__PLUMED_DEFAULT_KERNEL=${PLUMED_LIBDIR}/libplumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX}")
set_target_properties(LAMMPS::PLUMED PROPERTIES INTERFACE_COMPILE_DEFINITIONS "__PLUMED_DEFAULT_KERNEL=${PLUMED_LIBDIR}/${CMAKE_SHARED_LIBRARY_PREFIX}plumedKernel${CMAKE_SHARED_LIBRARY_SUFFIX}")
include(${PLUMED_LIBDIR}/plumed/src/lib/Plumed.cmake.runtime)
endif()
set_target_properties(LAMMPS::PLUMED PROPERTIES INTERFACE_LINK_LIBRARIES "${PLUMED_LOAD}")

9
cmake/Modules/Packages/VTK.cmake
View File

@ -1,4 +1,9 @@
find_package(VTK REQUIRED NO_MODULE)
include(${VTK_USE_FILE})
target_compile_definitions(lammps PRIVATE -DLAMMPS_VTK)
target_link_libraries(lammps PRIVATE ${VTK_LIBRARIES})
if (VTK_MAJOR_VERSION VERSION_LESS 9.0)
include(${VTK_USE_FILE})
target_link_libraries(lammps PRIVATE ${VTK_LIBRARIES})
else()
target_link_libraries(lammps PRIVATE VTK::CommonCore VTK::IOCore VTK::CommonDataModel VTK::IOXML VTK::IOLegacy VTK::IOParallelXML)
vtk_module_autoinit(TARGETS lammps MODULES VTK::CommonCore VTK::IOCore VTK::CommonDataModel VTK::IOXML VTK::IOLegacy VTK::IOParallelXML)
endif()

1
cmake/presets/all_off.cmake
View File

@ -56,6 +56,7 @@ set(ALL_PACKAGES
ML-HDNNP
ML-IAP
ML-PACE
ML-POD
ML-QUIP
ML-RANN
ML-SNAP

1
cmake/presets/all_on.cmake
View File

@ -58,6 +58,7 @@ set(ALL_PACKAGES
ML-HDNNP
ML-IAP
ML-PACE
ML-POD
ML-QUIP
ML-RANN
ML-SNAP

7
cmake/presets/clang.cmake
View File

@ -28,10 +28,3 @@ set(MPI_CXX "clang++" CACHE STRING "" FORCE)
set(MPI_CXX_COMPILER "mpicxx" CACHE STRING "" FORCE)
unset(HAVE_OMP_H_INCLUDE CACHE)
set(OpenMP_C "clang" CACHE STRING "" FORCE)
set(OpenMP_C_FLAGS "-fopenmp" CACHE STRING "" FORCE)
set(OpenMP_C_LIB_NAMES "omp" CACHE STRING "" FORCE)
set(OpenMP_CXX "clang++" CACHE STRING "" FORCE)
set(OpenMP_CXX_FLAGS "-fopenmp" CACHE STRING "" FORCE)
set(OpenMP_CXX_LIB_NAMES "omp" CACHE STRING "" FORCE)
set(OpenMP_omp_LIBRARY "libomp.so" CACHE PATH "" FORCE)

8
cmake/presets/gcc.cmake
View File

@ -19,11 +19,3 @@ set(CMAKE_Fortran_FLAGS_DEBUG "-Wall -Og -g -std=f2003" CACHE STRING "" FORCE)
set(CMAKE_Fortran_FLAGS_RELWITHDEBINFO "-g -O2 -DNDEBUG -std=f2003" CACHE STRING "" FORCE)
set(CMAKE_Fortran_FLAGS_RELEASE "-O3 -DNDEBUG -std=f2003" CACHE STRING "" FORCE)
unset(HAVE_OMP_H_INCLUDE CACHE)
set(OpenMP_C "gcc" CACHE STRING "" FORCE)
set(OpenMP_C_FLAGS "-fopenmp" CACHE STRING "" FORCE)
set(OpenMP_C_LIB_NAMES "gomp" CACHE STRING "" FORCE)
set(OpenMP_CXX "g++" CACHE STRING "" FORCE)
set(OpenMP_CXX_FLAGS "-fopenmp" CACHE STRING "" FORCE)
set(OpenMP_CXX_LIB_NAMES "gomp" CACHE STRING "" FORCE)
set(OpenMP_omp_LIBRARY "libgomp.so" CACHE PATH "" FORCE)

1
cmake/presets/mingw-cross.cmake
View File

@ -47,6 +47,7 @@ set(WIN_PACKAGES
MISC
ML-HDNNP
ML-IAP
ML-POD
ML-RANN
ML-SNAP
MOFFF

1
cmake/presets/most.cmake
View File

@ -41,6 +41,7 @@ set(ALL_PACKAGES
MEAM
MISC
ML-IAP
ML-POD
ML-SNAP
MOFFF
MOLECULE

9
cmake/presets/nvhpc.cmake Normal file
View File

@ -0,0 +1,9 @@
# preset that will enable Nvidia HPC SDK compilers with support for MPI and OpenMP (on Linux boxes)
set(CMAKE_CXX_COMPILER "nvc++" CACHE STRING "" FORCE)
set(CMAKE_C_COMPILER "nvc" CACHE STRING "" FORCE)
set(CMAKE_Fortran_COMPILER "nvfortran" CACHE STRING "" FORCE)
set(MPI_CXX "nvc++" CACHE STRING "" FORCE)
set(MPI_CXX_COMPILER "mpicxx" CACHE STRING "" FORCE)
unset(HAVE_OMP_H_INCLUDE CACHE)

9
cmake/presets/pedantic.cmake
View File

@ -1,4 +1,4 @@
# preset that will restore gcc/g++ with support for MPI and OpenMP (on Linux boxes)
# preset that will set gcc/g++ with extra warnings enabled and support for MPI and OpenMP (on Linux boxes)
set(CMAKE_CXX_COMPILER "g++" CACHE STRING "" FORCE)
set(CMAKE_C_COMPILER "gcc" CACHE STRING "" FORCE)
@ -17,10 +17,3 @@ set(MPI_Fortran "gfortran" CACHE STRING "" FORCE)
set(MPI_Fortran_COMPILER "mpifort" CACHE STRING "" FORCE)
unset(HAVE_OMP_H_INCLUDE CACHE)
set(OpenMP_C "gcc" CACHE STRING "" FORCE)
set(OpenMP_C_FLAGS "-fopenmp" CACHE STRING "" FORCE)
set(OpenMP_C_LIB_NAMES "gomp" CACHE STRING "" FORCE)
set(OpenMP_CXX "g++" CACHE STRING "" FORCE)
set(OpenMP_CXX_FLAGS "-fopenmp" CACHE STRING "" FORCE)
set(OpenMP_CXX_LIB_NAMES "gomp" CACHE STRING "" FORCE)
set(OpenMP_omp_LIBRARY "libgomp.so" CACHE PATH "" FORCE)

7
cmake/presets/pgi.cmake
View File

@ -7,10 +7,3 @@ set(MPI_CXX "pgc++" CACHE STRING "" FORCE)
set(MPI_CXX_COMPILER "mpicxx" CACHE STRING "" FORCE)
unset(HAVE_OMP_H_INCLUDE CACHE)
set(OpenMP_C "pgcc" CACHE STRING "" FORCE)
set(OpenMP_C_FLAGS "-mp" CACHE STRING "" FORCE)
set(OpenMP_C_LIB_NAMES "omp" CACHE STRING "" FORCE)
set(OpenMP_CXX "pgc++" CACHE STRING "" FORCE)
set(OpenMP_CXX_FLAGS "-mp" CACHE STRING "" FORCE)
set(OpenMP_CXX_LIB_NAMES "omp" CACHE STRING "" FORCE)
set(OpenMP_omp_LIBRARY "libomp.so" CACHE PATH "" FORCE)

23
doc/Makefile
View File

@ -38,16 +38,14 @@ endif
# override settings for PIP commands
# PIP_OPTIONS = --cert /etc/pki/ca-trust/extracted/openssl/ca-bundle.trust.crt --proxy http://proxy.mydomain.org
#SPHINXEXTRA = -j $(shell $(PYTHON) -c 'import multiprocessing;print(multiprocessing.cpu_count())') $(shell test -f $(BUILDDIR)/doxygen/xml/run.stamp && printf -- "-E")
# temporarily disable caching so that the hack for the sphinx-tabs extensions to get proper non-html output works
SPHINXEXTRA = -E -j $(shell $(PYTHON) -c 'import multiprocessing;print(multiprocessing.cpu_count())')
SPHINXEXTRA = -j $(shell $(PYTHON) -c 'import multiprocessing;print(multiprocessing.cpu_count())')
# grab list of sources from doxygen config file.
# we only want to use explicitly listed files.
DOXYFILES = $(shell sed -n -e 's/\#.*$$//' -e '/^ *INPUT \+=/,/^[A-Z_]\+ \+=/p' doxygen/Doxyfile.in | sed -e 's/@LAMMPS_SOURCE_DIR@/..\/src/g' -e 's/\\//g' -e 's/ \+/ /' -e 's/[A-Z_]\+ \+= *\(YES\|NO\|\)//')
.PHONY: help clean-all clean clean-spelling epub mobi rst html pdf spelling anchor_check style_check char_check xmlgen fasthtml
.PHONY: help clean-all clean clean-spelling epub mobi html pdf spelling anchor_check style_check char_check role_check xmlgen fasthtml
# ------------------------------------------
@ -89,6 +87,8 @@ html: xmlgen $(VENV) $(SPHINXCONFIG)/conf.py $(ANCHORCHECK) $(MATHJAX)
@$(MAKE) $(MFLAGS) -C graphviz all
@(\
. $(VENV)/bin/activate ; env PYTHONWARNINGS= \
sphinx-build -E $(SPHINXEXTRA) -b html -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) html ;\
touch $(RSTDIR)/Fortran.rst ;\
sphinx-build $(SPHINXEXTRA) -b html -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) html ;\
ln -sf Manual.html html/index.html;\
rm -f $(BUILDDIR)/doxygen/xml/run.stamp;\
@ -96,6 +96,7 @@ html: xmlgen $(VENV) $(SPHINXCONFIG)/conf.py $(ANCHORCHECK) $(MATHJAX)
rst_anchor_check src/*.rst ;\
python $(BUILDDIR)/utils/check-packages.py -s ../src -d src ;\
env LC_ALL=C grep -n '[^ -~]' $(RSTDIR)/*.rst ;\
env LC_ALL=C grep -n ' :[a-z]\+`' $(RSTDIR)/*.rst ;\
python $(BUILDDIR)/utils/check-styles.py -s ../src -d src ;\
echo "############################################" ;\
deactivate ;\
@ -114,7 +115,9 @@ fasthtml: xmlgen $(VENV) $(SPHINXCONFIG)/conf.py $(ANCHORCHECK) $(MATHJAX)
@mkdir -p fasthtml
@(\
. $(VENV)/bin/activate ; env PYTHONWARNINGS= \
sphinx-build -j 4 -b html -c $(SPHINXCONFIG) -d $(BUILDDIR)/fasthtml/doctrees $(RSTDIR) fasthtml ;\
sphinx-build $(SPHINXEXTRA) -b html -c $(SPHINXCONFIG) -d $(BUILDDIR)/fasthtml/doctrees $(RSTDIR) fasthtml ;\
touch $(RSTDIR)/Fortran.rst ;\
sphinx-build $(SPHINXEXTRA) -b html -c $(SPHINXCONFIG) -d $(BUILDDIR)/fasthtml/doctrees $(RSTDIR) fasthtml ;\
deactivate ;\
)
@rm -rf fasthtml/_sources
@ -144,6 +147,8 @@ epub: xmlgen $(VENV) $(SPHINXCONFIG)/conf.py $(ANCHORCHECK)
@cp src/JPG/*.* epub/JPG
@(\
. $(VENV)/bin/activate ;\
sphinx-build -E $(SPHINXEXTRA) -b epub -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) epub ;\
touch $(RSTDIR)/Fortran.rst ;\
sphinx-build $(SPHINXEXTRA) -b epub -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) epub ;\
rm -f $(BUILDDIR)/doxygen/xml/run.stamp;\
deactivate ;\
@ -163,12 +168,15 @@ pdf: xmlgen $(VENV) $(SPHINXCONFIG)/conf.py $(ANCHORCHECK)
@if [ "$(HAS_PDFLATEX)" == "NO" ] ; then echo "PDFLaTeX or latexmk were not found! Please check README for further instructions" 1>&2; exit 1; fi
@(\
. $(VENV)/bin/activate ; env PYTHONWARNINGS= \
sphinx-build $(SPHINXEXTRA) -b latex -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) latex ;\
sphinx-build -E $(SPHINXEXTRA) -b latex -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) latex ;\
touch $(RSTDIR)/Fortran.rst ;\
sphinx-build $(SPHINXEXTRA) -b latex -c $(SPHINXCONFIG) -d $(BUILDDIR)/doctrees $(RSTDIR) latex ;\
rm -f $(BUILDDIR)/doxygen/xml/run.stamp;\
echo "############################################" ;\
rst_anchor_check src/*.rst ;\
python utils/check-packages.py -s ../src -d src ;\
env LC_ALL=C grep -n '[^ -~]' $(RSTDIR)/*.rst ;\
env LC_ALL=C grep -n ' :[a-z]\+`' $(RSTDIR)/*.rst ;\
python utils/check-styles.py -s ../src -d src ;\
echo "############################################" ;\
deactivate ;\
@ -214,6 +222,9 @@ package_check : $(VENV)
char_check :
@( env LC_ALL=C grep -n '[^ -~]' $(RSTDIR)/*.rst && exit 1 || : )
role_check :
@( env LC_ALL=C grep -n ' :[a-z]\+`' $(RSTDIR)/*.rst && exit 1 || : )
xmlgen : doxygen/xml/index.xml
doxygen/Doxyfile: doxygen/Doxyfile.in

4
doc/lammps.1
View File

@ -1,7 +1,7 @@
.TH LAMMPS "1" "15 September 2022" "2022-9-15"
.TH LAMMPS "1" "22 December 2022" "2022-12-22"
.SH NAME
.B LAMMPS
\- Molecular Dynamics Simulator. Version 15 September 2022
\- Molecular Dynamics Simulator. Version 22 December 2022
.SH SYNOPSIS
.B lmp

10
doc/src/Build_development.rst
View File

@ -147,6 +147,16 @@ compile and will download and compile a specific recent version of the
`Googletest <https://github.com/google/googletest/>`_ C++ test framework
for implementing the tests.
.. admonition:: Software version requirements for testing
:class: note
The compiler and library version requirements for the testing
framework are more strict than for the main part of LAMMPS. For
example the default GNU C++ and Fortran compilers of RHEL/CentOS 7.x
(version 4.8.x) are not sufficient. The CMake configuration will try
to detect compatible versions and either skip incompatible tests or
stop with an error.
After compilation is complete, the unit testing is started in the build
folder using the ``ctest`` command, which is part of the CMake software.
The output of this command will be looking something like this::

104
doc/src/Build_extras.rst
View File

@ -36,6 +36,7 @@ This is the list of packages that may require additional steps.
* :ref:`AWPMD <awpmd>`
* :ref:`COLVARS <colvars>`
* :ref:`COMPRESS <compress>`
* :ref:`ELECTRODE <electrode>`
* :ref:`GPU <gpu>`
* :ref:`H5MD <h5md>`
* :ref:`INTEL <intel>`
@ -48,6 +49,7 @@ This is the list of packages that may require additional steps.
* :ref:`ML-HDNNP <ml-hdnnp>`
* :ref:`ML-IAP <mliap>`
* :ref:`ML-PACE <ml-pace>`
* :ref:`ML-POD <ml-pod>`
* :ref:`ML-QUIP <ml-quip>`
* :ref:`MOLFILE <molfile>`
* :ref:`MSCG <mscg>`
@ -234,7 +236,7 @@ LAMMPS code. This also applies to the ``-DLAMMPS_BIGBIG``\ ,
Makefile you use.
You can also build the library in one step from the ``lammps/src`` dir,
using a command like these, which simply invoke the ``lib/gpu/Install.py``
using a command like these, which simply invokes the ``lib/gpu/Install.py``
script with the specified args:
.. code-block:: bash
@ -350,7 +352,7 @@ minutes to hours) to build. Of course you only need to do that once.)
You can download and build the KIM library manually if you prefer;
follow the instructions in ``lib/kim/README``. You can also do
this in one step from the lammps/src directory, using a command like
these, which simply invoke the ``lib/kim/Install.py`` script with
these, which simply invokes the ``lib/kim/Install.py`` script with
the specified args.
.. code-block:: bash
@ -954,7 +956,7 @@ more details.
You can download and build the MS-CG library manually if you
prefer; follow the instructions in ``lib/mscg/README``\ . You can
also do it in one step from the ``lammps/src`` dir, using a
command like these, which simply invoke the
command like these, which simply invokes the
``lib/mscg/Install.py`` script with the specified args:
.. code-block:: bash
@ -1011,7 +1013,7 @@ POEMS package
``lib/poems``\ . You can do this manually if you prefer; follow
the instructions in ``lib/poems/README``\ . You can also do it in
one step from the ``lammps/src`` dir, using a command like these,
which simply invoke the ``lib/poems/Install.py`` script with the
which simply invokes the ``lib/poems/Install.py`` script with the
specified args:
.. code-block:: bash
@ -1100,7 +1102,7 @@ binary package provided by your operating system.
You can download and build the Voro++ library manually if you
prefer; follow the instructions in ``lib/voronoi/README``. You
can also do it in one step from the ``lammps/src`` dir, using a
command like these, which simply invoke the
command like these, which simply invokes the
``lib/voronoi/Install.py`` script with the specified args:
.. code-block:: bash
@ -1179,7 +1181,7 @@ The ATC package requires the MANYBODY package also be installed.
``lib/atc``. You can do this manually if you prefer; follow the
instructions in ``lib/atc/README``. You can also do it in one
step from the ``lammps/src`` dir, using a command like these,
which simply invoke the ``lib/atc/Install.py`` script with the
which simply invokes the ``lib/atc/Install.py`` script with the
specified args:
.. code-block:: bash
@ -1230,7 +1232,7 @@ AWPMD package
``lib/awpmd``. You can do this manually if you prefer; follow the
instructions in ``lib/awpmd/README``. You can also do it in one
step from the ``lammps/src`` dir, using a command like these,
which simply invoke the ``lib/awpmd/Install.py`` script with the
which simply invokes the ``lib/awpmd/Install.py`` script with the
specified args:
.. code-block:: bash
@ -1293,7 +1295,7 @@ be built for the most part with all major versions of the C++ language.
In general, it is safer to use build setting consistent with the
rest of LAMMPS. This is best carried out from the LAMMPS src
directory using a command like these, which simply invoke the
directory using a command like these, which simply invokes the
``lib/colvars/Install.py`` script with the specified args:
.. code-block:: bash
@ -1334,20 +1336,30 @@ This package depends on the KSPACE package.
.. tab:: CMake build
No additional settings are needed besides ``-D PKG_KSPACE=yes`` and ``-D
PKG_ELECTRODE=yes``.
No additional settings are needed besides ``-D PKG_KSPACE=yes`` and
``-D PKG_ELECTRODE=yes``.
.. tab:: Traditional make
The package is activated with ``make yes-KSPACE`` and ``make
yes-ELECTRODE``
Before building LAMMPS, you must configure the ELECTRODE support
libraries and settings in ``lib/electrode``. You can do this
manually, if you prefer, or do it in one step from the
``lammps/src`` dir, using a command like these, which simply
invokes the ``lib/electrode/Install.py`` script with the specified
args:
.. code-block:: bash
$ make lib-electrode # print help message
$ make lib-electrode args="-m serial" # build with GNU g++ compiler and MPI STUBS (settings as with "make serial")
$ make lib-electrode args="-m mpi" # build with default MPI compiler (settings as with "make mpi")
Note that the ``Makefile.lammps`` file has settings for the BLAS and
LAPACK linear algebra libraries. As explained in ``lib/awpmd/README``
these can either exist on your system, or you can use the files provided
in ``lib/linalg``. In the latter case you also need to build the library
in ``lib/linalg`` with a command like these:
Note that the ``Makefile.lammps`` file has settings for the BLAS
and LAPACK linear algebra libraries. These can either exist on
your system, or you can use the files provided in ``lib/linalg``.
In the latter case you also need to build the library in
``lib/linalg`` with a command like these:
.. code-block:: bash
@ -1356,6 +1368,9 @@ This package depends on the KSPACE package.
$ make lib-linalg args="-m mpi" # build with default MPI Fortran compiler (settings as with "make mpi")
$ make lib-linalg args="-m gfortran" # build with GNU Fortran compiler
The package itself is activated with ``make yes-KSPACE`` and
``make yes-ELECTRODE``
----------
.. _ml-pace:
@ -1398,6 +1413,49 @@ at: `https://github.com/ICAMS/lammps-user-pace/ <https://github.com/ICAMS/lammps
----------
.. _ml-pod:
ML-POD package
-----------------------------
.. tabs::
.. tab:: CMake build
No additional settings are needed besides ``-D PKG_ML-POD=yes``.
.. tab:: Traditional make
Before building LAMMPS, you must configure the ML-POD support
settings in ``lib/mlpod``. You can do this manually, if you
prefer, or do it in one step from the ``lammps/src`` dir, using a
command like the following, which simply invoke the
``lib/mlpod/Install.py`` script with the specified args:
.. code-block:: bash
$ make lib-mlpod # print help message
$ make lib-mlpod args="-m serial" # build with GNU g++ compiler and MPI STUBS (settings as with "make serial")
$ make lib-mlpod args="-m mpi" # build with default MPI compiler (settings as with "make mpi")
$ make lib-mlpod args="-m mpi -e linalg" # same as above but use the bundled linalg lib
Note that the ``Makefile.lammps`` file has settings to use the BLAS
and LAPACK linear algebra libraries. These can either exist on
your system, or you can use the files provided in ``lib/linalg``.
In the latter case you also need to build the library in
``lib/linalg`` with a command like these:
.. code-block:: bash
$ make lib-linalg # print help message
$ make lib-linalg args="-m serial" # build with GNU Fortran compiler (settings as with "make serial")
$ make lib-linalg args="-m mpi" # build with default MPI Fortran compiler (settings as with "make mpi")
$ make lib-linalg args="-m gfortran" # build with GNU Fortran compiler
The package itself is activated with ``make yes-ML-POD``.
----------
.. _plumed:
PLUMED package
@ -1555,7 +1613,7 @@ the HDF5 library.
``lib/h5md``. You can do this manually if you prefer; follow the
instructions in ``lib/h5md/README``. You can also do it in one
step from the ``lammps/src`` dir, using a command like these,
which simply invoke the ``lib/h5md/Install.py`` script with the
which simply invokes the ``lib/h5md/Install.py`` script with the
specified args:
.. code-block:: bash
@ -1611,7 +1669,7 @@ details please see ``lib/hdnnp/README`` and the `n2p2 build documentation
You can download and build the *n2p2* library manually if you prefer;
follow the instructions in ``lib/hdnnp/README``\ . You can also do it in
one step from the ``lammps/src`` dir, using a command like these, which
simply invoke the ``lib/hdnnp/Install.py`` script with the specified args:
simply invokes the ``lib/hdnnp/Install.py`` script with the specified args:
.. code-block:: bash
@ -1748,7 +1806,7 @@ they will be downloaded the first time this package is installed.
Before building LAMMPS, you must build the *mesont* library in
``lib/mesont``\ . You can also do it in one step from the
``lammps/src`` dir, using a command like these, which simply
invoke the ``lib/mesont/Install.py`` script with the specified
invokes the ``lib/mesont/Install.py`` script with the specified
args:
.. code-block:: bash
@ -1917,7 +1975,7 @@ verified to work in February 2020 with Quantum Espresso versions 6.3 to
``lib/qmmm``. You can do this manually if you prefer; follow the
first two steps explained in ``lib/qmmm/README``. You can also do
it in one step from the ``lammps/src`` dir, using a command like
these, which simply invoke the ``lib/qmmm/Install.py`` script with
these, which simply invokes the ``lib/qmmm/Install.py`` script with
the specified args:
.. code-block:: bash
@ -2025,7 +2083,7 @@ To build with this package, you must download and build the
You can download and build the ScaFaCoS library manually if you
prefer; follow the instructions in ``lib/scafacos/README``. You
can also do it in one step from the ``lammps/src`` dir, using a
command like these, which simply invoke the
command like these, which simply invokes the
``lib/scafacos/Install.py`` script with the specified args:
.. code-block:: bash
@ -2069,7 +2127,7 @@ Eigen3 is a template library, so you do not need to build it.
You can download the Eigen3 library manually if you prefer; follow
the instructions in ``lib/smd/README``. You can also do it in one
step from the ``lammps/src`` dir, using a command like these,
which simply invoke the ``lib/smd/Install.py`` script with the
which simply invokes the ``lib/smd/Install.py`` script with the
specified args:
.. code-block:: bash

5
doc/src/Commands_all.rst
View File

@ -31,7 +31,6 @@ table above.
* :doc:`bond_style <bond_style>`
* :doc:`bond_write <bond_write>`
* :doc:`boundary <boundary>`
* :doc:`box <box>`
* :doc:`change_box <change_box>`
* :doc:`clear <clear>`
* :doc:`comm_modify <comm_modify>`
@ -90,8 +89,7 @@ table above.
* :doc:`region <region>`
* :doc:`replicate <replicate>`
* :doc:`rerun <rerun>`
* :doc:`reset_atom_ids <reset_atom_ids>`
* :doc:`reset_mol_ids <reset_mol_ids>`
* :doc:`reset_atoms <reset_atoms>`
* :doc:`reset_timestep <reset_timestep>`
* :doc:`restart <restart>`
* :doc:`run <run>`
@ -127,6 +125,7 @@ additional letter in parenthesis: k = KOKKOS.
* :doc:`group2ndx <group2ndx>`
* :doc:`hyper <hyper>`
* :doc:`kim <kim_commands>`
* :doc:`fitpod <fitpod_command>`
* :doc:`mdi <mdi>`
* :doc:`ndx2group <group2ndx>`
* :doc:`neb <neb>`

1
doc/src/Commands_category.rst
View File

@ -25,7 +25,6 @@ Setup simulation box:
:columns: 4
* :doc:`boundary <boundary>`
* :doc:`box <box>`
* :doc:`change_box <change_box>`
* :doc:`create_box <create_box>`
* :doc:`dimension <dimension>`

1
doc/src/Commands_compute.rst
View File

@ -107,6 +107,7 @@ KOKKOS, o = OPENMP, t = OPT.
* :doc:`pressure/uef <compute_pressure_uef>`
* :doc:`property/atom <compute_property_atom>`
* :doc:`property/chunk <compute_property_chunk>`
* :doc:`property/grid <compute_property_grid>`
* :doc:`property/local <compute_property_local>`
* :doc:`ptm/atom <compute_ptm_atom>`
* :doc:`rdf <compute_rdf>`

3
doc/src/Commands_dump.rst
View File

@ -36,7 +36,8 @@ An alphabetic list of all LAMMPS :doc:`dump <dump>` commands.
* :doc:`custom/mpiio <dump>`
* :doc:`custom/zstd <dump>`
* :doc:`dcd <dump>`
* :doc:`deprecated <dump>`
* :doc:`grid <dump>`
* :doc:`grid/vtk <dump>`
* :doc:`h5md <dump_h5md>`
* :doc:`image <dump_image>`
* :doc:`local <dump>`

12
doc/src/Commands_fix.rst
View File

@ -38,6 +38,7 @@ OPT.
* :doc:`ave/chunk <fix_ave_chunk>`
* :doc:`ave/correlate <fix_ave_correlate>`
* :doc:`ave/correlate/long <fix_ave_correlate_long>`
* :doc:`ave/grid <fix_ave_grid>`
* :doc:`ave/histo <fix_ave_histo>`
* :doc:`ave/histo/weight <fix_ave_histo>`
* :doc:`ave/time <fix_ave_time>`
@ -65,13 +66,13 @@ OPT.
* :doc:`drude <fix_drude>`
* :doc:`drude/transform/direct <fix_drude_transform>`
* :doc:`drude/transform/inverse <fix_drude_transform>`
* :doc:`dt/reset <fix_dt_reset>`
* :doc:`dt/reset (k) <fix_dt_reset>`
* :doc:`edpd/source <fix_dpd_source>`
* :doc:`efield <fix_efield>`
* :doc:`ehex <fix_ehex>`
* :doc:`electrode/conp (i) <fix_electrode_conp>`
* :doc:`electrode/conq (i) <fix_electrode_conp>`
* :doc:`electrode/thermo (i) <fix_electrode_conp>`
* :doc:`electrode/conp (i) <fix_electrode>`
* :doc:`electrode/conq (i) <fix_electrode>`
* :doc:`electrode/thermo (i) <fix_electrode>`
* :doc:`electron/stopping <fix_electron_stopping>`
* :doc:`electron/stopping/fit <fix_electron_stopping>`
* :doc:`enforce2d (k) <fix_enforce2d>`
@ -213,6 +214,7 @@ OPT.
* :doc:`saed/vtk <fix_saed_vtk>`
* :doc:`setforce (k) <fix_setforce>`
* :doc:`setforce/spin <fix_setforce>`
* :doc:`sgcmc <fix_sgcmc>`
* :doc:`shake (k) <fix_shake>`
* :doc:`shardlow (k) <fix_shardlow>`
* :doc:`smd <fix_smd>`
@ -249,7 +251,7 @@ OPT.
* :doc:`tune/kspace <fix_tune_kspace>`
* :doc:`vector <fix_vector>`
* :doc:`viscosity <fix_viscosity>`
* :doc:`viscous <fix_viscous>`
* :doc:`viscous (k) <fix_viscous>`
* :doc:`viscous/sphere <fix_viscous_sphere>`
* :doc:`wall/body/polygon <fix_wall_body_polygon>`
* :doc:`wall/body/polyhedron <fix_wall_body_polyhedron>`

8
doc/src/Commands_pair.rst
View File

@ -93,8 +93,8 @@ OPT.
* :doc:`coul/wolf/cs <pair_cs>`
* :doc:`dpd (giko) <pair_dpd>`
* :doc:`dpd/fdt <pair_dpd_fdt>`
* :doc:`dpd/ext (k) <pair_dpd_ext>`
* :doc:`dpd/ext/tstat (k) <pair_dpd_ext>`
* :doc:`dpd/ext (ko) <pair_dpd_ext>`
* :doc:`dpd/ext/tstat (ko) <pair_dpd_ext>`
* :doc:`dpd/fdt/energy (k) <pair_dpd_fdt>`
* :doc:`dpd/tstat (gko) <pair_dpd>`
* :doc:`dsmc <pair_dsmc>`
@ -205,7 +205,7 @@ OPT.
* :doc:`mesont/tpm <pair_mesont_tpm>`
* :doc:`mgpt <pair_mgpt>`
* :doc:`mie/cut (g) <pair_mie>`
* :doc:`mliap <pair_mliap>`
* :doc:`mliap (k) <pair_mliap>`
* :doc:`mm3/switch3/coulgauss/long <pair_lj_switch3_coulgauss_long>`
* :doc:`momb <pair_momb>`
* :doc:`morse (gkot) <pair_morse>`
@ -237,6 +237,7 @@ OPT.
* :doc:`oxrna2/coaxstk <pair_oxrna2>`
* :doc:`pace (k) <pair_pace>`
* :doc:`pace/extrapolation <pair_pace>`
* :doc:`pod <pair_pod>`
* :doc:`peri/eps <pair_peri>`
* :doc:`peri/lps (o) <pair_peri>`
* :doc:`peri/pmb (o) <pair_peri>`
@ -295,6 +296,7 @@ OPT.
* :doc:`vashishta (gko) <pair_vashishta>`
* :doc:`vashishta/table (o) <pair_vashishta>`
* :doc:`wf/cut <pair_wf_cut>`
* :doc:`ylz <pair_ylz>`
* :doc:`yukawa (gko) <pair_yukawa>`
* :doc:`yukawa/colloid (go) <pair_yukawa_colloid>`
* :doc:`zbl (gko) <pair_zbl>`

52
doc/src/Commands_removed.rst
View File

@ -2,14 +2,17 @@ Removed commands and packages
=============================
This page lists LAMMPS commands and packages that have been removed from
the distribution and provides suggestions for alternatives or replacements.
LAMMPS has special dummy styles implemented, that will stop LAMMPS and
print a suitable error message in most cases, when a style/command is used
that has been removed.
the distribution and provides suggestions for alternatives or
replacements. LAMMPS has special dummy styles implemented, that will
stop LAMMPS and print a suitable error message in most cases, when a
style/command is used that has been removed or will replace the command
with the direct alternative (if available) and print a warning.
Fix ave/spatial and fix ave/spatial/sphere
------------------------------------------
.. deprecated:: 11Dec2015
The fixes ave/spatial and ave/spatial/sphere have been removed from LAMMPS
since they were superseded by the more general and extensible "chunk
infrastructure". Here the system is partitioned in one of many possible
@ -17,10 +20,23 @@ ways through the :doc:`compute chunk/atom <compute_chunk_atom>` command
and then averaging is done using :doc:`fix ave/chunk <fix_ave_chunk>`.
Please refer to the :doc:`chunk HOWTO <Howto_chunk>` section for an overview.
Reset_ids command
-----------------
Box command
-----------
The reset_ids command has been renamed to :doc:`reset_atom_ids <reset_atom_ids>`.
.. deprecated:: 22Dec2022
The *box* command has been removed and the LAMMPS code changed so it won't
be needed. If present, LAMMPS will ignore the command and print a warning.
Reset_ids, reset_atom_ids, reset_mol_ids commands
-------------------------------------------------
.. deprecated:: 22Dec2022
The *reset_ids*, *reset_atom_ids*, and *reset_mol_ids* commands have
been folded into the :doc:`reset_atoms <reset_atoms>` command. If
present, LAMMPS will replace the commands accordingly and print a
warning.
MEAM package
------------
@ -30,18 +46,21 @@ The code in the :ref:`MEAM package <PKG-MEAM>` is a translation of the
Fortran code of MEAM into C++, which removes several restrictions
(e.g. there can be multiple instances in hybrid pair styles) and allows
for some optimizations leading to better performance. The pair style
:doc:`meam <pair_meam>` has the exact same syntax.
:doc:`meam <pair_meam>` has the exact same syntax. For a transition
period the C++ version of MEAM was called USER-MEAMC so it could
coexist with the Fortran version.
REAX package
------------
The REAX package has been removed since it was superseded by the
:ref:`REAXFF package <PKG-REAXFF>`. The REAXFF
package has been tested to yield equivalent results to the REAX package,
offers better performance, supports OpenMP multi-threading via OPENMP,
and GPU and threading parallelization through KOKKOS. The new pair styles
are not syntax compatible with the removed reax pair style, so input
files will have to be adapted.
:ref:`REAXFF package <PKG-REAXFF>`. The REAXFF package has been tested
to yield equivalent results to the REAX package, offers better
performance, supports OpenMP multi-threading via OPENMP, and GPU and
threading parallelization through KOKKOS. The new pair styles are not
syntax compatible with the removed reax pair style, so input files will
have to be adapted. The REAXFF package was originally called
USER-REAXC.
USER-CUDA package
-----------------
@ -60,5 +79,6 @@ restart2data tool
The functionality of the restart2data tool has been folded into the
LAMMPS executable directly instead of having a separate tool. A
combination of the commands :doc:`read_restart <read_restart>` and
:doc:`write_data <write_data>` can be used to the same effect. For added
convenience this conversion can also be triggered by :doc:`command line flags <Run_options>`
:doc:`write_data <write_data>` can be used to the same effect. For
added convenience this conversion can also be triggered by
:doc:`command line flags <Run_options>`

1
doc/src/Developer.rst
View File

@ -23,3 +23,4 @@ of time and requests from the LAMMPS user community.
Classes
Developer_platform
Developer_utils
Developer_grid

14
doc/src/Developer_code_design.rst
View File

@ -50,7 +50,7 @@ parallel each MPI process creates such an instance. This can be seen
in the ``main.cpp`` file where the core steps of running a LAMMPS
simulation are the following 3 lines of code:
.. code-block:: C++
.. code-block:: c++
LAMMPS *lammps = new LAMMPS(argc, argv, lammps_comm);
lammps->input->file();
@ -78,7 +78,7 @@ LAMMPS makes extensive use of the object oriented programming (OOP)
principles of *compositing* and *inheritance*. Classes like the
``LAMMPS`` class are a **composite** containing pointers to instances
of other classes like ``Atom``, ``Comm``, ``Force``, ``Neighbor``,
``Modify``, and so on. Each of these classes implement certain
``Modify``, and so on. Each of these classes implements certain
functionality by storing and manipulating data related to the
simulation and providing member functions that trigger certain
actions. Some of those classes like ``Force`` are themselves
@ -87,9 +87,9 @@ interactions. Similarly the ``Modify`` class contains a list of
``Fix`` and ``Compute`` classes. If the input commands that
correspond to these classes include the word *style*, then LAMMPS
stores only a single instance of that class. E.g. *atom_style*,
*comm_style*, *pair_style*, *bond_style*. It the input command does
not include the word *style*, there can be many instances of that
class defined. E.g. *region*, *fix*, *compute*, *dump*.
*comm_style*, *pair_style*, *bond_style*. If the input command does
**not** include the word *style*, then there may be many instances of
that class defined, for example *region*, *fix*, *compute*, *dump*.
**Inheritance** enables creation of *derived* classes that can share
common functionality in their base class while providing a consistent
@ -232,7 +232,7 @@ macro ``PairStyle()`` will associate the style name "lj/cut"
with a factory function creating an instance of the ``PairLJCut``
class.
.. code-block:: C++
.. code-block:: c++
// from force.h
typedef Pair *(*PairCreator)(LAMMPS *);
@ -360,7 +360,7 @@ characters; "{:<8}" would do this as left aligned, "{:^8}" as centered,
argument type must be compatible or else the {fmt} formatting code will
throw an exception. Some format string examples are given below:
.. code-block:: C
.. code-block:: c++
auto mesg = fmt::format(" CPU time: {:4d}:{:02d}:{:02d}\n", cpuh, cpum, cpus);
mesg = fmt::format("{:<8s}| {:<10.5g} | {:<10.5g} | {:<10.5g} |{:6.1f} |{:6.2f}\n",

846
doc/src/Developer_grid.rst Normal file
View File

@ -0,0 +1,846 @@
Use of distributed grids within style classes
---------------------------------------------
.. versionadded:: 22Dec2022
The LAMMPS source code includes two classes which facilitate the
creation and use of distributed grids. These are the Grid2d and
Grid3d classes in the src/grid2d.cpp.h and src/grid3d.cpp.h files
respectively. As the names imply, they are used for 2d or 3d
simulations, as defined by the :doc:`dimension <dimension>` command.
The :doc:`Howto_grid <Howto_grid>` page gives an overview of how
distributed grids are defined from a user perspective, lists LAMMPS
commands which use them, and explains how grid cell data is referenced
from an input script. Please read that page first as it motivates the
coding details discussed here.
This doc page is for users who wish to write new styles (input script
commands) which use distributed grids. There are a variety of
material models and analysis methods which use atoms (or
coarse-grained particles) and grids in tandem.
A *distributed* grid means each processor owns a subset of the grid
cells. In LAMMPS, the subset for each processor will be a sub-block
of grid cells with low and high index bounds in each dimension of the
grid. The union of the sub-blocks across all processors is the global
grid.
More specifically, a grid point is defined for each cell (by default
the center point), and a processor owns a grid cell if its point is
within the processor's spatial sub-domain. The union of processor
sub-domains is the global simulation box. If a grid point is on the
boundary of two sub-domains, the lower processor owns the grid cell. A
processor may also store copies of ghost cells which surround its
owned cells.
----------
Style commands
^^^^^^^^^^^^^^
Style commands which can define and use distributed grids include the
:doc:`compute <compute>`, :doc:`fix <fix>`, :doc:`pair <pair_style>`,
and :doc:`kspace <kspace_style>` styles. If you wish grid cell data
to persist across timesteps, then use a fix. If you wish grid cell
data to be accessible by other commands, then use a fix or compute.
Currently in LAMMPS, the :doc:`pair_style amoeba <pair_amoeba>`,
:doc:`kspace_style pppm <kspace_style>`, and :doc:`kspace_style msm
<kspace_style>` commands use distributed grids but do not require
either of these capabilities; they thus create and use distributed
grids internally. Note that a pair style which needs grid cell data
to persist could be coded to work in tandem with a fix style which
provides that capability.
The *size* of a grid is specified by the number of grid cells in each
dimension of the simulation domain. In any dimension the size can be
any value >= 1. Thus a 10x10x1 grid for a 3d simulation is
effectively a 2d grid, where each grid cell spans the entire
z-dimension. A 1x100x1 grid for a 3d simulation is effectively a 1d
grid, where grid cells are a series of thin xz slabs in the
y-dimension. It is even possible to define a 1x1x1 3d grid, though it
may be inefficient to use it in a computational sense.
Note that the choice of grid size is independent of the number of
processors or their layout in a grid of processor sub-domains which
overlays the simulations domain. Depending on the distributed grid
size, a single processor may own many 1000s or no grid cells.
A command can define multiple grids, each of a different size. Each
grid is an instantiation of the Grid2d or Grid3d class.
The command also defines what data it will store for each grid it
creates and it allocates the multi-dimensional array(s) needed to
store the data. No grid cell data is stored within the Grid2d or
Grid3d classes.
If a single value per grid cell is needed, the data array will have
the same dimension as the grid, i.e. a 2d array for a 2d grid,
likewise for 3d. If multiple values per grid cell are needed, the
data array will have one more dimension than the grid, i.e. a 3d array
for a 2d grid, or 4d array for a 3d grid. A command can choose to
define multiple data arrays for each grid it defines.
----------
Grid data allocation and access
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
The simplest way for a command to allocate and access grid cell data
is to use the *create_offset()* methods provided by the Memory class.
Arguments for these methods can be values returned by the
*setup_grid()* method (described below), which define the extent of
the grid cells (owned+ghost) the processor owns. These 4 methods
allocate memory for 2d (first two) and 3d (second two) grid data. The
two methods that end in "_one" allocate an array which stores a single
value per grid cell. The two that end in "_multi" allocate an array
which stores *Nvalues* per grid cell.
.. code-block:: c++
// single value per cell for a 2d grid = 2d array
memory->create2d_offset(data2d_one, nylo_out, nyhi_out,
nxlo_out, nxhi_out, "data2d_one");
// nvalues per cell for a 2d grid = 3d array
memory->create3d_offset_last(data2d_multi, nylo_out, nyhi_out,
nxlo_out, nxhi_out, nvalues, "data2d_multi");
// single value per cell for a 3d grid = 3d array
memory->create3d_offset(data3d_one, nzlo_out, nzhi_out, nylo_out,
nyhi_out, nxlo_out, nxhi_out, "data3d_one");
// nvalues per cell for a 3d grid = 4d array
memory->create4d_offset_last(data3d_multi, nzlo_out, nzhi_out, nylo_out,
nyhi_out, nxlo_out, nxhi_out, nvalues,
"data3d_multi");
Note that these multi-dimensional arrays are allocated as contiguous
chunks of memory where the x-index of the grid varies fastest, then y,
and the z-index slowest. For multiple values per grid cell, the
Nvalues are contiguous, so their index varies even faster than the
x-index.
The key point is that the "offset" methods create arrays which are
indexed by the range of indices which are the bounds of the sub-block
of the global grid owned by this processor. This means loops like
these can be written in the caller code to loop over owned grid cells,
where the "i" loop bounds are the range of owned grid cells for the
processor. These are the bounds returned by the *setup_grid()*
method:
.. code-block:: c++
for (int iy = iylo; iy <= iyhi; iy++)
for (int ix = ixlo; ix <= ixhi; ix++)
data2d_one[iy][ix] = 0.0;
for (int iy = iylo; iy <= iyhi; iy++)
for (int ix = ixlo; ix <= ixhi; ix++)
for (int m = 0; m < nvalues; m++)
data2d_multi[iy][ix][m] = 0.0;
for (int iz = izlo; iz <= izhi; iz++)
for (int iy = iylo; iy <= iyhi; iy++)
for (int ix = ixlo; ix <= ixhi; ix++)
data3d_one[iz][iy][ix] = 0.0;
for (int iz = izlo; iz <= izhi; iz++)
for (int iy = iylo; iy <= iyhi; iy++)
for (int ix = ixlo; ix <= ixhi; ix++)
for (int m = 0; m < nvalues; m++)
data3d_multi[iz][iy][ix][m] = 0.0;
Simply replacing the "i" bounds with "o" bounds, also returned by the
*setup_grid()* method, would alter this code to loop over owned+ghost
cells (the entire allocated grid).
----------
Grid class constructors
^^^^^^^^^^^^^^^^^^^^^^^
The following sub-sections describe the public methods of the Grid3d
class which a style command can invoke. The Grid2d methods are
similar; simply remove arguments which refer to the z-dimension.
There are 2 constructors which can be used. They differ in the extra
i/o xyz lo/hi arguments:
.. code-block:: c++
Grid3d(class LAMMPS *lmp, MPI_Comm gcomm, int gnx, int gny, int gnz)
Grid3d(class LAMMPS *lmp, MPI_Comm gcomm, int gnx, int gny, int gnz,
int ixlo, int ixhi, int iylo, int iyhi, int izlo, int izhi,
int oxlo, int oxhi, int oylo, int oyhi, int ozlo, int ozhi)
Both constructors take the LAMMPS instance pointer and a communicator
over which the grid will be distributed. Typically this is the
*world* communicator the LAMMPS instance is using. The
:doc:`kspace_style msm <kspace_style>` command creates a series of
grids, each of different size, which are partitioned across different
sub-communicators of processors. Both constructors are also passed
the global grid size: *gnx* by *gny* by *gnz*.
The first constructor is used when the caller wants the Grid class to
partition the global grid across processors; the Grid class defines
which grid cells each processor owns and also which it stores as ghost
cells. A subsequent call to *setup_grid()*, discussed below, returns
this info to the caller.
The second constructor allows the caller to define the extent of owned
and ghost cells, and pass them to the Grid class. The 6 arguments
which start with "i" are the inclusive lower and upper index bounds of
the owned (inner) grid cells this processor owns in each of the 3
dimensions within the global grid. Owned grid cells are indexed from
0 to N-1 in each dimension.
The 6 arguments which start with "o" are the inclusive bounds of the
owned+ghost (outer) grid cells it stores. If the ghost cells are on
the other side of a periodic boundary, then these indices may be < 0
or >= N in any dimension, so that oxlo <= ixlo and ixhi >= ixhi is
always the case.
For example, if Nx = 100, then a processor might pass ixlo=50,
ixhi=60, oxlo=48, oxhi=62 to the Grid class. Or ixlo=0, ixhi=10,
oxlo=-2, oxhi=13. If a processor owns no grid cells in a dimension,
then the ihi value should be specified as one less than the ilo value.
Note that the only reason to use the second constructor is if the
logic for assigning ghost cells is too complex for the Grid class to
compute, using the various set() methods described next. Currently
only the kspace_style pppm/electrode and kspace_style msm commands use
the second constructor.
----------
Grid class set methods
^^^^^^^^^^^^^^^^^^^^^^
The following methods affect how the Grid class computes which owned
and ghost cells are assigned to each processor. *Set_shift_grid()* is
the only method which influences owned cell assignment; all the rest
influence ghost cell assignment. These methods are only used with the
first constructor; they are ignored if the second constructor is used.
These methods must be called before the *setup_grid()* method is
invoked, because they influence its operation.
.. code-block:: c++
void set_shift_grid(double shift);
void set_distance(double distance);
void set_stencil_atom(int lo, int hi);
void set_shift_atom(double shift_lo, double shift_hi);
void set_stencil_grid(int lo, int hi);
void set_zfactor(double factor);
Processors own a grid cell if a point within the grid cell is inside
the processor's sub-domain. By default this is the center point of the
grid cell. The *set_shift_grid()* method can change this. The *shift*
argument is a value from 0.0 to 1.0 (inclusive) which is the offset of
the point within the grid cell in each dimension. The default is 0.5
for the center of the cell. A value of 0.0 is the lower left corner
point; a value of 1.0 is the upper right corner point. There is
typically no need to change the default as it is optimal for
minimizing the number of ghost cells needed.
If a processor maps its particles to grid cells, it needs to allow for
its particles being outside its sub-domain between reneighboring. The
*distance* argument of the *set_distance()* method sets the furthest
distance outside a processor's sub-domain which a particle can move.
Typically this is half the neighbor skin distance, assuming
reneighboring is done appropriately. This distance is used in
determining how many ghost cells a processor needs to store to enable
its particles to be mapped to grid cells. The default value is 0.0.
Some commands, like the :doc:`kspace_style pppm <kspace_style>`
command, map values (charge in the case of PPPM) to a stencil of grid
cells beyond the grid cell the particle is in. The stencil extent may
be different in the low and high directions. The *set_stencil_atom()*
method defines the maximum values of those 2 extents, assumed to be
the same in each of the 3 dimensions. Both the lo and hi values are
specified as positive integers. The default values are both 0.
Some commands, like the :doc:`kspace_style pppm <kspace_style>`
command, shift the position of an atom when mapping it to a grid cell,
based on the size of the stencil used to map values to the grid
(charge in the case of PPPM). The lo and hi arguments of the
*set_shift_atom()* method are the minimum shift in the low direction
and the maximum shift in the high direction, assumed to be the same in
each of the 3 dimensions. The shifts should be fractions of a grid
cell size with values between 0.0 and 1.0 inclusive. The default
values are both 0.0. See the src/pppm.cpp file for examples of these
lo/hi values for regular and staggered grids.
Some methods like the :doc:`fix ttm/grid <fix_ttm>` command, perform
finite difference kinds of operations on the grid, to diffuse electron
heat in the case of the two-temperature model (TTM). This operation
uses ghost grid values beyond the owned grid values the processor
updates. The *set_stencil_grid()* method defines the extent of this
stencil in both directions, assumed to be the same in each of the 3
dimensions. Both the lo and hi values are specified as positive
integers. The default values are both 0.
The kspace_style pppm commands allow a grid to be defined which
overlays a volume which extends beyond the simulation box in the z
dimension. This is for the purpose of modeling a 2d-periodic slab
(non-periodic in z) as if it were a larger 3d periodic system,
extended (with empty space) in the z dimension. The
:doc:`kspace_modify slab <kspace_modify>` command is used to specify
the ratio of the larger volume to the simulation volume; a volume
ratio of ~3 is typical. For this kind of model, the PPPM caller sets
the global grid size *gnz* ~3x larger than it would be otherwise.
This same ratio is passed by the PPPM caller as the *factor* argument
to the Grid class via the *set_zfactor()* method (*set_yfactor()* for
2d grids). The Grid class will then assign ownership of the 1/3 of
grid cells that overlay the simulation box to the processors which
also overlay the simulation box. The remaining 2/3 of the grid cells
are assigned to processors whose sub-domains are adjacent to the upper
z boundary of the simulation box.
----------
Grid class setup_grid method
^^^^^^^^^^^^^^^^^^^^^^^^^^^^
The *setup_grid()* method is called after the first constructor
(above) to partition the grid across processors, which determines
which grid cells each processor owns. It also calculates how many
ghost grid cells in each dimension and each direction each processor
needs to store.
Note that this method is NOT called if the second constructor above is
used. In that case, the caller assigns owned and ghost cells to each
processor.
Also note that this method must be invoked after any *set_*()* methods have
been used, since they can influence the assignment of owned and ghost
cells.
.. code-block:: c++
void setup_grid(int &ixlo, int &ixhi, int &iylo, int &iyhi, int &izlo, int &izhi,
int &oxlo, int &oxhi, int &oylo, int &oyhi, int &ozlo, int &ozhi)
The 6 return arguments which start with "i" are the inclusive lower
and upper index bounds of the owned (inner) grid cells this processor
owns in each of the 3 dimensions within the global grid. Owned grid
cells are indexed from 0 to N-1 in each dimension.
The 6 return arguments which start with "o" are the inclusive bounds of
the owned+ghost cells it owns. If the ghost cells are on the other
side of a periodic boundary, then these indices may be < 0 or >= N in
any dimension, so that oxlo <= ixlo and ixhi >= ixhi is always the
case.
----------
More grid class set methods
^^^^^^^^^^^^^^^^^^^^^^^^^^^
The following 2 methods can be used to override settings made by the
constructors above. If used, they must be called called before the
*setup_comm()* method is invoked, since it uses the settings that
these methods override. In LAMMPS these methods are called by by the
:doc:`kspace_style msm <kspace_style>` command for the grids it
instantiates using the 2nd constructor above.
.. code-block:: c++
void set_proc_neighs(int pxlo, int pxhi, int pylo, int pyhi, int pzlo, int pzhi)
void set_caller_grid(int fxlo, int fxhi, int fylo, int fyhi, int fzlo, int fzhi)
The *set_proc_neighs()* method sets the processor IDs of the 6
neighboring processors for each processor. Normally these would match
the processor grid neighbors which LAMMPS creates to overlay the
simulation box (the default). However, MSM excludes non-participating
processors from coarse grid communication when less processors are
used. This method allows MSM to override the default values.
The *set_caller_grid()* method species the size of the data arrays the
caller allocates. Normally these would match the extent of the ghost
grid cells (the default). However the MSM caller allocates a larger
data array (more ghost cells) for its finest-level grid, for use in
other operations besides owned/ghost cell communication. This method
allows MSM to override the default values.
----------
Grid class get methods
^^^^^^^^^^^^^^^^^^^^^^
The following methods allow the caller to query the settings for a
specific grid, whether it created the grid or another command created
it.
.. code-block:: c++
void get_size(int &nxgrid, int &nygrid, int &nzgrid);
void get_bounds_owned(int &xlo, int &xhi, int &ylo, int &yhi, int &zlo, int &zhi)
void get_bounds_ghost(int &xlo, int &xhi, int &ylo, int &yhi, int &zlo, int &zhi)
The *get_size()* method returns the size of the global grid in each dimension.
The *get_bounds_owned()* method return the inclusive index bounds of
the grid cells this processor owns. The values range from 0 to N-1 in
each dimension. These values are the same as the "i" values returned
by *setup_grid()*.
The *get_bounds_ghost()* method return the inclusive index bounds of
the owned+ghost grid cells this processor stores. The owned cell
indices range from 0 to N-1, so these indices may be less than 0 or
greater than or equal to N in each dimension. These values are the
same as the "o" values returned by *setup_grid()*.
----------
Grid class owned/ghost communication
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
If needed by the command, the following methods setup and perform
communication of grid data to/from neighboring processors. The
*forward_comm()* method sends owned grid cell data to the
corresponding ghost grid cells on other processors. The
*reverse_comm()* method sends ghost grid cell data to the
corresponding owned grid cells on another processor. The caller can
choose to sum ghost grid cell data to the owned grid cell or simply
copy it.
.. code-block:: c++
void setup_comm(int &nbuf1, int &nbuf2)
void forward_comm(int caller, void *ptr, int which, int nper, int nbyte,
void *buf1, void *buf2, MPI_Datatype datatype);
void reverse_comm(int caller, void *ptr, int which, int nper, int nbyte,
void *buf1, void *buf2, MPI_Datatype datatype)
int ghost_adjacent();
The *setup_comm()* method must be called one time before performing
*forward* or *reverse* communication (multiple times if needed). It
returns two integers, which should be used to allocate two buffers.
The *nbuf1* and *nbuf2* values are the number of grid cells whose data
will be stored in two buffers by the Grid class when *forward* or
*reverse* communication is performed. The caller should thus allocate
them to a size large enough to hold all the data used in any single
forward or reverse communication operation it performs. Note that the
caller may allocate and communicate multiple data arrays for a grid it
instantiates. This size includes the bytes needed for the data type
of the grid data it stores, e.g. double precision values.
The *forward_comm()* and *reverse_comm()* methods send grid cell data
from owned to ghost cells, or ghost to owned cells, respectively, as
described above. The *caller* argument should be one of these values
-- Grid3d::COMPUTE, Grid3d::FIX, Grid3d::KSPACE, Grid3d::PAIR --
depending on the style of the caller class. The *ptr* argument is the
"this" pointer to the caller class. These 2 arguments are used to
call back to pack()/unpack() functions in the caller class, as
explained below.
The *which* argument is a flag the caller can set which is passed to
the caller's pack()/unpack() methods. This allows a single callback
method to pack/unpack data for several different flavors of
forward/reverse communication, e.g. operating on different grids or
grid data.
The *nper* argument is the number of values per grid cell to be
communicated. The *nbyte* argument is the number of bytes per value,
e.g. 8 for double-precision values. The *buf1* and *buf2* arguments
are the two allocated buffers described above. So long as they are
allocated for the maximum size communication, they can be re-used for
any *forward_comm()/reverse_comm()* call. The *datatype* argument is
the MPI_Datatype setting, which should match the buffer allocation and
the *nbyte* argument. E.g. MPI_DOUBLE for buffers storing double
precision values.
To use the *forward_grid()* method, the caller must provide two
callback functions; likewise for use of the *reverse_grid()* methods.
These are the 4 functions, their arguments are all the same.
.. code-block:: c++
void pack_forward_grid(int which, void *vbuf, int nlist, int *list);
void unpack_forward_grid(int which, void *vbuf, int nlist, int *list);
void pack_reverse_grid(int which, void *vbuf, int nlist, int *list);
void unpack_reverse_grid(int which, void *vbuf, int nlist, int *list);
The *which* argument is set to the *which* value of the
*forward_comm()* or *reverse_comm()* calls. It allows the pack/unpack
function to select what data values to pack/unpack. *Vbuf* is the
buffer to pack/unpack the data to/from. It is a void pointer so that
the caller can cast it to whatever data type it chooses, e.g. double
precision values. *Nlist* is the number of grid cells to pack/unpack
and *list* is a vector (nlist in length) of offsets to where the data
for each grid cell resides in the caller's data arrays, which is best
illustrated with an example from the src/EXTRA-FIX/fix_ttm_grid.cpp
class which stores the scalar electron temperature for 3d system in a
3d grid (one value per grid cell):
.. code-block:: c++
void FixTTMGrid::pack_forward_grid(int /*which*/, void *vbuf, int nlist, int *list)
{
auto buf = (double *) vbuf;
double *src = &T_electron[nzlo_out][nylo_out][nxlo_out];
for (int i = 0; i < nlist; i++) buf[i] = src[list[i]];
}
In this case, the *which* argument is not used, *vbuf* points to a
buffer of doubles, and the electron temperature is stored by the
FixTTMGrid class in a 3d array of owned+ghost cells called T_electron.
That array is allocated by the *memory->create_3d_offset()* method
described above so that the first grid cell it stores is indexed as
T_electron[nzlo_out][nylo_out][nxlo_out]. The *nlist* values in
*list* are integer offsets from that first grid cell. Setting *src*
to the address of the first cell allows those offsets to be used to
access the temperatures to pack into the buffer.
Here is a similar portion of code from the src/fix_ave_grid.cpp class
which can store two kinds of data, a scalar count of atoms in a grid
cell, and one or more grid-cell-averaged atom properties. The code
from its *unpack_reverse_grid()* function for 2d grids and multiple
per-atom properties per grid cell (*nvalues*) is shown here:
.. code-block:: c++
void FixAveGrid::unpack_reverse_grid(int /*which*/, void *vbuf, int nlist, int *list)
{
auto buf = (double *) vbuf;
double *count,*data,*values;
count = &count2d[nylo_out][nxlo_out];
data = &array2d[nylo_out][nxlo_out][0];
m = 0;
for (i = 0; i < nlist; i++) {
count[list[i]] += buf[m++];
values = &data[nvalues*list[i]];
for (j = 0; j < nvalues; j++)
values[j] += buf[m++];
}
}
Both the count and the multiple values per grid cell are communicated
in *vbuf*. Note that *data* is now a pointer to the first value in
the first grid cell. And *values* points to where the first value in
*data* is for an offset of grid cells, calculated by multiplying
*nvalues* by *list[i]*. Finally, because this is reverse
communication, the communicated buffer values are summed to the caller
values.
The *ghost_adjacent()* method returns a 1 if every processor can
perform the necessary owned/ghost communication with only its nearest
neighbor processors (4 in 2d, 6 in 3d). It returns a 0 if any
processor's ghost cells extend further than nearest neighbor
processors.
This can be checked by callers who have the option to change the
global grid size to insure more efficient nearest-neighbor-only
communication if they wish. In this case, they instantiate a grid of
a given size (resolution), then invoke *setup_comm()* followed by
*ghost_adjacent()*. If the ghost cells are not adjacent, they destroy
the grid instance and start over with a higher-resolution grid.
Several of the :doc:`kspace_style pppm <kspace_style>` command
variants have this option.
----------
Grid class remap methods for load balancing
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
The following methods are used when a load-balancing operation,
triggered by the :doc:`balance <balance>` or :doc:`fix balance
<fix_balance>` commands, changes the partitioning of the simulation
domain into processor sub-domains.
In order to work with load-balancing, any style command (compute, fix,
pair, or kspace style) which allocates a grid and stores per-grid data
should define a *reset_grid()* method; it takes no arguments. It will
be called by the two balance commands after they have reset processor
sub-domains and migrated atoms (particles) to new owning processors.
The *reset_grid()* method will typically perform some or all of the
following operations. See the src/fix_ave_grid.cpp and
src/EXTRA_FIX/fix_ttm_grid.cpp files for examples of *reset_grid()*
methods, as well as the *pack_remap_grid()* and *unpack_remap_grid()*
functions.
First, the *reset_grid()* method can instantiate new grid(s) of the
same global size, then call *setup_grid()* to partition them via the
new processor sub-domains. At this point, it can invoke the
*identical()* method which compares the owned and ghost grid cell
index bounds between two grids, the old grid passed as a pointer
argument, and the new grid whose *identical()* method is being called.
It returns 1 if the indices match on all processors, otherwise 0. If
they all match, then the new grids can be deleted; the command can
continue to use the old grids.
If not, then the command should allocate new grid data array(s) which
depend on the new partitioning. If the command does not need to
persist its grid data from the old partitioning to the new one, then
the command can simply delete the old data array(s) and grid
instance(s). It can then return.
If the grid data does need to persist, then the data for each grid
needs to be "remapped" from the old grid partitioning to the new grid
partitioning. The *setup_remap()* and *remap()* methods are used for
that purpose.
.. code-block:: c++
int identical(Grid3d *old);
void setup_remap(Grid3d *old, int &nremap_buf1, int &nremap_buf2)
void remap(int caller, void *ptr, int which, int nper, int nbyte,
void *buf1, void *buf2, MPI_Datatype datatype)
The arguments to these methods are identical to those for
the *setup_comm()* and *forward_comm()* or *reverse_comm()* methods.
However the returned *nremap_buf1* and *nremap2_buf* values will be
different than the *nbuf1* and *nbuf2* values. They should be used to
allocate two different remap buffers, separate from the owned/ghost
communication buffers.
To use the *remap()* method, the caller must provide two
callback functions:
.. code-block:: c++
void pack_remap_grid(int which, void *vbuf, int nlist, int *list);
void unpack_remap_grid(int which, void *vbuf, int list, int *list);
Their arguments are identical to those for the *pack_forward_grid()*
and *unpack_forward_grid()* callback functions (or the reverse
variants) discussed above. Normally, both these methods pack/unpack
all the data arrays for a given grid. The *which* argument of the
*remap()* method sets the *which* value for the pack/unpack functions.
If the command instantiates multiple grids (of different sizes), it
can be used within the pack/unpack methods to select which grid's data
is being remapped.
Note that the *pack_remap_grid()* function must copy values from the
OLD grid data arrays into the *vbuf* buffer. The *unpack_remap_grid()*
function must copy values from the *vbuf* buffer into the NEW grid
data arrays.
After the remap operation for grid cell data has been performed, the
*reset_grid()* method can deallocate the two remap buffers it created,
and can then exit.
----------
Grid class I/O methods
^^^^^^^^^^^^^^^^^^^^^^
There are two I/O methods in the Grid classes which can be used to
read and write grid cell data to files. The caller can decide on the
precise format of each file, e.g. whether header lines are prepended
or comment lines are allowed. Fundamentally, the file should contain
one line per grid cell for the entire global grid. Each line should
contain identifying info as to which grid cell it is, e.g. a unique
grid cell ID or the ix,iy,iz indices of the cell within a 3d grid.
The line should also contain one or more data values which are stored
within the grid data arrays created by the command
For grid cell IDs, the LAMMPS convention is that the IDs run from 1 to
N, where N = Nx * Ny for 2d grids and N = Nx * Ny * Nz for 3d grids.
The x-index of the grid cell varies fastest, then y, and the z-index
varies slowest. So for a 10x10x10 grid the cell IDs from 901-1000
would be in the top xy layer of the z dimension.
The *read_file()* method does something simple. It reads a chunk of
consecutive lines from the file and passes them back to the caller to
process. The caller provides a *unpack_read_grid()* function for this
purpose. The function checks the grid cell ID or indices and only
stores grid cell data for the grid cells it owns.
The *write_file()* method does something slightly more complex. Each
processor packs the data for its owned grid cells into a buffer. The
caller provides a *pack_write_grid()* function for this purpose. The
*write_file()* method then loops over all processors and each sends
its buffer one at a time to processor 0, along with the 3d (or 2d)
index bounds of its grid cell data within the global grid. Processor
0 calls back to the *unpack_write_grid()* function provided by the
caller with the buffer. The function writes one line per grid cell to
the file.
See the src/EXTRA_FIX/fix_ttm_grid.cpp file for examples of now both
these methods are used to read/write electron temperature values
from/to a file, as well as for implementations of the the pack/unpack
functions described below.
Here are the details of the two I/O methods and the 3 callback
functions. See the src/fix_ave_grid.cpp file for examples of all of
them.
.. code-block:: c++
void read_file(int caller, void *ptr, FILE *fp, int nchunk, int maxline)
void write_file(int caller, void *ptr, int which,
int nper, int nbyte, MPI_Datatype datatype
The *caller* argument in both methods should be one of these values --
Grid3d::COMPUTE, Grid3d::FIX, Grid3d::KSPACE, Grid3d::PAIR --
depending on the style of the caller class. The *ptr* argument in
both methods is the "this" pointer to the caller class. These 2
arguments are used to call back to pack()/unpack() functions in the
caller class, as explained below.
For the *read_file()* method, the *fp* argument is a file pointer to
the file to be read from, opened on processor 0 by the caller.
*Nchunk* is the number of lines to read per chunk, and *maxline* is
the maximum number of characters per line. The Grid class will
allocate a buffer for storing chunks of lines based on these values.
For the *write_file()* method, the *which* argument is a flag the
caller can set which is passed back to the caller's pack()/unpack()
methods. If the command instantiates multiple grids (of different
sizes), this flag can be used within the pack/unpack methods to select
which grid's data is being written out (presumably to different
files). the *nper* argument is the number of values per grid cell to
be written out. The *nbyte* argument is the number of bytes per
value, e.g. 8 for double-precision values. The *datatype* argument is
the MPI_Datatype setting, which should match the *nbyte* argument.
E.g. MPI_DOUBLE for double precision values.
To use the *read_grid()* method, the caller must provide one callback
function. To use the *write_grid()* method, it provides two callback
functions:
.. code-block:: c++
int unpack_read_grid(int nlines, char *buffer)
void pack_write_grid(int which, void *vbuf)
void unpack_write_grid(int which, void *vbuf, int *bounds)
For *unpack_read_grid()* the *nlines* argument is the number of lines
of character data read from the file and contained in *buffer*. The
lines each include a newline character at the end. When the function
processes the lines, it may choose to skip some of them (header or
comment lines). It returns an integer count of the number of grid
cell lines it processed. This enables the Grid class *read_file()*
method to know when it has read the correct number of lines.
For *pack_write_grid()* and *unpack_write_grid()*, the *vbuf* argument
is the buffer to pack/unpack data to/from. It is a void pointer so
that the caller can cast it to whatever data type it chooses,
e.g. double precision values. the *which* argument is set to the
*which* value of the *write_file()* method. It allows the caller to
choose which grid data to operate on.
For *unpack_write_grid()*, the *bounds* argument is a vector of 4 or 6
integer grid indices (4 for 2d, 6 for 3d). They are the
xlo,xhi,ylo,yhi,zlo,zhi index bounds of the portion of the global grid
which the *vbuf* holds owned grid cell data values for. The caller
should loop over the values in *vbuf* with a double loop (2d) or
triple loop (3d), similar to the code snippets listed above. The
x-index varies fastest, then y, and the z-index slowest. If there are
multiple values per grid cell, the index for those values varies
fastest of all. The caller can add the x,y,z indices of the grid cell
(or the corresponding grid cell ID) to the data value(s) written as
one line to the output file.
----------
Style class grid access methods
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
A style command can enable its grid cell data to be accessible from
other commands. For example :doc:`fix ave/grid <fix_ave_grid>` or
:doc:`dump grid <dump>` or :doc:`dump grid/vtk <dump>`. Those
commands access the grid cell data by using a *grid reference* in
their input script syntax, as described on the :doc:`Howto_grid
<Howto_grid>` doc page. They look like this:
* c_ID:gname:dname
* c_ID:gname:dname[I]
* f_ID:gname:dname
* f_ID:gname:dname[I]
Each grid a command instantiates has a unique *gname*, defined by the
command. Likewise each grid cell data structure (scalar or vector)
associated with a grid has a unique *dname*, also defined by the
command.
To provide access to its grid cell data, a style command needs to
implement the following 4 methods:
.. code-block:: c++
int get_grid_by_name(const std::string &name, int &dim);
void *get_grid_by_index(int index);
int get_griddata_by_name(int igrid, const std::string &name, int &ncol);
void *get_griddata_by_index(int index);
Currently only computes and fixes can implement these methods. If it
does so, the compute of fix should also set the variable
*pergrid_flag* to 1. See any of the compute or fix commands which set
"pergrid_flag = 1" for examples of how these 4 functions can be
implemented.
The *get_grid_by_name()* method takes a grid name as input and returns
two values. The *dim* argument is returned as 2 or 3 for the
dimensionality of the grid. The function return is a grid index from
0 to G-1 where *G* is the number of grids the command instantiates. A
value of -1 is returned if the grid name is not recognized.
The *get_grid_by_index()* method is called after the
*get_grid_by_name()* method, using the grid index it returned as its
argument. This method will return a pointer to the Grid2d or Grid3d
class. The caller can use this to query grid attributes, such as the
global size of the grid. The :doc:`dump grid <dump>` to insure each
its grid reference arguments are for grids of the same size.
The *get_griddata_by_name()* method takes a grid index *igrid* and a
data name as input. It returns two values. The *ncol* argument is
returned as a 0 if the grid data is a single value (scalar) per grid
cell, or an integer M > 0 if there are M values (vector) per grid
cell. Note that even if M = 1, it is still a 1-length vector, not a
scalar. The function return is a data index from 0 to D-1 where *D*
is the number of data sets associated with that grid by the command.
A value of -1 is returned if the data name is not recognized.
The *get_griddata_by_index()* method is called after the
*get_griddata_by_name()* method, using the data index it returned as
its argument. This method will return a pointer to the
multi-dimensional array which stores the requested data.
As in the discussion above of the Memory class *create_offset()*
methods, the dimensionality of the array associated with the returned
pointer depends on whether it is a 2d or 3d grid and whether there is
a single or multiple values stored for each grid cell:
* single value per cell for a 2d grid = 2d array pointer
* multiple values per cell for a 2d grid = 3d array pointer
* single value per cell for a 3d grid = 3d array pointer
* multiple values per cell for a 3d grid = 4d array pointer
The caller will typically access the data by casting the void pointer
to the corresponding array pointer and using nested loops in x,y,z
between owned or ghost index bounds returned by the
*get_bounds_owned()* or *get_bounds_ghost()* methods to index into the
array. Example code snippets with this logic were listed above,
----------
Final notes
^^^^^^^^^^^
Finally, here are some additional issues to pay attention to for
writing any style command which uses distributed grids via the Grid2d
or Grid3d class.
The command destructor should delete all instances of the Grid class,
any buffers it allocated for forward/reverse or remap communication,
and any data arrays it allocated to store grid cell data.
If a command is intended to work for either 2d or 3d simulations, then
it should have logic to instantiate either 2d or 3d grids and their
associated data arrays, depending on the dimension of the simulation
box. The :doc:`fix ave/grid <fix_ave_grid>` command is an example of
such a command.
When a command maps its particles to the grid and updates grid cell
values, it should check that it is not updating or accessing a grid
cell value outside the range of its owned+ghost cells, and generate an
error message if that is the case. This could happen, for example, if
a particle has moved further than half the neighbor skin distance,
because the neighbor list update criterion are not adequate to prevent
it from happening. See the src/KSPACE/pppm.cpp file and its
*particle_map()* method for an example of this kind of error check.

16
doc/src/Developer_notes.rst
View File

@ -105,7 +105,7 @@ list, where each pair of atoms is listed only once (except when the
pairs straddling sub-domains or periodic boundaries will be listed twice).
Thus these are the default settings when a neighbor list request is created in:
.. code-block:: C++
.. code-block:: c++
void Pair::init_style()
{
@ -129,7 +129,7 @@ neighbor list request to the specific needs of a style an additional
request flag is needed. The :doc:`tersoff <pair_tersoff>` pair style,
for example, needs a "full" neighbor list:
.. code-block:: C++
.. code-block:: c++
void PairTersoff::init_style()
{
@ -141,7 +141,7 @@ When a pair style supports r-RESPA time integration with different cutoff region
the request flag may depend on the corresponding r-RESPA settings. Here an example
from pair style lj/cut:
.. code-block:: C++
.. code-block:: c++
void PairLJCut::init_style()
{
@ -160,7 +160,7 @@ Granular pair styles need neighbor lists based on particle sizes and not cutoff
and also may require to have the list of previous neighbors available ("history").
For example with:
.. code-block:: C++
.. code-block:: c++
if (use_history) neighbor->add_request(this, NeighConst::REQ_SIZE | NeighConst::REQ_HISTORY);
else neighbor->add_request(this, NeighConst::REQ_SIZE);
@ -170,7 +170,7 @@ settings each request can set an id which is then used in the corresponding
``init_list()`` function to assign it to the suitable pointer variable. This is
done for example by the :doc:`pair style meam <pair_meam>`:
.. code-block:: C++
.. code-block:: c++
void PairMEAM::init_style()
{
@ -189,7 +189,7 @@ just once) and this can also be indicated by a flag. As an example here
is the request from the ``FixPeriNeigh`` class which is created
internally by :doc:`Peridynamics pair styles <pair_peri>`:
.. code-block:: C++
.. code-block:: c++
neighbor->add_request(this, NeighConst::REQ_FULL | NeighConst::REQ_OCCASIONAL);
@ -198,7 +198,7 @@ than what is usually inferred from the pair style settings (largest cutoff of
all pair styles plus neighbor list skin). The following is used in the
:doc:`compute rdf <compute_rdf>` command implementation:
.. code-block:: C++
.. code-block:: c++
if (cutflag)
neighbor->add_request(this, NeighConst::REQ_OCCASIONAL)->set_cutoff(mycutneigh);
@ -212,7 +212,7 @@ for printing the neighbor list summary the name of the requesting command
should be set. Below is the request from the :doc:`delete atoms <delete_atoms>`
command:
.. code-block:: C++
.. code-block:: c++
neighbor->add_request(this, "delete_atoms", NeighConst::REQ_FULL);

6
doc/src/Developer_plugins.rst
View File

@ -95,7 +95,7 @@ a class ``PairMorse2`` in the files ``pair_morse2.h`` and
``pair_morse2.cpp`` with the factory function and initialization
function would look like this:
.. code-block:: C++
.. code-block:: c++
#include "lammpsplugin.h"
#include "version.h"
@ -141,7 +141,7 @@ list of argument strings), then the pointer type is ``lammpsplugin_factory2``
and it must be assigned to the *creator.v2* member of the plugin struct.
Below is an example for that:
.. code-block:: C++
.. code-block:: c++
#include "lammpsplugin.h"
#include "version.h"
@ -176,7 +176,7 @@ demonstrated in the following example, which also shows that the
implementation of the plugin class may be within the same source
file as the plugin interface code:
.. code-block:: C++
.. code-block:: c++
#include "lammpsplugin.h"

10
doc/src/Developer_unittest.rst
View File

@ -194,7 +194,7 @@ macro. These tests operate by capturing the screen output when executing
the failing command and then comparing that with a provided regular
expression string pattern. Example:
.. code-block:: C++
.. code-block:: c++
TEST_F(SimpleCommandsTest, UnknownCommand)
{
@ -226,9 +226,9 @@ The following test programs are currently available:
* - ``test_kim_commands.cpp``
- KimCommands
- Tests for several commands from the :ref:`KIM package <PKG-KIM>`
* - ``test_reset_ids.cpp``
- ResetIDs
- Tests to validate the :doc:`reset_atom_ids <reset_atom_ids>` and :doc:`reset_mol_ids <reset_mol_ids>` commands
* - ``test_reset_atoms.cpp``
- ResetAtoms
- Tests to validate the :doc:`reset_atoms <reset_atoms>` sub-commands
Tests for the C-style library interface
@ -249,7 +249,7 @@ MPI support. These include tests where LAMMPS is run in multi-partition
mode or only on a subset of the MPI world communicator. The CMake
script code for adding this kind of test looks like this:
.. code-block:: CMake
.. code-block:: cmake
if (BUILD_MPI)
add_executable(test_library_mpi test_library_mpi.cpp)

100
doc/src/Developer_updating.rst
View File

@ -7,7 +7,7 @@ source files provided as a supplement to a publication) that are written
for an older version of LAMMPS and thus need to be updated to be
compatible with the current version of LAMMPS. Due to the active
development of LAMMPS it is likely to always be incomplete. Please
contact developer@lammps.org in case you run across an issue that is not
contact developers@lammps.org in case you run across an issue that is not
(yet) listed here. Please also review the latest information about the
LAMMPS :doc:`programming style conventions <Modify_style>`, especially
if you are considering to submit the updated version for inclusion into
@ -25,6 +25,7 @@ Available topics in mostly chronological order are:
- `Simplified and more compact neighbor list requests`_
- `Split of fix STORE into fix STORE/GLOBAL and fix STORE/PERATOM`_
- `Use Output::get_dump_by_id() instead of Output::find_dump()`_
- `Refactored grid communication using Grid3d/Grid2d classes instead of GridComm`_
----
@ -61,7 +62,7 @@ header file needs to be updated accordingly.
Old:
.. code-block:: C++
.. code-block:: c++
int PairEAM::pack_comm(int n, int *list, double *buf, int pbc_flag, int *pbc)
{
@ -75,7 +76,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
int PairEAM::pack_forward_comm(int n, int *list, double *buf, int pbc_flag, int *pbc)
{
@ -112,14 +113,14 @@ Example from a pair style:
Old:
.. code-block:: C++
.. code-block:: c++
if (eflag || vflag) ev_setup(eflag, vflag);
else evflag = vflag_fdotr = eflag_global = eflag_atom = 0;
New:
.. code-block:: C++
.. code-block:: c++
ev_init(eflag, vflag);
@ -142,14 +143,14 @@ when they are called from only one or a subset of the MPI processes.
Old:
.. code-block:: C++
.. code-block:: c++
val = force->numeric(FLERR, arg[1]);
num = force->inumeric(FLERR, arg[2]);
New:
.. code-block:: C++
.. code-block:: c++
val = utils::numeric(FLERR, true, arg[1], lmp);
num = utils::inumeric(FLERR, false, arg[2], lmp);
@ -183,14 +184,14 @@ copy them around for simulations.
Old:
.. code-block:: C++
.. code-block:: c++
fp = force->open_potential(filename);
fp = fopen(filename, "r");
New:
.. code-block:: C++
.. code-block:: c++
fp = utils::open_potential(filename, lmp);
@ -207,7 +208,7 @@ Example:
Old:
.. code-block:: C++
.. code-block:: c++
if (fptr == NULL) {
char str[128];
@ -217,7 +218,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
if (fptr == nullptr)
error->one(FLERR, "Cannot open AEAM potential file {}: {}", filename, utils::getsyserror());
@ -237,7 +238,7 @@ an example from the ``FixWallReflect`` class:
Old:
.. code-block:: C++
.. code-block:: c++
FixWallReflect(class LAMMPS *, int, char **);
virtual ~FixWallReflect();
@ -247,7 +248,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
FixWallReflect(class LAMMPS *, int, char **);
~FixWallReflect() override;
@ -271,7 +272,7 @@ the type of the "this" pointer argument.
Old:
.. code-block:: C++
.. code-block:: c++
comm->forward_comm_pair(this);
comm->forward_comm_fix(this);
@ -284,7 +285,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
comm->forward_comm(this);
comm->reverse_comm(this);
@ -304,7 +305,7 @@ requests can be :doc:`found here <Developer_notes>`. Example from the
Old:
.. code-block:: C++
.. code-block:: c++
int irequest = neighbor->request(this,instance_me);
neighbor->requests[irequest]->pair = 0;
@ -317,7 +318,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
auto req = neighbor->add_request(this, NeighConst::REQ_OCCASIONAL);
if (cutflag) req->set_cutoff(mycutneigh);
@ -340,7 +341,7 @@ these are internal fixes, there is no user visible change.
Old:
.. code-block:: C++
.. code-block:: c++
#include "fix_store.h"
@ -351,7 +352,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
#include "fix_store_peratom.h"
@ -362,7 +363,7 @@ New:
Old:
.. code-block:: C++
.. code-block:: c++
#include "fix_store.h"
@ -373,7 +374,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
#include "fix_store_global.h"
@ -396,7 +397,7 @@ the dump directly. Example:
Old:
.. code-block:: C++
.. code-block:: c++
int idump = output->find_dump(arg[iarg+1]);
if (idump < 0)
@ -412,7 +413,7 @@ Old:
New:
.. code-block:: C++
.. code-block:: c++
auto idump = output->get_dump_by_id(arg[iarg+1]);
if (!idump) error->all(FLERR,"Dump ID {} in hyper command does not exist", arg[iarg+1]);
@ -423,3 +424,56 @@ New:
if (dumpflag) for (auto idump : dumplist) idump->write();
This change is **required** or else the code will not compile.
Refactored grid communication using Grid3d/Grid2d classes instead of GridComm
^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^
.. versionchanged:: 22Dec2022
The ``GridComm`` class was for creating and communicating distributed
grids was replaced by the ``Grid3d`` class with added functionality.
A ``Grid2d`` class was also added for additional flexibility.
The new functionality and commands using the two grid classes are
discussed on the following documentation pages:
- :doc:`Howto_grid`
- :doc:`Developer_grid`
If you have custom LAMMPS code, which uses the GridComm class, here are some notes
on how to adapt it for using the Grid3d class.
(1) The constructor has changed to allow the ``Grid3d`` / ``Grid2d``
classes to partition the global grid across processors, both for
owned and ghost grid cells. Previously any class which called
``GridComm`` performed the partitioning itself and that information
was passed in the ``GridComm::GridComm()`` constructor. There are
several "set" functions which can be called to alter how ``Grid3d``
/ ``Grid2d`` perform the partitioning. They should be sufficient
for most use cases of the grid classes.
(2) The partitioning is triggered by the ``setup_grid()`` method.
(3) The ``setup()`` method of the ``GridComm`` class has been replaced
by the ``setup_comm()`` method in the new grid classes. The syntax
for the ``forward_comm()`` and ``reverse_comm()`` methods is
slightly altered as is the syntax of the associated pack/unpack
callback methods. But the functionality of these operations is the
same as before.
(4) The new ``Grid3d`` / ``Grid2d`` classes have additional
functionality for dynamic load-balancing of grids and their
associated data across processors. This did not exist in the
``GridComm`` class.
This and more is explained in detail on the :doc:`Developer_grid` page.
The following LAMMPS source files can be used as illustrative examples
for how the new grid classes are used by computes, fixes, and various
KSpace solvers which use distributed FFT grids:
- ``src/fix_ave_grid.cpp``
- ``src/compute_property_grid.cpp``
- ``src/EXTRA-FIX/fix_ttm_grid.cpp``
- ``src/KSPACE/pppm.cpp``
This change is **required** or else the code will not compile.

16
doc/src/Developer_utils.rst
View File

@ -133,6 +133,9 @@ and parsing files or arguments.
.. doxygenfunction:: trim_comment
:project: progguide
.. doxygenfunction:: strip_style_suffix
:project: progguide
.. doxygenfunction:: star_subst
:project: progguide
@ -211,6 +214,9 @@ Argument processing
.. doxygenfunction:: expand_args
:project: progguide
.. doxygenfunction:: parse_grid_id
:project: progguide
.. doxygenfunction:: expand_type
:project: progguide
@ -317,7 +323,7 @@ are all "whitespace" characters, i.e. the space character, the tabulator
character, the carriage return character, the linefeed character, and
the form feed character.
.. code-block:: C++
.. code-block:: c++
:caption: Tokenizer class example listing entries of the PATH environment variable
#include "tokenizer.h"
@ -349,7 +355,7 @@ tokenizer into a ``try`` / ``catch`` block to handle errors. The
when a (type of) number is requested as next token that is not
compatible with the string representing the next word.
.. code-block:: C++
.. code-block:: c++
:caption: ValueTokenizer class example with exception handling
#include "tokenizer.h"
@ -427,7 +433,7 @@ one or two array indices "[<number>]" with numbers > 0.
A typical code segment would look like this:
.. code-block:: C++
.. code-block:: c++
:caption: Usage example for ArgInfo class
int nvalues = 0;
@ -476,7 +482,7 @@ open the file, and will call the :cpp:class:`LAMMPS_NS::Error` class in
case of failures to read or to convert numbers, so that LAMMPS will be
aborted.
.. code-block:: C++
.. code-block:: c++
:caption: Use of PotentialFileReader class in pair style coul/streitz
PotentialFileReader reader(lmp, file, "coul/streitz");
@ -555,7 +561,7 @@ chunk size needs to be known in advance, 2) with :cpp:func:`MyPage::vget()
its size is registered later with :cpp:func:`MyPage::vgot()
<LAMMPS_NS::MyPage::vgot>`.
.. code-block:: C++
.. code-block:: c++
:caption: Example of using :cpp:class:`MyPage <LAMMPS_NS::MyPage>`
#include "my_page.h"

14
doc/src/Developer_write.rst
View File

@ -26,7 +26,7 @@ constructor with the signature: ``FixPrintVel(class LAMMPS *, int, char **)``.
Every fix must be registered in LAMMPS by writing the following lines
of code in the header before include guards:
.. code-block:: c
.. code-block:: c++
#ifdef FIX_CLASS
// clang-format off
@ -47,7 +47,7 @@ keyword when it parses the input script.
Let's write a simple fix which will print the average velocity at the end
of each timestep. First of all, implement a constructor:
.. code-block:: C++
.. code-block:: c++
FixPrintVel::FixPrintVel(LAMMPS *lmp, int narg, char **arg)
: Fix(lmp, narg, arg)
@ -72,7 +72,7 @@ in the Fix class called ``nevery`` which specifies how often the method
The next method we need to implement is ``setmask()``:
.. code-block:: C++
.. code-block:: c++
int FixPrintVel::setmask()
{
@ -87,7 +87,7 @@ during execution. The constant ``END_OF_STEP`` corresponds to the
are called during a timestep and the order in which they are called
are shown in the previous section.
.. code-block:: C++
.. code-block:: c++
void FixPrintVel::end_of_step()
{
@ -143,7 +143,7 @@ The group membership information of an atom is contained in the *mask*
property of and atom and the bit corresponding to a given group is
stored in the groupbit variable which is defined in Fix base class:
.. code-block:: C++
.. code-block:: c++
for (int i = 0; i < nlocal; ++i) {
if (atom->mask[i] & groupbit) {
@ -174,7 +174,7 @@ to store positions of atoms from previous timestep, we need to add
``double** xold`` to the header file. Than add allocation code
to the constructor:
.. code-block:: C++
.. code-block:: c++
FixSavePos::FixSavePos(LAMMPS *lmp, int narg, char **arg), xold(nullptr)
{
@ -190,7 +190,7 @@ to the constructor:
Implement the aforementioned methods:
.. code-block:: C++
.. code-block:: c++
double FixSavePos::memory_usage()
{

1823
doc/src/Fortran.rst
View File

File diff suppressed because it is too large Load Diff

1
doc/src/Howto.rst
View File

@ -51,6 +51,7 @@ Analysis howto
Howto_output
Howto_chunk
Howto_grid
Howto_temperature
Howto_elastic
Howto_kappa

102
doc/src/Howto_grid.rst Normal file
View File

@ -0,0 +1,102 @@
Using distributed grids
=======================
.. versionadded:: 22Dec2022
LAMMPS has internal capabilities to create uniformly spaced grids
which overlay the simulation domain. For 2d and 3d simulations these
are 2d and 3d grids respectively. Conceptually a grid can be thought
of as a collection of grid cells. Each grid cell can store one or
more values (data).
The grid cells and data they store are distributed across processors.
Each processor owns the grid cells (and data) whose center points lie
within the spatial sub-domain of the processor. If needed for its
computations, a processor may also store ghost grid cells with their
data.
Distributed grids can overlay orthogonal or triclinic simulation
boxes; see the :doc:`Howto triclinic <Howto_triclinic>` doc page for
an explanation of the latter. For a triclinic box, the grid cell
shape conforms to the shape of the simulation domain,
e.g. parallelograms instead of rectangles in 2d.
If the box size or shape changes during a simulation, the grid changes
with it, so that it always overlays the entire simulation domain. For
non-periodic dimensions, the grid size in that dimension matches the
box size, as set by the :doc:`boundary <boundary>` command for fixed
or shrink-wrapped boundaries.
If load-balancing is invoked by the :doc:`balance <balance>` or
:doc:`fix balance <fix_balance>` commands, then the sub-domain owned
by a processor can change which may also change which grid cells they
own.
Post-processing and visualization of grid cell data can be enabled by
the :doc:`dump grid <dump>`, :doc:`dump grid/vtk <dump>`, and
:doc:`dump image <dump_image>` commands. The latter has an optional
*grid* keyword. The `OVITO visualization tool
<https://www.ovito.org>`_ also plans (as of Nov 2022) to add support
for visualizing grid cell data (along with atoms) using :doc:`dump
grid <dump>` output files as input.
.. note::
For developers, distributed grids are implemented within the code via
two classes: Grid2d and Grid3d. These partition the grid across
processors and have methods which allow forward and reverse
communication of ghost grid data as well as load balancing. If you
write a new compute or fix which needs a distributed grid, these are
the classes to look at. A new pair style could use a distributed
grid by having a fix define it. Please see the section on
:doc:`using distributed grids within style classes <Developer_grid>`
for a detailed description.
----------
These are the commands which currently define or use distributed
grids:
* :doc:`fix ttm/grid <fix_ttm>` - store electron temperature on grid
* :doc:`fix ave/grid <fix_ave_grid>` - time average per-atom or per-grid values
* :doc:`compute property/grid <compute_property_grid>` - generate grid IDs and coords
* :doc:`dump grid <dump>` - output per-grid values in LAMMPS format
* :doc:`dump grid/vtk <dump>` - output per-grid values in VTK format
* :doc:`dump image grid <dump_image>` - include colored grid in output images
* :doc:`pair_style amoeba <pair_amoeba>` - FFT grids
* :doc:`kspace_style pppm <kspace_style>` (and variants) - FFT grids
* :doc:`kspace_style msm <kspace_style>` (and variants) - MSM grids
The grids used by the :doc:`kspace_style <kspace_style>` can not be
referenced by an input script. However the grids and data created and
used by the other commands can be.
A compute or fix command may create one or more grids (of different
sizes). Each grid can store one or more data fields. A data field
can be a single value per grid point (per-grid vector) or multiple
values per grid point (per-grid array). See the :doc:`Howto output
<Howto_output>` doc page for an explanation of how per-grid data can
be generated by some commands and used by other commands.
A command accesses grid data from a compute or fix using a *grid
reference* with the following syntax:
* c_ID:gname:dname
* c_ID:gname:dname[I]
* f_ID:gname:dname
* f_ID:gname:dname[I]
The prefix "c\_" or "f\_" refers to the ID of the compute or fix; gname is
the name of the grid, which is assigned by the compute or fix; dname is
the name of the data field, which is also assigned by the compute or
fix.
If the data field is a per-grid vector (one value per grid point),
then no brackets are used to access the values. If the data field is
a per-grid array (multiple values per grid point), then brackets are
used to specify the column I of the array. I ranges from 1 to Ncol
inclusive, where Ncol is the number of columns in the array and is
defined by the compute or fix.
Currently, there are no per-grid variables implemented in LAMMPS. We
may add this feature at some point.

329
doc/src/Howto_output.rst
View File

@ -22,14 +22,17 @@ commands you specify.
As discussed below, LAMMPS gives you a variety of ways to determine
what quantities are computed and printed when the thermodynamics,
dump, or fix commands listed above perform output. Throughout this
discussion, note that users can also :doc:`add their own computes and fixes to LAMMPS <Modify>` which can then generate values that can then be
output with these commands.
discussion, note that users can also :doc:`add their own computes and
fixes to LAMMPS <Modify>` which can then generate values that can then
be output with these commands.
The following sub-sections discuss different LAMMPS command related
The following sub-sections discuss different LAMMPS commands related
to output and the kind of data they operate on and produce:
* :ref:`Global/per-atom/local data <global>`
* :ref:`Global/per-atom/local/per-grid data <global>`
* :ref:`Scalar/vector/array data <scalar>`
* :ref:`Per-grid data <grid>`
* :ref:`Disambiguation <disambiguation>`
* :ref:`Thermodynamic output <thermo>`
* :ref:`Dump file output <dump>`
* :ref:`Fixes that write output files <fixoutput>`
@ -42,27 +45,32 @@ to output and the kind of data they operate on and produce:
.. _global:
Global/per-atom/local data
--------------------------
Global/per-atom/local/per-grid data
-----------------------------------
Various output-related commands work with three different styles of
data: global, per-atom, or local. A global datum is one or more
system-wide values, e.g. the temperature of the system. A per-atom
datum is one or more values per atom, e.g. the kinetic energy of each
atom. Local datums are calculated by each processor based on the
atoms it owns, but there may be zero or more per atom, e.g. a list of
bond distances.
Various output-related commands work with four different styles of
data: global, per-atom, local, and per-grid. A global datum is one or
more system-wide values, e.g. the temperature of the system. A
per-atom datum is one or more values per atom, e.g. the kinetic energy
of each atom. Local datums are calculated by each processor based on
the atoms it owns, but there may be zero or more per atom, e.g. a list
of bond distances.
A per-grid datum is one or more values per grid cell, for a grid which
overlays the simulation domain. The grid cells and the data they
store are distributed across processors; each processor owns the grid
cells whose center point falls within its sub-domain.
.. _scalar:
Scalar/vector/array data
------------------------
Global, per-atom, and local datums can each come in three kinds: a
single scalar value, a vector of values, or a 2d array of values. The
doc page for a "compute" or "fix" or "variable" that generates data
will specify both the style and kind of data it produces, e.g. a
per-atom vector.
Global, per-atom, and local datums can come in three kinds: a single
scalar value, a vector of values, or a 2d array of values. The doc
page for a "compute" or "fix" or "variable" that generates data will
specify both the style and kind of data it produces, e.g. a per-atom
vector.
When a quantity is accessed, as in many of the output commands
discussed below, it can be referenced via the following bracket
@ -83,6 +91,18 @@ the dimension twice (array -> scalar). Thus a command that uses
scalar values as input can typically also process elements of a vector
or array.
.. _grid:
Per-grid data
------------------------
Per-grid data can come in two kinds: a vector of values (one per grid
cekk), or a 2d array of values (multiple values per grid ckk). The
doc page for a "compute" or "fix" that generates data will specify
names for both the grid(s) and datum(s) it produces, e.g. per-grid
vectors or arrays, which can be referenced by other commands. See the
:doc:`Howto grid <Howto_grid>` doc page for more details.
.. _disambiguation:
Disambiguation
@ -90,15 +110,15 @@ Disambiguation
Some computes and fixes produce data in multiple styles, e.g. a global
scalar and a per-atom vector. Usually the context in which the input
script references the data determines which style is meant. Example: if
a compute provides both a global scalar and a per-atom vector, the
script references the data determines which style is meant. Example:
if a compute provides both a global scalar and a per-atom vector, the
former will be accessed by using ``c_ID`` in an equal-style variable,
while the latter will be accessed by using ``c_ID`` in an atom-style
variable. Note that atom-style variable formulas can also access global
scalars, but in this case it is not possible to do directly because of
the ambiguity. Instead, an equal-style variable can be defined which
accesses the global scalar, and that variable used in the atom-style
variable formula in place of ``c_ID``.
variable. Note that atom-style variable formulas can also access
global scalars, but in this case it is not possible to do this
directly because of the ambiguity. Instead, an equal-style variable
can be defined which accesses the global scalar, and that variable can
be used in the atom-style variable formula in place of ``c_ID``.
.. _thermo:
@ -107,15 +127,14 @@ Thermodynamic output
The frequency and format of thermodynamic output is set by the
:doc:`thermo <thermo>`, :doc:`thermo_style <thermo_style>`, and
:doc:`thermo_modify <thermo_modify>` commands. The
:doc:`thermo_style <thermo_style>` command also specifies what values
are calculated and written out. Pre-defined keywords can be specified
(e.g. press, etotal, etc). Three additional kinds of keywords can
also be specified (c_ID, f_ID, v_name), where a :doc:`compute <compute>`
or :doc:`fix <fix>` or :doc:`variable <variable>` provides the value to be
output. In each case, the compute, fix, or variable must generate
global values for input to the :doc:`thermo_style custom <dump>`
command.
:doc:`thermo_modify <thermo_modify>` commands. The :doc:`thermo_style
<thermo_style>` command also specifies what values are calculated and
written out. Pre-defined keywords can be specified (e.g. press, etotal,
etc). Three additional kinds of keywords can also be specified (c_ID,
f_ID, v_name), where a :doc:`compute <compute>` or :doc:`fix <fix>` or
:doc:`variable <variable>` provides the value to be output. In each
case, the compute, fix, or variable must generate global values for
input to the :doc:`thermo_style custom <dump>` command.
Note that thermodynamic output values can be "extensive" or
"intensive". The former scale with the number of atoms in the system
@ -141,9 +160,10 @@ There is also a :doc:`dump custom <dump>` format where the user
specifies what values are output with each atom. Pre-defined atom
attributes can be specified (id, x, fx, etc). Three additional kinds
of keywords can also be specified (c_ID, f_ID, v_name), where a
:doc:`compute <compute>` or :doc:`fix <fix>` or :doc:`variable <variable>`
provides the values to be output. In each case, the compute, fix, or
variable must generate per-atom values for input to the :doc:`dump custom <dump>` command.
:doc:`compute <compute>` or :doc:`fix <fix>` or :doc:`variable
<variable>` provides the values to be output. In each case, the
compute, fix, or variable must generate per-atom values for input to
the :doc:`dump custom <dump>` command.
There is also a :doc:`dump local <dump>` format where the user specifies
what local values to output. A pre-defined index keyword can be
@ -154,18 +174,23 @@ provides the values to be output. In each case, the compute or fix
must generate local values for input to the :doc:`dump local <dump>`
command.
There is also a :doc:`dump grid <dump>` format where the user
specifies what per-grid values to output from computes or fixes that
generate per-grid data.
.. _fixoutput:
Fixes that write output files
-----------------------------
Several fixes take various quantities as input and can write output
files: :doc:`fix ave/time <fix_ave_time>`, :doc:`fix ave/chunk <fix_ave_chunk>`, :doc:`fix ave/histo <fix_ave_histo>`,
:doc:`fix ave/correlate <fix_ave_correlate>`, and :doc:`fix print <fix_print>`.
files: :doc:`fix ave/time <fix_ave_time>`, :doc:`fix ave/chunk
<fix_ave_chunk>`, :doc:`fix ave/histo <fix_ave_histo>`, :doc:`fix
ave/correlate <fix_ave_correlate>`, and :doc:`fix print <fix_print>`.
The :doc:`fix ave/time <fix_ave_time>` command enables direct output to
a file and/or time-averaging of global scalars or vectors. The user
specifies one or more quantities as input. These can be global
The :doc:`fix ave/time <fix_ave_time>` command enables direct output
to a file and/or time-averaging of global scalars or vectors. The
user specifies one or more quantities as input. These can be global
:doc:`compute <compute>` values, global :doc:`fix <fix>` values, or
:doc:`variables <variable>` of any style except the atom style which
produces per-atom values. Since a variable can refer to keywords used
@ -184,8 +209,14 @@ atoms, e.g. individual molecules. The per-atom quantities can be atom
density (mass or number) or atom attributes such as position,
velocity, force. They can also be per-atom quantities calculated by a
:doc:`compute <compute>`, by a :doc:`fix <fix>`, or by an atom-style
:doc:`variable <variable>`. The chunk-averaged output of this fix can
also be used as input to other output commands.
:doc:`variable <variable>`. The chunk-averaged output of this fix is
global and can also be used as input to other output commands.
Note that the :doc:`fix ave/grid <fix_ave_grid>` command can also
average the same per-atom quantities within spatial bins, but it does
this for a distributed grid whose grid cells are owned by different
processors. It outputs per-grid data, not global data, so it is more
efficient for large numbers of averaging bins.
The :doc:`fix ave/histo <fix_ave_histo>` command enables direct output
to a file of histogrammed quantities, which can be global or per-atom
@ -202,38 +233,53 @@ written to the screen and log file or to a separate file, periodically
during a running simulation. The line can contain one or more
:doc:`variable <variable>` values for any style variable except the
vector or atom styles). As explained above, variables themselves can
contain references to global values generated by :doc:`thermodynamic keywords <thermo_style>`, :doc:`computes <compute>`,
:doc:`fixes <fix>`, or other :doc:`variables <variable>`, or to per-atom
values for a specific atom. Thus the :doc:`fix print <fix_print>`
command is a means to output a wide variety of quantities separate
from normal thermodynamic or dump file output.
contain references to global values generated by :doc:`thermodynamic
keywords <thermo_style>`, :doc:`computes <compute>`, :doc:`fixes
<fix>`, or other :doc:`variables <variable>`, or to per-atom values
for a specific atom. Thus the :doc:`fix print <fix_print>` command is
a means to output a wide variety of quantities separate from normal
thermodynamic or dump file output.
.. _computeoutput:
Computes that process output quantities
---------------------------------------
The :doc:`compute reduce <compute_reduce>` and :doc:`compute reduce/region <compute_reduce>` commands take one or more per-atom
or local vector quantities as inputs and "reduce" them (sum, min, max,
The :doc:`compute reduce <compute_reduce>` and :doc:`compute
reduce/region <compute_reduce>` commands take one or more per-atom or
local vector quantities as inputs and "reduce" them (sum, min, max,
ave) to scalar quantities. These are produced as output values which
can be used as input to other output commands.
The :doc:`compute slice <compute_slice>` command take one or more global
vector or array quantities as inputs and extracts a subset of their
values to create a new vector or array. These are produced as output
values which can be used as input to other output commands.
The :doc:`compute slice <compute_slice>` command take one or more
global vector or array quantities as inputs and extracts a subset of
their values to create a new vector or array. These are produced as
output values which can be used as input to other output commands.
The :doc:`compute property/atom <compute_property_atom>` command takes a
list of one or more pre-defined atom attributes (id, x, fx, etc) and
The :doc:`compute property/atom <compute_property_atom>` command takes
a list of one or more pre-defined atom attributes (id, x, fx, etc) and
stores the values in a per-atom vector or array. These are produced
as output values which can be used as input to other output commands.
The list of atom attributes is the same as for the :doc:`dump custom <dump>` command.
The list of atom attributes is the same as for the :doc:`dump custom
<dump>` command.
The :doc:`compute property/local <compute_property_local>` command takes
a list of one or more pre-defined local attributes (bond info, angle
info, etc) and stores the values in a local vector or array. These
are produced as output values which can be used as input to other
output commands.
The :doc:`compute property/local <compute_property_local>` command
takes a list of one or more pre-defined local attributes (bond info,
angle info, etc) and stores the values in a local vector or array.
These are produced as output values which can be used as input to
other output commands.
The :doc:`compute property/grid <compute_property_grid>` command takes
a list of one or more pre-defined per-grid attributes (id, grid cell
coords, etc) and stores the values in a per-grid vector or array.
These are produced as output values which can be used as input to the
:doc:`dump grid <dump>` command.
The :doc:`compute property/chunk <compute_property_chunk>` command
takes a list of one or more pre-defined chunk attributes (id, count,
coords for spatial bins) and stores the values in a global vector or
array. These are produced as output values which can be used as input
to other output commands.
.. _fixprocoutput:
@ -247,18 +293,42 @@ a time.
The :doc:`fix ave/atom <fix_ave_atom>` command performs time-averaging
of per-atom vectors. The per-atom quantities can be atom attributes
such as position, velocity, force. They can also be per-atom
quantities calculated by a :doc:`compute <compute>`, by a
:doc:`fix <fix>`, or by an atom-style :doc:`variable <variable>`. The
quantities calculated by a :doc:`compute <compute>`, by a :doc:`fix
<fix>`, or by an atom-style :doc:`variable <variable>`. The
time-averaged per-atom output of this fix can be used as input to
other output commands.
The :doc:`fix store/state <fix_store_state>` command can archive one or
more per-atom attributes at a particular time, so that the old values
can be used in a future calculation or output. The list of atom
attributes is the same as for the :doc:`dump custom <dump>` command,
including per-atom quantities calculated by a :doc:`compute <compute>`,
by a :doc:`fix <fix>`, or by an atom-style :doc:`variable <variable>`.
The output of this fix can be used as input to other output commands.
The :doc:`fix store/state <fix_store_state>` command can archive one
or more per-atom attributes at a particular time, so that the old
values can be used in a future calculation or output. The list of
atom attributes is the same as for the :doc:`dump custom <dump>`
command, including per-atom quantities calculated by a :doc:`compute
<compute>`, by a :doc:`fix <fix>`, or by an atom-style :doc:`variable
<variable>`. The output of this fix can be used as input to other
output commands.
The :doc:`fix ave/grid <fix_ave_grid>` command performs time-averaging
of either per-atom or per-grid data.
For per-atom data it performs averaging for the atoms within each grid
cell, similar to the :doc:`fix ave/chunk <fix_ave_chunk>` command when
its chunks are defined as regular 2d or 3d bins. The per-atom
quantities can be atom density (mass or number) or atom attributes
such as position, velocity, force. They can also be per-atom
quantities calculated by a :doc:`compute <compute>`, by a :doc:`fix
<fix>`, or by an atom-style :doc:`variable <variable>`.
The chief difference between the :doc:`fix ave/grid <fix_ave_grid>`
and :doc:`fix ave/chunk <fix_ave_chunk>` commands when used in this
context is that the former uses a distributed grid, while the latter
uses a global grid. Distributed means that each processor owns the
subset of grid cells within its sub-domain. Global means that each
processor owns a copy of the entire grid. The :doc:`fix ave/grid
<fix_ave_grid>` command is thus more efficient for large grids.
For per-grid data, the :doc:`fix ave/grid <fix_ave_grid>` command
takes inputs for grid data produced by other computes or fixes and
averages the values for each grid point over time.
.. _compute:
@ -266,24 +336,25 @@ Computes that generate values to output
---------------------------------------
Every :doc:`compute <compute>` in LAMMPS produces either global or
per-atom or local values. The values can be scalars or vectors or
arrays of data. These values can be output using the other commands
described in this section. The page for each compute command
per-atom or local or per-grid values. The values can be scalars or
vectors or arrays of data. These values can be output using the other
commands described in this section. The page for each compute command
describes what it produces. Computes that produce per-atom or local
values have the word "atom" or "local" in their style name. Computes
without the word "atom" or "local" produce global values.
or per-grid values have the word "atom" or "local" or "grid as the
last word in their style name. Computes without the word "atom" or
"local" or "grid" produce global values.
.. _fix:
Fixes that generate values to output
------------------------------------
Some :doc:`fixes <fix>` in LAMMPS produces either global or per-atom or
local values which can be accessed by other commands. The values can
be scalars or vectors or arrays of data. These values can be output
using the other commands described in this section. The page for
each fix command tells whether it produces any output quantities and
describes them.
Some :doc:`fixes <fix>` in LAMMPS produces either global or per-atom
or local or per-grid values which can be accessed by other commands.
The values can be scalars or vectors or arrays of data. These values
can be output using the other commands described in this section. The
page for each fix command tells whether it produces any output
quantities and describes them.
.. _variable:
@ -300,6 +371,8 @@ computes, fixes, and other variables. The values generated by
variables can be used as input to and thus output by the other
commands described in this section.
Per-grid variables have not (yet) been implemented.
.. _table:
Summary table of output options and data flow between commands
@ -319,44 +392,52 @@ Also note that, as described above, when a command takes a scalar as
input, that could be an element of a vector or array. Likewise a
vector input could be a column of an array.
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| Command | Input | Output |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`thermo_style custom <thermo_style>` | global scalars | screen, log file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`dump custom <dump>` | per-atom vectors | dump file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`dump local <dump>` | local vectors | dump file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix print <fix_print>` | global scalar from variable | screen, file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`print <print>` | global scalar from variable | screen |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`computes <compute>` | N/A | global/per-atom/local scalar/vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fixes <fix>` | N/A | global/per-atom/local scalar/vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`variables <variable>` | global scalars and vectors, per-atom vectors | global scalar and vector, per-atom vector |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`compute reduce <compute_reduce>` | per-atom/local vectors | global scalar/vector |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`compute slice <compute_slice>` | global vectors/arrays | global vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`compute property/atom <compute_property_atom>` | per-atom vectors | per-atom vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`compute property/local <compute_property_local>` | local vectors | local vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix vector <fix_vector>` | global scalars | global vector |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix ave/atom <fix_ave_atom>` | per-atom vectors | per-atom vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix ave/time <fix_ave_time>` | global scalars/vectors | global scalar/vector/array, file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix ave/chunk <fix_ave_chunk>` | per-atom vectors | global array, file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix ave/histo <fix_ave_histo>` | global/per-atom/local scalars and vectors | global array, file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix ave/correlate <fix_ave_correlate>` | global scalars | global array, file |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
| :doc:`fix store/state <fix_store_state>` | per-atom vectors | per-atom vector/array |
+--------------------------------------------------------+----------------------------------------------+-------------------------------------------+
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| Command | Input | Output |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`thermo_style custom <thermo_style>` | global scalars | screen, log file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`dump custom <dump>` | per-atom vectors | dump file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`dump local <dump>` | local vectors | dump file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`dump grid <dump>` | per-grid vectors | dump file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix print <fix_print>` | global scalar from variable | screen, file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`print <print>` | global scalar from variable | screen |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`computes <compute>` | N/A | global/per-atom/local/per-grid scalar/vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fixes <fix>` | N/A | global/per-atom/local/per-grid scalar/vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`variables <variable>` | global scalars and vectors, per-atom vectors | global scalar and vector, per-atom vector |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`compute reduce <compute_reduce>` | per-atom/local vectors | global scalar/vector |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`compute slice <compute_slice>` | global vectors/arrays | global vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`compute property/atom <compute_property_atom>` | N/A | per-atom vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`compute property/local <compute_property_local>` | N/A | local vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`compute property/grid <compute_property_grid>` | N/A | per-grid vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`compute property/chunk <compute_property_chunk>` | N/A | global vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix vector <fix_vector>` | global scalars | global vector |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix ave/atom <fix_ave_atom>` | per-atom vectors | per-atom vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix ave/time <fix_ave_time>` | global scalars/vectors | global scalar/vector/array, file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix ave/chunk <fix_ave_chunk>` | per-atom vectors | global array, file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix ave/grid <fix_ave_grid>` | per-atom vectors or per-grid vectors | per-grid vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix ave/histo <fix_ave_histo>` | global/per-atom/local scalars and vectors | global array, file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix ave/correlate <fix_ave_correlate>` | global scalars | global array, file |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+
| :doc:`fix store/state <fix_store_state>` | per-atom vectors | per-atom vector/array |
+--------------------------------------------------------+----------------------------------------------+----------------------------------------------------+

38
doc/src/Howto_pylammps.rst
View File

@ -152,14 +152,14 @@ Creating a new instance of PyLammps
To create a PyLammps object you need to first import the class from the lammps
module. By using the default constructor, a new *lammps* instance is created.
.. code-block:: Python
.. code-block:: python
from lammps import PyLammps
L = PyLammps()
You can also initialize PyLammps on top of this existing *lammps* object:
.. code-block:: Python
.. code-block:: python
from lammps import lammps, PyLammps
lmp = lammps()
@ -180,14 +180,14 @@ For instance, let's take the following LAMMPS command:
In the original interface this command can be executed with the following
Python code if *L* was a lammps instance:
.. code-block:: Python
.. code-block:: python
L.command("region box block 0 10 0 5 -0.5 0.5")
With the PyLammps interface, any command can be split up into arbitrary parts
separated by white-space, passed as individual arguments to a region method.
.. code-block:: Python
.. code-block:: python
L.region("box block", 0, 10, 0, 5, -0.5, 0.5)
@ -199,14 +199,14 @@ The benefit of this approach is avoiding redundant command calls and easier
parameterization. In the original interface parameterization needed to be done
manually by creating formatted strings.
.. code-block:: Python
.. code-block:: python
L.command("region box block %f %f %f %f %f %f" % (xlo, xhi, ylo, yhi, zlo, zhi))
In contrast, methods of PyLammps accept parameters directly and will convert
them automatically to a final command string.
.. code-block:: Python
.. code-block:: python
L.region("box block", xlo, xhi, ylo, yhi, zlo, zhi)
@ -256,7 +256,7 @@ LAMMPS variables can be both defined and accessed via the PyLammps interface.
To define a variable you can use the :doc:`variable <variable>` command:
.. code-block:: Python
.. code-block:: python
L.variable("a index 2")
@ -265,14 +265,14 @@ A dictionary of all variables is returned by L.variables
you can access an individual variable by retrieving a variable object from the
L.variables dictionary by name
.. code-block:: Python
.. code-block:: python
a = L.variables['a']
The variable value can then be easily read and written by accessing the value
property of this object.
.. code-block:: Python
.. code-block:: python
print(a.value)
a.value = 4
@ -284,7 +284,7 @@ LAMMPS expressions can be immediately evaluated by using the eval method. The
passed string parameter can be any expression containing global thermo values,
variables, compute or fix data.
.. code-block:: Python
.. code-block:: python
result = L.eval("ke") # kinetic energy
result = L.eval("pe") # potential energy
@ -298,7 +298,7 @@ All atoms in the current simulation can be accessed by using the L.atoms list.
Each element of this list is an object which exposes its properties (id, type,
position, velocity, force, etc.).
.. code-block:: Python
.. code-block:: python
# access first atom
L.atoms[0].id
@ -311,7 +311,7 @@ position, velocity, force, etc.).
Some properties can also be used to set:
.. code-block:: Python
.. code-block:: python
# set position in 2D simulation
L.atoms[0].position = (1.0, 0.0)
@ -328,7 +328,7 @@ after a run via the L.runs list. This list contains a growing list of run data.
The first element is the output of the first run, the second element that of
the second run.
.. code-block:: Python
.. code-block:: python
L.run(1000)
L.runs[0] # data of first 1000 time steps
@ -339,14 +339,14 @@ the second run.
Each run contains a dictionary of all trajectories. Each trajectory is
accessible through its thermo name:
.. code-block:: Python
.. code-block:: python
L.runs[0].thermo.Step # list of time steps in first run
L.runs[0].thermo.Ke # list of kinetic energy values in first run
Together with matplotlib plotting data out of LAMMPS becomes simple:
.. code-block:: Python
.. code-block:: python
import matplotlib.plot as plt
steps = L.runs[0].thermo.Step
@ -406,7 +406,7 @@ Four atoms are placed in the simulation and the dihedral potential is applied on
them using a datafile. Then one of the atoms is rotated along the central axis by
setting its position from Python, which changes the dihedral angle.
.. code-block:: Python
.. code-block:: python
phi = [d \* math.pi / 180 for d in range(360)]
@ -439,7 +439,7 @@ Initially, a 2D system is created in a state with minimal energy.
It is then disordered by moving each atom by a random delta.
.. code-block:: Python
.. code-block:: python
random.seed(27848)
deltaperturb = 0.2
@ -458,7 +458,7 @@ It is then disordered by moving each atom by a random delta.
Finally, the Monte Carlo algorithm is implemented in Python. It continuously
moves random atoms by a random delta and only accepts certain moves.
.. code-block:: Python
.. code-block:: python
estart = L.eval("pe")
elast = estart
@ -517,7 +517,7 @@ PyLammps can be run in parallel using mpi4py. This python package can be install
The following is a short example which reads in an existing LAMMPS input file and
executes it in parallel. You can find in.melt in the examples/melt folder.
.. code-block:: Python
.. code-block:: python
from mpi4py import MPI
from lammps import PyLammps

2
doc/src/Howto_structured_data.rst
View File

@ -43,7 +43,7 @@ JSON
"ke": $(ke)
}""" file current_state.json screen no
.. code-block:: JSON
.. code-block:: json
:caption: current_state.json
{

37
doc/src/Howto_tip4p.rst
View File

@ -8,18 +8,28 @@ This site M is located at a fixed distance away from the oxygen along
the bisector of the HOH bond angle. A bond style of *harmonic* and an
angle style of *harmonic* or *charmm* should also be used.
A TIP4P model is run with LAMMPS using either this command
A TIP4P model is run with LAMMPS using either these commands
for a cutoff model:
* :doc:`pair_style tip4p/cut <pair_lj_cut_tip4p>`
* :doc:`pair_style lj/cut/tip4p/cut <pair_lj_cut_tip4p>`
or these two commands for a long-range model:
or these commands for a long-range model:
* :doc:`pair_style tip4p/long <pair_coul>`
* :doc:`pair_style lj/cut/tip4p/long <pair_lj_cut_tip4p>`
* :doc:`pair_style lj/long/tip4p/long <pair_lj_long>`
* :doc:`pair_style tip4p/long/soft <pair_fep_soft>`
* :doc:`pair_style lj/cut/tip4p/long/soft <pair_fep_soft>`
* :doc:`kspace_style pppm/tip4p <kspace_style>`
* :doc:`kspace_style pppm/disp/tip4p <kspace_style>`
For both models, the bond lengths and bond angles should be held fixed
using the :doc:`fix shake <fix_shake>` command.
The bond lengths and bond angles should be held fixed using the
:doc:`fix shake <fix_shake>` or :doc:`fix rattle <fix_shake>` command,
unless a parameterization for a flexible TIP4P model is used. The
parameter sets listed below are all for rigid TIP4P model variants and
thus the bond and angle force constants are not used and can be set to
any legal value; only equilibrium length and angle are used.
These are the additional parameters (in real units) to set for O and H
atoms and the water molecule to run a rigid TIP4P model with a cutoff
@ -87,15 +97,16 @@ solver (e.g. Ewald or PPPM in LAMMPS):
| LJ :math:`\epsilon`, :math:`\sigma` of OH, HH = 0.0
|
Note that the when using the TIP4P pair style, the neighbor list
cutoff for Coulomb interactions is effectively extended by a distance
2 \* (OM distance), to account for the offset distance of the
fictitious charges on O atoms in water molecules. Thus it is
typically best in an efficiency sense to use a LJ cutoff >= Coulomb
cutoff + 2\*(OM distance), to shrink the size of the neighbor list.
This leads to slightly larger cost for the long-range calculation, so
you can test the trade-off for your model. The OM distance and the LJ
and Coulombic cutoffs are set in the :doc:`pair_style lj/cut/tip4p/long <pair_lj_cut_tip4p>` command.
Note that the when using the TIP4P pair style, the neighbor list cutoff
for Coulomb interactions is effectively extended by a distance 2 \* (OM
distance), to account for the offset distance of the fictitious charges
on O atoms in water molecules. Thus it is typically best in an
efficiency sense to use a LJ cutoff >= Coulomb cutoff + 2\*(OM
distance), to shrink the size of the neighbor list. This leads to
slightly larger cost for the long-range calculation, so you can test the
trade-off for your model. The OM distance and the LJ and Coulombic
cutoffs are set in the :doc:`pair_style lj/cut/tip4p/long
<pair_lj_cut_tip4p>` command.
Wikipedia also has a nice article on `water models <https://en.wikipedia.org/wiki/Water_model>`_.

5
doc/src/Howto_triclinic.rst
View File

@ -144,11 +144,6 @@ does not change the atom positions due to non-periodicity. In this
mode, if you tilt the system to extreme angles, the simulation will
simply become inefficient, due to the highly skewed simulation box.
The limitation on not creating a simulation box with a tilt factor
skewing the box more than half the distance of the parallel box length
can be overridden via the :doc:`box <box>` command. Setting the *tilt*
keyword to *large* allows any tilt factors to be specified.
Box flips that may occur using the :doc:`fix deform <fix_deform>` or
:doc:`fix npt <fix_nh>` commands can be turned off using the *flip no*
option with either of the commands.

25
doc/src/Library.rst
View File

@ -2,12 +2,13 @@ LAMMPS Library Interfaces
*************************
As described on the :doc:`library interface to LAMMPS <Howto_library>`
page, LAMMPS can be built as a library (static or shared), so that
it can be called by another code, used in a :doc:`coupled manner
page, LAMMPS can be built as a library (static or shared), so that it
can be called by another code, used in a :doc:`coupled manner
<Howto_couple>` with other codes, or driven through a :doc:`Python
script <Python_head>`. Even the LAMMPS standalone executable is
essentially a thin wrapper on top of the LAMMPS library, creating a
LAMMPS instance, processing input and then existing.
script <Python_head>`. The LAMMPS standalone executable itself is
essentially a thin wrapper on top of the LAMMPS library, which creates a
LAMMPS instance, passes the input for processing to that instance, and
then exits.
Most of the APIs described below are based on C language wrapper
functions in the files ``src/library.h`` and ``src/library.cpp``, but
@ -87,6 +88,18 @@ run LAMMPS in serial mode.
message retrieved <lammps_get_last_error_message>`. We thus
recommend enabling C++ exceptions when using the library interface,
.. admonition:: Using the C library interface as a plugin
:class: note
Rather than including the C library directly and link to the LAMMPS
library at compile time, you can use the ``liblammpsplugin.h`` header
file and the ``liblammpsplugin.c`` C code in the
``examples/COUPLE/plugin`` folder for an interface to LAMMPS that is
largely identical to the regular library interface, only that it will
load a LAMMPS shared library file at runtime. This can be useful for
applications where the interface to LAMMPS would be an optional
feature.
.. warning::
No checks are made on the arguments of the function calls of the C
@ -163,5 +176,3 @@ The following links provide some examples and references to the C++ API.
:maxdepth: 1
Cplusplus

2
doc/src/Library_config.rst
View File

@ -39,7 +39,7 @@ crashes within LAMMPS may be recovered from by enabling
:ref:`exceptions <exceptions>`, avoiding them proactively is a safer
approach.
.. code-block:: C
.. code-block:: c
:caption: Example for using configuration settings functions
#include "library.h"

2
doc/src/Library_create.rst
View File

@ -22,7 +22,7 @@ as the "handle" argument in subsequent function calls until that
instance is destroyed by calling :cpp:func:`lammps_close`. Here is a
simple example demonstrating its use:
.. code-block:: C
.. code-block:: c
#include "library.h"
#include <stdio.h>

2
doc/src/Library_execute.rst
View File

@ -30,7 +30,7 @@ be included in the file or strings, and expansion of variables with
``${name}`` or ``$(expression)`` syntax is performed.
Below is a short example using some of these functions.
.. code-block:: C
.. code-block:: c
/* define to make the otherwise hidden prototype for "lammps_open()" visible */
#define LAMMPS_LIB_MPI

2
doc/src/Library_properties.rst
View File

@ -32,7 +32,7 @@ indexed accordingly. Per-atom data can change sizes and ordering at
every neighbor list rebuild or atom sort event as atoms migrate between
sub-domains and processors.
.. code-block:: C
.. code-block:: c
#include "library.h"
#include <stdio.h>

6
doc/src/Library_utility.rst
View File

@ -7,6 +7,7 @@ functions. They do not directly call the LAMMPS library.
- :cpp:func:`lammps_encode_image_flags`
- :cpp:func:`lammps_decode_image_flags`
- :cpp:func:`lammps_set_fix_external_callback`
- :cpp:func:`lammps_fix_external_get_force`
- :cpp:func:`lammps_fix_external_set_energy_global`
- :cpp:func:`lammps_fix_external_set_energy_peratom`
- :cpp:func:`lammps_fix_external_set_virial_global`
@ -44,6 +45,11 @@ where such memory buffers were allocated that require the use of
-----------------------
.. doxygenfunction:: lammps_fix_external_get_force
:project: progguide
-----------------------
.. doxygenfunction:: lammps_fix_external_set_energy_global
:project: progguide

2
doc/src/Manual.rst
View File

@ -42,7 +42,7 @@ descriptions of all commands included in the LAMMPS code.
.. only:: html
Once you are familiar with LAMMPS, you may want to bookmark
:doc:`this page <Commands_all>` since it gives quick access
:doc:`this page <Commands_all>` since it gives quick access to
the documentation for all LAMMPS commands.
.. _lws: https://www.lammps.org

83
doc/src/Modify_bond.rst
View File

@ -13,24 +13,65 @@ Here is a brief description of common methods you define in your
new derived class. See bond.h, angle.h, dihedral.h, and improper.h
for details and specific additional methods.
+-----------------------+---------------------------------------------------------------------------------------+
| init | check if all coefficients are set, calls *init_style* (optional) |
+-----------------------+---------------------------------------------------------------------------------------+
| init_style | check if style specific conditions are met (optional) |
+-----------------------+---------------------------------------------------------------------------------------+
| compute | compute the molecular interactions (required) |
+-----------------------+---------------------------------------------------------------------------------------+
| settings | apply global settings for all types (optional) |
+-----------------------+---------------------------------------------------------------------------------------+
| coeff | set coefficients for one type (required) |
+-----------------------+---------------------------------------------------------------------------------------+
| equilibrium_distance | length of bond, used by SHAKE (required, bond only) |
+-----------------------+---------------------------------------------------------------------------------------+
| equilibrium_angle | opening of angle, used by SHAKE (required, angle only) |
+-----------------------+---------------------------------------------------------------------------------------+
| write & read_restart | writes/reads coeffs to restart files (required) |
+-----------------------+---------------------------------------------------------------------------------------+
| single | force (bond only) and energy of a single bond or angle (required, bond or angle only) |
+-----------------------+---------------------------------------------------------------------------------------+
| memory_usage | tally memory allocated by the style (optional) |
+-----------------------+---------------------------------------------------------------------------------------+
+-----------------------+---------------------------------------------------------------------+
| Required | "pure" methods that *must* be overridden in a derived class |
+=======================+=====================================================================+
| compute | compute the molecular interactions for all listed items |
+-----------------------+---------------------------------------------------------------------+
| coeff | set coefficients for one type |
+-----------------------+---------------------------------------------------------------------+
| equilibrium_distance | length of bond, used by SHAKE (bond styles only) |
+-----------------------+---------------------------------------------------------------------+
| equilibrium_angle | opening of angle, used by SHAKE (angle styles only) |
+-----------------------+---------------------------------------------------------------------+
| write & read_restart | writes/reads coeffs to restart files |
+-----------------------+---------------------------------------------------------------------+
| single | force/r (bond styles only) and energy of a single bond or angle |
+-----------------------+---------------------------------------------------------------------+
+--------------------------------+----------------------------------------------------------------------+
| Optional | methods that have a default or dummy implementation |
+================================+======================================================================+
| init | check if all coefficients are set, calls init_style() |
+--------------------------------+----------------------------------------------------------------------+
| init_style | check if style specific conditions are met |
+--------------------------------+----------------------------------------------------------------------+
| settings | apply global settings for all types |
+--------------------------------+----------------------------------------------------------------------+
| write & read_restart_settings | writes/reads global style settings to restart files |
+--------------------------------+----------------------------------------------------------------------+
| write_data | write corresponding Coeffs section(s) in data file |
+--------------------------------+----------------------------------------------------------------------+
| memory_usage | tally memory allocated by the style |
+--------------------------------+----------------------------------------------------------------------+
| extract | provide access to internal data (bond or angle styles only) |
+--------------------------------+----------------------------------------------------------------------+
| reinit | reset all type-based parameters, called by fix adapt (bonds only) |
+--------------------------------+----------------------------------------------------------------------+
| pack & unpack_forward_comm | copy data to and from buffer in forward communication (bonds only) |
+--------------------------------+----------------------------------------------------------------------+
| pack & unpack_reverse_comm | copy data to and from buffer in reverse communication (bonds only) |
+--------------------------------+----------------------------------------------------------------------+
Here is a list of flags or settings that should be set in the
constructor of the derived class when they differ from the default
setting.
+---------------------------------+------------------------------------------------------------------------------+---------+
| Name of flag | Description | default |
+=================================+==============================================================================+=========+
| writedata | 1 if write_data() is implemented | 1 |
+---------------------------------+------------------------------------------------------------------------------+---------+
| single_extra | number of extra single values calculated (bond styles only) | 0 |
+---------------------------------+------------------------------------------------------------------------------+---------+
| partial_flag | 1 if bond type can be set to 0 and deleted (bond styles only) | 0 |
+---------------------------------+------------------------------------------------------------------------------+---------+
| reinitflag | 1 if style has reinit() and is compatible with fix adapt | 1 |
+---------------------------------+------------------------------------------------------------------------------+---------+
| comm_forward | size of buffer (in doubles) for forward communication (bond styles only) | 0 |
+---------------------------------+------------------------------------------------------------------------------+---------+
| comm_reverse | size of buffer (in doubles) for reverse communication (bond styles only) | 0 |
+---------------------------------+------------------------------------------------------------------------------+---------+
| comm_reverse_off | size of buffer for reverse communication with newton off (bond styles only) | 0 |
+---------------------------------+------------------------------------------------------------------------------+---------+

132
doc/src/Modify_pair.rst
View File

@ -1,35 +1,121 @@
Pair styles
===========
Classes that compute pairwise interactions are derived from the Pair
class. In LAMMPS, pairwise calculation include many-body potentials
such as EAM or Tersoff where particles interact without a static bond
topology. New styles can be created to add new pair potentials to
LAMMPS.
Classes that compute pairwise non-bonded interactions are derived from
the Pair class. In LAMMPS, pairwise calculation include many-body
potentials such as EAM, Tersoff, or ReaxFF where particles interact
without an explicit bond topology but include interactions beyond
pairwise non-bonded contributions. New styles can be created to add
support for additional pair potentials to LAMMPS. When the
modifications are small, sometimes it is more effective to derive from
an existing pair style class. This latter approach is also used by
:doc:`Accelerator packages <Speed_packages>` where the accelerated style
names differ from their base classes by an appended suffix.
Pair_lj_cut.cpp is a simple example of a Pair class, though it
includes some optional methods to enable its use with rRESPA.
The file ``src/pair_lj_cut.cpp`` is an example of a Pair class with a
very simple potential function. It includes several optional methods to
enable its use with :doc:`run_style respa <run_style>` and :doc:`compute
group/group <compute_group_group>`.
Here is a brief description of the class methods in pair.h:
Here is a brief list of some the class methods in the Pair class that
*must* be or *may* be overridden in a derived class.
+---------------------------------+---------------------------------------------------------------------+
| Required | "pure" methods that *must* be overridden in a derived class |
+=================================+=====================================================================+
| compute | workhorse routine that computes pairwise interactions |
+---------------------------------+---------------------------------------------------------------------+
| settings | reads the input script line with arguments you define |
| settings | processes the arguments to the pair_style command |
+---------------------------------+---------------------------------------------------------------------+
| coeff | set coefficients for one i,j type pair |
+---------------------------------+---------------------------------------------------------------------+
| init_one | perform initialization for one i,j type pair |
+---------------------------------+---------------------------------------------------------------------+
| init_style | initialization specific to this pair style |
+---------------------------------+---------------------------------------------------------------------+
| write & read_restart | write/read i,j pair coeffs to restart files |
+---------------------------------+---------------------------------------------------------------------+
| write & read_restart_settings | write/read global settings to restart files |
+---------------------------------+---------------------------------------------------------------------+
| single | force/r and energy of a single pairwise interaction between 2 atoms |
+---------------------------------+---------------------------------------------------------------------+
| compute_inner/middle/outer | versions of compute used by rRESPA |
| coeff | set coefficients for one i,j type pair, called from pair_coeff |
+---------------------------------+---------------------------------------------------------------------+
The inner/middle/outer routines are optional.
+---------------------------------+----------------------------------------------------------------------+
| Optional | methods that have a default or dummy implementation |
+=================================+======================================================================+
| init_one | perform initialization for one i,j type pair |
+---------------------------------+----------------------------------------------------------------------+
| init_style | style initialization: request neighbor list(s), error checks |
+---------------------------------+----------------------------------------------------------------------+
| init_list | Neighbor class callback function to pass neighbor list to pair style |
+---------------------------------+----------------------------------------------------------------------+
| single | force/r and energy of a single pairwise interaction between 2 atoms |
+---------------------------------+----------------------------------------------------------------------+
| compute_inner/middle/outer | versions of compute used by rRESPA |
+---------------------------------+----------------------------------------------------------------------+
| memory_usage | return estimated amount of memory used by the pair style |
+---------------------------------+----------------------------------------------------------------------+
| modify_params | process arguments to pair_modify command |
+---------------------------------+----------------------------------------------------------------------+
| extract | provide access to internal scalar or per-type data like cutoffs |
+---------------------------------+----------------------------------------------------------------------+
| extract_peratom | provide access to internal per-atom data |
+---------------------------------+----------------------------------------------------------------------+
| setup | initialization at the beginning of a run |
+---------------------------------+----------------------------------------------------------------------+
| finish | called at the end of a run, e.g. to print |
+---------------------------------+----------------------------------------------------------------------+
| write & read_restart | write/read i,j pair coeffs to restart files |
+---------------------------------+----------------------------------------------------------------------+
| write & read_restart_settings | write/read global settings to restart files |
+---------------------------------+----------------------------------------------------------------------+
| write_data | write Pair Coeffs section to data file |
+---------------------------------+----------------------------------------------------------------------+
| write_data_all | write PairIJ Coeffs section to data file |
+---------------------------------+----------------------------------------------------------------------+
| pack & unpack_forward_comm | copy data to and from buffer if style uses forward communication |
+---------------------------------+----------------------------------------------------------------------+
| pack & unpack_reverse_comm | copy data to and from buffer if style uses reverse communication |
+---------------------------------+----------------------------------------------------------------------+
| reinit | reset all type-based parameters, called by fix adapt for example |
+---------------------------------+----------------------------------------------------------------------+
| reset_dt | called when the time step is changed by timestep or fix reset/dt |
+---------------------------------+----------------------------------------------------------------------+
Here is a list of flags or settings that should be set in the
constructor of the derived pair class when they differ from the default
setting.
+---------------------------------+-------------------------------------------------------------+---------+
| Name of flag | Description | default |
+=================================+=============================================================+=========+
| single_enable | 1 if single() method is implemented, 0 if missing | 1 |
+---------------------------------+-------------------------------------------------------------+---------+
| respa_enable | 1 if pair style has compute_inner/middle/outer() | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| restartinfo | 1 if pair style writes its settings to a restart | 1 |
+---------------------------------+-------------------------------------------------------------+---------+
| one_coeff | 1 if only a pair_coeff * * command is allowed | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| manybody_flag | 1 if pair style is a manybody potential | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| unit_convert_flag | value != 0 indicates support for unit conversion | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| no_virial_fdotr_compute | 1 if pair style does not call virial_fdotr_compute() | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| writedata | 1 if write_data() and write_data_all() are implemented | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| comm_forward | size of buffer (in doubles) for forward communication | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| comm_reverse | size of buffer (in doubles) for reverse communication | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| ghostneigh | 1 if cutghost is set and style uses neighbors of ghosts | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| finitecutflag | 1 if cutoff depends on diameter of atoms | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| reinitflag | 1 if style has reinit() and is compatible with fix adapt | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| ewaldflag | 1 if compatible with kspace_style ewald | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| pppmflag | 1 if compatible with kspace_style pppm | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| msmflag | 1 if compatible with kspace_style msm | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| dispersionflag | 1 if compatible with ewald/disp or pppm/disp | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| tip4pflag | 1 if compatible with kspace_style pppm/tip4p | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| dipoleflag | 1 if compatible with dipole kspace_style | 0 |
+---------------------------------+-------------------------------------------------------------+---------+
| spinflag | 1 if compatible with spin kspace_style | 0 |
+---------------------------------+-------------------------------------------------------------+---------+

6
doc/src/Modify_style.rst
View File

@ -359,6 +359,12 @@ you are uncertain, please ask.
- I/O is done via the C-style stdio library and **not** iostreams.
- Do not use so-called "alternative tokens" like ``and``, ``or``,
``not`` and similar, but rather use the corresponding operators
``&&``, ``||``, and ``!``. The alternative tokens are not available
by default on all compilers, and also we want to maintain a consistent
programming style.
- Output to the screen and the logfile should be using the corresponding
FILE pointers and only be done on MPI rank 0. Use the :cpp:func:`utils::logmesg`
convenience function where possible.

47
doc/src/Packages_details.rst
View File

@ -80,6 +80,7 @@ page gives those details.
* :ref:`ML-HDNNP <PKG-ML-HDNNP>`
* :ref:`ML-IAP <PKG-ML-IAP>`
* :ref:`ML-PACE <PKG-ML-PACE>`
* :ref:`ML-POD <PKG-ML-POD>`
* :ref:`ML-QUIP <PKG-ML-QUIP>`
* :ref:`ML-RANN <PKG-ML-RANN>`
* :ref:`ML-SNAP <PKG-ML-SNAP>`
@ -200,6 +201,7 @@ particle models including ellipsoids, 2d lines, and 3d triangles.
* :doc:`Howto spherical <Howto_spherical>`
* :doc:`pair_style gayberne <pair_gayberne>`
* :doc:`pair_style resquared <pair_resquared>`
* :doc:`pair_style ylz <pair_ylz>`
* `doc/PDF/pair_gayberne_extra.pdf <PDF/pair_gayberne_extra.pdf>`_
* `doc/PDF/pair_resquared_extra.pdf <PDF/pair_resquared_extra.pdf>`_
* examples/ASPHERE
@ -864,7 +866,7 @@ ELECTRODE package
The ELECTRODE package allows the user to enforce a constant potential method for
groups of atoms that interact with the remaining atoms as electrolyte.
**Authors:** The ELECTRODE library is written and maintained by Ludwig
**Authors:** The ELECTRODE package is written and maintained by Ludwig
Ahrens-Iwers (TUHH, Hamburg, Germany), Shern Tee (UQ, Brisbane, Australia) and
Robert Meissner (TUHH, Hamburg, Germany).
@ -877,7 +879,7 @@ This package has :ref:`specific installation instructions <electrode>` on the
**Supporting info:**
* :doc:`fix electrode/conp <fix_electrode_conp>`
* :doc:`fix electrode/conp <fix_electrode>`
----------
@ -1484,8 +1486,9 @@ MC package
Several fixes and a pair style that have Monte Carlo (MC) or MC-like
attributes. These include fixes for creating, breaking, and swapping
bonds, for performing atomic swaps, and performing grand-canonical MC
(GCMC) or similar processes in conjunction with dynamics.
bonds, for performing atomic swaps, and performing grand canonical
MC (GCMC), semi-grand canonical MC (SGCMC), or similar processes in
conjunction with molecular dynamics (MD).
**Supporting info:**
@ -1497,6 +1500,7 @@ bonds, for performing atomic swaps, and performing grand-canonical MC
* :doc:`fix bond/swap <fix_bond_swap>`
* :doc:`fix charge/regulation <fix_charge_regulation>`
* :doc:`fix gcmc <fix_gcmc>`
* :doc:`fix sgcmc <fix_sgcmc>`
* :doc:`fix tfmc <fix_tfmc>`
* :doc:`fix widom <fix_widom>`
* :doc:`pair_style dsmc <pair_dsmc>`
@ -1736,8 +1740,6 @@ must be installed.
.. versionadded:: 30Jun2020
.. versionadded:: 30Jun2020
**Supporting info:**
* src/ML-IAP: filenames -> commands
@ -1797,6 +1799,39 @@ This package has :ref:`specific installation instructions <ml-pace>` on the
----------
.. _PKG-ML-POD:
ML-POD package
-------------------
**Contents:**
A pair style and fitpod style for Proper Orthogonal Descriptors
(POD). POD is a methodology for deriving descriptors based on the proper
orthogonal decomposition. The ML-POD package provides an efficient
implementation for running simulations with POD potentials, along with
fitting the potentials natively in LAMMPS.
**Authors:**
Ngoc Cuong Nguyen (MIT), Andrew Rohskopf (Sandia)
.. versionadded:: 22Dec2022
**Install:**
This package has :ref:`specific installation instructions <ml-pod>` on the
:doc:`Build extras <Build_extras>` page.
**Supporting info:**
* src/ML-POD: filenames -> commands
* :doc:`pair_style pod <pair_pod>`
* :doc:`command_style fitpod <fitpod_command>`
* examples/PACKAGES/pod
----------
.. _PKG-ML-QUIP:
ML-QUIP package

7
doc/src/Packages_list.rst
View File

@ -155,7 +155,7 @@ whether an extra library is needed to build and use the package:
- no
* - :ref:`ELECTRODE <PKG-ELECTRODE>`
- electrode charges to match potential
- :doc:`fix electrode/conp <fix_electrode_conp>`
- :doc:`fix electrode/conp <fix_electrode>`
- PACKAGES/electrode
- no
* - :ref:`EXTRA-COMPUTE <PKG-EXTRA-COMPUTE>`
@ -298,6 +298,11 @@ whether an extra library is needed to build and use the package:
- :doc:`pair pace <pair_pace>`
- PACKAGES/pace
- ext
* - :ref:`ML-POD <PKG-ML-POD>`
- Proper orthogonal decomposition potentials
- :doc:`pair pod <pair_pod>`
- pod
- ext
* - :ref:`ML-QUIP <PKG-ML-QUIP>`
- QUIP/libatoms interface
- :doc:`pair_style quip <pair_quip>`

4
doc/src/Python_atoms.rst
View File

@ -58,7 +58,7 @@ against invalid accesses.
Each element of this list is a :py:class:`Atom <lammps.Atom>` or :py:class:`Atom2D <lammps.Atom2D>` object. The attributes of
these objects provide access to their data (id, type, position, velocity, force, etc.):
.. code-block:: Python
.. code-block:: python
# access first atom
L.atoms[0].id
@ -71,7 +71,7 @@ against invalid accesses.
Some attributes can be changed:
.. code-block:: Python
.. code-block:: python
# set position in 2D simulation
L.atoms[0].position = (1.0, 0.0)

2
doc/src/Python_config.rst
View File

@ -4,7 +4,7 @@ Configuration information
The following methods can be used to query the LAMMPS library
about compile time settings and included packages and styles.
.. code-block:: Python
.. code-block:: python
:caption: Example for using configuration settings functions
from lammps import lammps

6
doc/src/Python_create.rst
View File

@ -74,7 +74,7 @@ Here are simple examples using all three Python interfaces:
:py:class:`PyLammps <lammps.PyLammps>` objects can also be created on top of an existing
:py:class:`lammps <lammps.lammps>` object:
.. code-block:: Python
.. code-block:: python
from lammps import lammps, PyLammps
...
@ -113,7 +113,7 @@ Here are simple examples using all three Python interfaces:
You can also initialize IPyLammps on top of an existing :py:class:`lammps` or :py:class:`PyLammps` object:
.. code-block:: Python
.. code-block:: python
from lammps import lammps, IPyLammps
...
@ -142,7 +142,7 @@ the MPI and/or Kokkos environment if enabled and active.
Note that you can create multiple LAMMPS objects in your Python
script, and coordinate and run multiple simulations, e.g.
.. code-block:: Python
.. code-block:: python
from lammps import lammps
lmp1 = lammps()

2
doc/src/Python_error.rst
View File

@ -7,7 +7,7 @@ current Python process with an error message. C++ exceptions allow capturing
them on the C++ side and rethrowing them on the Python side. This way
LAMMPS errors can be handled through the Python exception handling mechanism.
.. code-block:: Python
.. code-block:: python
from lammps import lammps, MPIAbortException

8
doc/src/Python_execute.rst
View File

@ -60,7 +60,7 @@ it is possible to "compute" what the next LAMMPS command should be.
can be executed using with the lammps API with the following Python code if ``lmp`` is an
instance of :py:class:`lammps <lammps.lammps>`:
.. code-block:: Python
.. code-block:: python
from lammps import lammps
@ -73,7 +73,7 @@ it is possible to "compute" what the next LAMMPS command should be.
The arguments of the command can be passed as one string, or
individually.
.. code-block:: Python
.. code-block:: python
from lammps import PyLammps
@ -93,14 +93,14 @@ it is possible to "compute" what the next LAMMPS command should be.
parameterization. In the lammps API parameterization needed to be done
manually by creating formatted command strings.
.. code-block:: Python
.. code-block:: python
lmp.command("region box block %f %f %f %f %f %f" % (xlo, xhi, ylo, yhi, zlo, zhi))
In contrast, methods of PyLammps accept parameters directly and will convert
them automatically to a final command string.
.. code-block:: Python
.. code-block:: python
L.region("box block", xlo, xhi, ylo, yhi, zlo, zhi)

2
doc/src/Python_launch.rst
View File

@ -56,7 +56,7 @@ and you should see the same output as if you had typed
Note that without the mpi4py specific lines from ``test.py``
.. code-block:: Python
.. code-block:: python
from lammps import lammps
lmp = lammps()

6
doc/src/Python_objects.rst
View File

@ -76,7 +76,7 @@ computes, fixes, or variables in LAMMPS using the :py:mod:`lammps` module.
To define a variable you can use the :doc:`variable <variable>` command:
.. code-block:: Python
.. code-block:: python
L.variable("a index 2")
@ -85,14 +85,14 @@ computes, fixes, or variables in LAMMPS using the :py:mod:`lammps` module.
you can access an individual variable by retrieving a variable object from the
``L.variables`` dictionary by name
.. code-block:: Python
.. code-block:: python
a = L.variables['a']
The variable value can then be easily read and written by accessing the value
property of this object.
.. code-block:: Python
.. code-block:: python
print(a.value)
a.value = 4

2
doc/src/Python_properties.rst
View File

@ -105,7 +105,7 @@ against invalid accesses.
variables, compute or fix data (see :doc:`Howto_output`):
.. code-block:: Python
.. code-block:: python
result = L.eval("ke") # kinetic energy
result = L.eval("pe") # potential energy

4
doc/src/Python_scatter.rst
View File

@ -1,7 +1,7 @@
Scatter/gather operations
=========================
.. code-block:: Python
.. code-block:: python
data = lmp.gather_atoms(name,type,count) # return per-atom property of all atoms gathered into data, ordered by atom ID
# name = "x", "charge", "type", etc
@ -42,7 +42,7 @@ For the scatter methods, the array of coordinates passed to must be a
ctypes vector of ints or doubles, allocated and initialized something
like this:
.. code-block:: Python
.. code-block:: python
from ctypes import c_double
natoms = lmp.get_natoms()

38
doc/src/Run_options.rst
View File

@ -262,6 +262,8 @@ Disable generating a citation reminder (see above) at all.
**-nonbuf**
.. versionadded:: 15Sep2022
Turn off buffering for screen and logfile output. For performance
reasons, output to the screen and logfile is usually buffered, i.e.
output is only written to a file if its buffer - typically 4096 bytes -
@ -442,7 +444,7 @@ the LAMMPS simulation domain.
.. _restart2data:
**-restart2data restartfile [remap] datafile keyword value ...**
**-restart2data restartfile datafile keyword value ...**
Convert the restart file into a data file and immediately exit. This
is the same operation as if the following 2-line input script were
@ -450,7 +452,7 @@ run:
.. code-block:: LAMMPS
read_restart restartfile [remap]
read_restart restartfile
write_data datafile keyword value ...
The specified restartfile and/or datafile name may contain the wild-card
@ -462,28 +464,21 @@ Note that a filename such as file.\* may need to be enclosed in quotes or
the "\*" character prefixed with a backslash ("\") to avoid shell
expansion of the "\*" character.
Following restartfile argument, the optional word "remap" may be used.
This has the same effect like adding it to a
:doc:`read_restart <read_restart>` command, and operates as explained on
its doc page. This is useful if reading the restart file triggers an
error that atoms have been lost. In that case, use of the remap flag
should allow the data file to still be produced.
The syntax following restartfile (or remap), namely
The syntax following restartfile, namely
.. parsed-literal::
datafile keyword value ...
is identical to the arguments of the :doc:`write_data <write_data>`
command. See its page for details. This includes its
command. See its documentation page for details. This includes its
optional keyword/value settings.
----------
.. _restart2dump:
**-restart2dump restartfile [remap] group-ID dumpstyle dumpfile arg1 arg2 ...**
**-restart2dump restartfile group-ID dumpstyle dumpfile arg1 arg2 ...**
Convert the restart file into a dump file and immediately exit. This
is the same operation as if the following 2-line input script were
@ -491,7 +486,7 @@ run:
.. code-block:: LAMMPS
read_restart restartfile [remap]
read_restart restartfile
write_dump group-ID dumpstyle dumpfile arg1 arg2 ...
Note that the specified restartfile and dumpfile names may contain
@ -503,24 +498,17 @@ such as file.\* may need to be enclosed in quotes or the "\*" character
prefixed with a backslash ("\") to avoid shell expansion of the "\*"
character.
Note that following the restartfile argument, the optional word "remap"
can be used. This has the effect as adding it to the
:doc:`read_restart <read_restart>` command, as explained on its doc page.
This is useful if reading the restart file triggers an error that atoms
have been lost. In that case, use of the remap flag should allow the
dump file to still be produced.
The syntax following restartfile (or remap), namely
The syntax following restartfile, namely
.. code-block:: LAMMPS
group-ID dumpstyle dumpfile arg1 arg2 ...
is identical to the arguments of the :doc:`write_dump <write_dump>`
command. See its page for details. This includes what per-atom
fields are written to the dump file and optional dump_modify settings,
including ones that affect how parallel dump files are written, e.g.
the *nfile* and *fileper* keywords. See the
command. See its documentation page for details. This includes what
per-atom fields are written to the dump file and optional dump_modify
settings, including ones that affect how parallel dump files are written,
e.g. the *nfile* and *fileper* keywords. See the
:doc:`dump_modify <dump_modify>` page for details.
----------

59
doc/src/Run_output.rst
View File

@ -16,46 +16,47 @@ simulation. An example set of statistics is shown here:
.. parsed-literal::
Loop time of 2.81192 on 4 procs for 300 steps with 2004 atoms
Loop time of 0.942801 on 4 procs for 300 steps with 2004 atoms
Performance: 18.436 ns/day 1.302 hours/ns 106.689 timesteps/s
97.0% CPU use with 4 MPI tasks x no OpenMP threads
Performance: 54.985 ns/day, 0.436 hours/ns, 318.201 timesteps/s, 637.674 katom-step/s
195.2% CPU use with 2 MPI tasks x 2 OpenMP threads
MPI task timings breakdown:
MPI task timing breakdown:
Section \| min time \| avg time \| max time \|%varavg\| %total
---------------------------------------------------------------
Pair \| 1.9808 \| 2.0134 \| 2.0318 \| 1.4 \| 71.60
Bond \| 0.0021894 \| 0.0060319 \| 0.010058 \| 4.7 \| 0.21
Kspace \| 0.3207 \| 0.3366 \| 0.36616 \| 3.1 \| 11.97
Neigh \| 0.28411 \| 0.28464 \| 0.28516 \| 0.1 \| 10.12
Comm \| 0.075732 \| 0.077018 \| 0.07883 \| 0.4 \| 2.74
Output \| 0.00030518 \| 0.00042665 \| 0.00078821 \| 1.0 \| 0.02
Modify \| 0.086606 \| 0.086631 \| 0.086668 \| 0.0 \| 3.08
Other \| \| 0.007178 \| \| \| 0.26
Pair \| 0.61419 \| 0.62872 \| 0.64325 \| 1.8 \| 66.69
Bond \| 0.0028608 \| 0.0028899 \| 0.002919 \| 0.1 \| 0.31
Kspace \| 0.12652 \| 0.14048 \| 0.15444 \| 3.7 \| 14.90
Neigh \| 0.10242 \| 0.10242 \| 0.10242 \| 0.0 \| 10.86
Comm \| 0.026753 \| 0.027593 \| 0.028434 \| 0.5 \| 2.93
Output \| 0.00018341 \| 0.00030942 \| 0.00043542 \| 0.0 \| 0.03
Modify \| 0.039117 \| 0.039348 \| 0.039579 \| 0.1 \| 4.17
Other \| \| 0.001041 \| \| \| 0.11
Nlocal: 501 ave 508 max 490 min
Histogram: 1 0 0 0 0 0 1 1 0 1
Nghost: 6586.25 ave 6628 max 6548 min
Histogram: 1 0 1 0 0 0 1 0 0 1
Neighs: 177007 ave 180562 max 170212 min
Histogram: 1 0 0 0 0 0 0 1 1 1
Nlocal: 1002 ave 1006 max 998 min
Histogram: 1 0 0 0 0 0 0 0 0 1
Nghost: 8670.5 ave 8691 max 8650 min
Histogram: 1 0 0 0 0 0 0 0 0 1
Neighs: 354010 ave 357257 max 350763 min
Histogram: 1 0 0 0 0 0 0 0 0 1
Total # of neighbors = 708028
Ave neighs/atom = 353.307
Ave special neighs/atom = 2.34032
Total # of neighbors = 708020
Ave neighs/atom = 353.30339
Ave special neighs/atom = 2.3403194
Neighbor list builds = 26
Dangerous builds = 0
----------
The first section provides a global loop timing summary. The *loop
time* is the total wall-clock time for the simulation to run. The
*Performance* line is provided for convenience to help predict how
long it will take to run a desired physical simulation. The *CPU use*
line provides the CPU utilization per MPI task; it should be close to
100% times the number of OpenMP threads (or 1 of not using OpenMP).
Lower numbers correspond to delays due to file I/O or insufficient
thread utilization.
The first section provides a global loop timing summary. The *loop time*
is the total wall-clock time for the simulation to run. The
*Performance* line is provided for convenience to help predict how long
it will take to run a desired physical simulation and to have numbers
useful for performance comparison between different simulation settings
or system sizes. The *CPU use* line provides the CPU utilization per
MPI task; it should be close to 100% times the number of OpenMP threads
(or 1 of not using OpenMP). Lower numbers correspond to delays due to
file I/O or insufficient thread utilization.
----------

40
doc/src/Speed_kokkos.rst
View File

@ -212,14 +212,15 @@ threads/task as Nt. The product of these two values should be N, i.e.
.. note::
The default for the :doc:`package kokkos <package>` command when
running on KNL is to use "half" neighbor lists and set the Newton flag
to "on" for both pairwise and bonded interactions. This will typically
be best for many-body potentials. For simpler pairwise potentials, it
may be faster to use a "full" neighbor list with Newton flag to "off".
Use the "-pk kokkos" :doc:`command-line switch <Run_options>` to change
the default :doc:`package kokkos <package>` options. See its page for
details and default settings. Experimenting with its options can provide
a speed-up for specific calculations. For example:
running on KNL is to use "half" neighbor lists and set the Newton
flag to "on" for both pairwise and bonded interactions. This will
typically be best for many-body potentials. For simpler pairwise
potentials, it may be faster to use a "full" neighbor list with
Newton flag to "off". Use the "-pk kokkos" :doc:`command-line switch
<Run_options>` to change the default :doc:`package kokkos <package>`
options. See its documentation page for details and default
settings. Experimenting with its options can provide a speed-up for
specific calculations. For example:
.. code-block:: bash
@ -271,17 +272,18 @@ one or more nodes, each with two GPUs:
.. note::
The default for the :doc:`package kokkos <package>` command when
running on GPUs is to use "full" neighbor lists and set the Newton flag
to "off" for both pairwise and bonded interactions, along with threaded
communication. When running on Maxwell or Kepler GPUs, this will
typically be best. For Pascal GPUs and beyond, using "half" neighbor lists and
setting the Newton flag to "on" may be faster. For many pair styles,
setting the neighbor binsize equal to twice the CPU default value will
give speedup, which is the default when running on GPUs. Use the "-pk
kokkos" :doc:`command-line switch <Run_options>` to change the default
:doc:`package kokkos <package>` options. See its page for details and
default settings. Experimenting with its options can provide a speed-up
for specific calculations. For example:
running on GPUs is to use "full" neighbor lists and set the Newton
flag to "off" for both pairwise and bonded interactions, along with
threaded communication. When running on Maxwell or Kepler GPUs, this
will typically be best. For Pascal GPUs and beyond, using "half"
neighbor lists and setting the Newton flag to "on" may be faster. For
many pair styles, setting the neighbor binsize equal to twice the CPU
default value will give speedup, which is the default when running on
GPUs. Use the "-pk kokkos" :doc:`command-line switch <Run_options>`
to change the default :doc:`package kokkos <package>` options. See
its documentation page for details and default
settings. Experimenting with its options can provide a speed-up for
specific calculations. For example:
.. code-block:: bash

20
doc/src/Tools.rst
View File

@ -57,7 +57,7 @@ Pre-processing tools
* :ref:`msi2lmp <msi>`
* :ref:`polybond <polybond>`
* :ref:`stl_bin2txt <stlconvert>`
* :ref:`tabulate <tabulate>`
Post-processing tools
=====================
@ -1159,13 +1159,27 @@ For illustration purposes below is a part of the Tcl example script.
----------
.. _tabulate:
tabulate tool
--------------
.. versionadded:: 22Dec2022
The ``tabulate`` folder contains Python scripts scripts to generate tabulated
potential files for LAMMPS. The bulk of the code is in the ``tabulate`` module
in the ``tabulate.py`` file. Some example files demonstrating its use are
included. See the README file for more information.
----------
.. _vim:
vim tool
------------------
The files in the tools/vim directory are add-ons to the VIM editor
that allow easier editing of LAMMPS input scripts. See the README.txt
The files in the ``tools/vim`` directory are add-ons to the VIM editor
that allow easier editing of LAMMPS input scripts. See the ``README.txt``
file for details.
These files were provided by Gerolf Ziegenhain (gerolf at

18
doc/src/angle_gaussian.rst
View File

@ -25,23 +25,25 @@ The *gaussian* angle style uses the potential:
.. math::
E = -k_B T ln\left(\sum_{i=1}^{n} \frac{A_i}{w_i \sqrt{\pi/2}} exp\left( \frac{-(\theta-\theta_{i})^2}{w_i^2})\right) \right)
E = -k_B T ln\left(\sum_{i=1}^{n} \frac{A_i}{w_i \sqrt{\pi/2}} exp\left( \frac{-2(\theta-\theta_{i})^2}{w_i^2}\right) \right)
This analytical form is a suitable potential for obtaining mesoscale
effective force fields which can reproduce target atomistic
distributions :ref:`(Milano) <Milano1>`.
This analytical form is a suitable potential for obtaining
mesoscale effective force fields which can reproduce target atomistic distributions :ref:`(Milano) <Milano1>`
The following coefficients must be defined for each angle type via the
:doc:`angle_coeff <angle_coeff>` command as in the example above, or in
the data file or restart files read by the :doc:`read_data <read_data>`
or :doc:`read_restart <read_restart>` commands:
* T temperature at which the potential was derived
* :math:`T` temperature at which the potential was derived
* :math:`n` (integer >=1)
* :math:`A_1` (-)
* :math:`w_1` (-)
* :math:`A_1` (> 0, radians)
* :math:`w_1` (> 0, radians)
* :math:`\theta_1` (degrees)
* ...
* :math:`A_n` (-)
* :math:`w_n` (-)
* :math:`A_n` (> 0, radians)
* :math:`w_n` (> 0, radians)
* :math:`\theta_n` (degrees)

4
doc/src/angle_table.rst
View File

@ -59,6 +59,10 @@ format of this file is described below.
----------
Suitable tables for use with this angle style can be created using the
Python code in the ``tools/tabulate`` folder of the LAMMPS source code
distribution.
The format of a tabulated file is as follows (without the
parenthesized comments):

10
doc/src/bond_bpm_rotational.rst
View File

@ -45,6 +45,8 @@ Examples
Description
"""""""""""
.. versionadded:: 4May2022
The *bpm/rotational* bond style computes forces and torques based on
deviations from the initial reference state of the two atoms. The
reference state is stored by each bond when it is first computed in
@ -67,7 +69,7 @@ which is proportional to the tangential shear displacement with a
stiffness of :math:`k_s`. This tangential force also induces a torque.
In addition, bending and twisting torques are also applied to
particles which are proportional to angular bending and twisting
displacements with stiffnesses of :math`k_b` and :math:`k_t',
displacements with stiffnesses of :math:`k_b` and :math:`k_t`,
respectively. Details on the calculations of shear displacements and
angular displacements can be found in :ref:`(Wang) <Wang2009>` and
:ref:`(Wang and Mora) <Wang2009b>`.
@ -211,9 +213,9 @@ command, as *b1*, *b2*, ..., *b7*\ .
Restrictions
""""""""""""
This bond style can only be used if LAMMPS was built with the BPM
package. See the :doc:`Build package <Build_package>` doc page for
more info.
This bond style is part of the BPM package. It is only enabled if
LAMMPS was built with that package. See the :doc:`Build package
<Build_package>` page for more info.
By default if pair interactions are to be disabled, this bond style
requires setting

8
doc/src/bond_bpm_spring.rst
View File

@ -45,6 +45,8 @@ Examples
Description
"""""""""""
.. versionadded:: 4May2022
The *bpm/spring* bond style computes forces and torques based on
deviations from the initial reference state of the two atoms. The
reference state is stored by each bond when it is first computed in
@ -167,9 +169,9 @@ extra quantity can be accessed by the
Restrictions
""""""""""""
This bond style can only be used if LAMMPS was built with the BPM
package. See the :doc:`Build package <Build_package>` doc page for
more info.
This bond style is part of the BPM package. It is only enabled if
LAMMPS was built with that package. See the :doc:`Build package
<Build_package>` page for more info.
By default if pair interactions are to be disabled, this bond style
requires setting

25
doc/src/bond_gaussian.rst
View File

@ -25,33 +25,34 @@ The *gaussian* bond style uses the potential:
.. math::
E = -k_B T ln\left(\sum_{i=1}^{n} \frac{A_i}{w_i \sqrt{\pi/2}} exp\left( \frac{-(r-r_{i})^2}{w_i^2})\right) \right)
E = -k_B T ln\left(\sum_{i=1}^{n} \frac{A_i}{w_i \sqrt{\pi/2}} exp\left( \frac{-2(r-r_{i})^2}{w_i^2}\right)\right)
This analytical form is a suitable potential for obtaining
mesoscale effective force fields which can reproduce target atomistic distributions :ref:`(Milano) <Milano0>`
This analytical form is a suitable potential for obtaining mesoscale
effective force fields which can reproduce target atomistic
distributions :ref:`(Milano) <Milano0>`
The following coefficients must be defined for each bond type via the
:doc:`bond_coeff <bond_coeff>` command as in the example above, or in
the data file or restart files read by the :doc:`read_data <read_data>`
or :doc:`read_restart <read_restart>` commands:
* T temperature at which the potential was derived
* :math:`T` temperature at which the potential was derived
* :math:`n` (integer >=1)
* :math:`A_1` (-)
* :math:`w_1` (-)
* :math:`r_1` (length)
* :math:`A_1` (> 0, distance)
* :math:`w_1` (> 0, distance)
* :math:`r_1` (>= 0, distance)
* ...
* :math:`A_n` (-)
* :math:`w_n` (-)
* :math:`r_n` (length)
* :math:`A_n` (> 0, distance)
* :math:`w_n` (> 0, distance)
* :math:`r_n` (>= 0, distance)
Restrictions
""""""""""""
This bond style can only be used if LAMMPS was built with the
EXTRA-MOLECULE package. See the :doc:`Build package <Build_package>` doc
page for more info.
EXTRA-MOLECULE package. See the :doc:`Build package <Build_package>`
doc page for more info.
Related commands
""""""""""""""""

10
doc/src/bond_table.rst
View File

@ -59,6 +59,13 @@ this file is described below.
----------
Suitable tables for use with this bond style can be created by LAMMPS
itself from existing bond styles using the :doc:`bond_write
<bond_write>` command. This can be useful to have a template file for
testing the bond style settings and to build a compatible custom file.
Another option to generate tables is the Python code in the
``tools/tabulate`` folder of the LAMMPS source code distribution.
The format of a tabulated file is as follows (without the
parenthesized comments):
@ -149,7 +156,8 @@ info.
Related commands
""""""""""""""""
:doc:`bond_coeff <bond_coeff>`, :doc:`delete_bonds <delete_bonds>`
:doc:`bond_coeff <bond_coeff>`, :doc:`delete_bonds <delete_bonds>`,
:doc:`bond_write <bond_write>`
Default
"""""""

70
doc/src/box.rst
View File

@ -1,70 +0,0 @@
.. index:: box
box command
===========
Syntax
""""""
.. code-block:: LAMMPS
box keyword value ...
* one or more keyword/value pairs may be appended
* keyword = *tilt*
.. parsed-literal::
*tilt* value = *small* or *large*
Examples
""""""""
.. code-block:: LAMMPS
box tilt large
box tilt small
Description
"""""""""""
Set attributes of the simulation box.
For triclinic (non-orthogonal) simulation boxes, the *tilt* keyword
allows simulation domains to be created with arbitrary tilt factors,
e.g. via the :doc:`create_box <create_box>` or
:doc:`read_data <read_data>` commands. Tilt factors determine how
skewed the triclinic box is; see the :doc:`Howto triclinic <Howto_triclinic>` page for a discussion of triclinic
boxes in LAMMPS.
LAMMPS normally requires that no tilt factor can skew the box more
than half the distance of the parallel box length, which is the first
dimension in the tilt factor (x for xz). If *tilt* is set to
*small*, which is the default, then an error will be
generated if a box is created which exceeds this limit. If *tilt*
is set to *large*, then no limit is enforced. You can create
a box with any tilt factors you wish.
Note that if a simulation box has a large tilt factor, LAMMPS will run
less efficiently, due to the large volume of communication needed to
acquire ghost atoms around a processor's irregular-shaped sub-domain.
For extreme values of tilt, LAMMPS may also lose atoms and generate an
error.
Restrictions
""""""""""""
This command cannot be used after the simulation box is defined by a
:doc:`read_data <read_data>` or :doc:`create_box <create_box>` command or
:doc:`read_restart <read_restart>` command.
Related commands
""""""""""""""""
none
Default
"""""""
The default value is tilt = small.

15
doc/src/clear.rst
View File

@ -23,15 +23,16 @@ Description
"""""""""""
This command deletes all atoms, restores all settings to their default
values, and frees all memory allocated by LAMMPS. Once a clear
command has been executed, it is almost as if LAMMPS were starting
over, with only the exceptions noted below. This command enables
multiple jobs to be run sequentially from one input script.
values, and frees all memory allocated by LAMMPS. Once a clear command
has been executed, it is almost as if LAMMPS were starting over, with
only the exceptions noted below. This command enables multiple jobs to
be run sequentially from one input script.
These settings are not affected by a clear command: the working
directory (:doc:`shell <shell>` command), log file status
(:doc:`log <log>` command), echo status (:doc:`echo <echo>` command), and
input script variables (:doc:`variable <variable>` command).
directory (:doc:`shell <shell>` command), log file status (:doc:`log
<log>` command), echo status (:doc:`echo <echo>` command), and input
script variables except for *atomfile* style variables (:doc:`variable
<variable>` command).
Restrictions
""""""""""""

5
doc/src/commands_list.rst
View File

@ -13,7 +13,6 @@ Commands
bond_style
bond_write
boundary
box
change_box
clear
comm_modify
@ -43,6 +42,7 @@ Commands
echo
fix
fix_modify
fitpod_command
group
group2ndx
hyper
@ -90,8 +90,7 @@ Commands
region
replicate
rerun
reset_atom_ids
reset_mol_ids
reset_atoms
reset_timestep
restart
run

54
doc/src/compute.rst
View File

@ -43,29 +43,38 @@ underscores.
----------
Computes calculate one of three styles of quantities: global,
per-atom, or local. A global quantity is one or more system-wide
values (e.g., the temperature of the system). A per-atom quantity is
one or more values per atom (e.g., the kinetic energy of each atom).
Per-atom values are set to 0.0 for atoms not in the specified compute
group. Local quantities are calculated by each processor based on the
atoms it owns, but there may be zero or more per atom (e.g., a list of
bond distances). Computes that produce per-atom quantities have the
word "atom" in their style (e.g., *ke/atom*\ ). Computes that produce
local quantities have the word "local" in their style
(e.g., *bond/local*\ ). Styles with neither "atom" or "local" in their
style produce global quantities.
Computes calculate one or more of four styles of quantities: global,
per-atom, local, or per-atom. A global quantity is one or more
system-wide values, e.g. the temperature of the system. A per-atom
quantity is one or more values per atom, e.g. the kinetic energy of
each atom. Per-atom values are set to 0.0 for atoms not in the
specified compute group. Local quantities are calculated by each
processor based on the atoms it owns, but there may be zero or more
per atom, e.g. a list of bond distances. Per-grid quantities are
calculated on a regular 2d or 3d grid which overlays a 2d or 3d
simulation domain. The grid points and the data they store are
distributed across processors; each processor owns the grid points
which fall within its sub-domain.
Note that a single compute can produce either global or per-atom or
local quantities, but not both global and per-atom. It can produce
local quantities in tandem with global or per-atom quantities. The
compute page will explain.
Computes that produce per-atom quantities have the word "atom" at the
end of their style, e.g. *ke/atom*\ . Computes that produce local
quantities have the word "local" at the end of their style,
e.g. *bond/local*\ . Computes that produce per-grid quantities have
the word "grid" at the end of their style, e.g. *property/grid*\ .
Styles with neither "atom" or "local" or "grid" at the end of their
style name produce global quantities.
Global, per-atom, and local quantities each come in three kinds: a
single scalar value, a vector of values, or a 2d array of values. The
doc page for each compute describes the style and kind of values it
produces (e.g., a per-atom vector). Some computes produce more than one
kind of a single style (e.g., a global scalar and a global vector).
Note that a single compute typically produces either global or
per-atom or local or per-grid values. It does not compute both global
and per-atom values. It can produce local values or per-grid values
in tandem with global or per-atom quantities. The compute doc page
will explain the details.
Global, per-atom, local, and per-grid quantities come in three kinds:
a single scalar value, a vector of values, or a 2d array of values.
The doc page for each compute describes the style and kind of values
it produces, e.g. a per-atom vector. Some computes produce more than
one kind of a single style, e.g. a global scalar and a global vector.
When a compute quantity is accessed, as in many of the output commands
discussed below, it can be referenced via the following bracket
@ -252,7 +261,8 @@ The individual style names on the :doc:`Commands compute <Commands_compute>` pag
* :doc:`pressure/uef <compute_pressure_uef>` - pressure tensor in the reference frame of an applied flow field
* :doc:`property/atom <compute_property_atom>` - convert atom attributes to per-atom vectors/arrays
* :doc:`property/chunk <compute_property_chunk>` - extract various per-chunk attributes
* :doc:`property/local <compute_property_local>` - convert local attributes to localvectors/arrays
* :doc:`property/grid <compute_property_grid>` - convert per-grid attributes to per-grid vectors/arrays
* :doc:`property/local <compute_property_local>` - convert local attributes to local vectors/arrays
* :doc:`ptm/atom <compute_ptm_atom>` - determines the local lattice structure based on the Polyhedral Template Matching method
* :doc:`rdf <compute_rdf>` - radial distribution function :math:`g(r)` histogram of group of atoms
* :doc:`reduce <compute_reduce>` - combine per-atom quantities into a single global value

38
doc/src/compute_modify.rst
View File

@ -37,27 +37,29 @@ Description
Modify one or more parameters of a previously defined compute. Not
all compute styles support all parameters.
The *extra/dof* or *extra* keyword refers to how many degrees of freedom are
subtracted (typically from :math:`3N`) as a normalizing
The *extra/dof* or *extra* keyword refers to how many degrees of
freedom are subtracted (typically from :math:`3N`) as a normalizing
factor in a temperature computation. Only computes that compute a
temperature use this option. The default is 2 or 3 for
:doc:`2d or 3d systems <dimension>`, which is a correction factor for an
ensemble of velocities with zero total linear momentum. For compute
temp/partial, if one or more velocity components are excluded, the
value used for *extra* is scaled accordingly. You can use a negative
number for the *extra* parameter if you need to add
degrees-of-freedom. See the :doc:`compute temp/asphere <compute_temp_asphere>` command for an example.
temperature use this option. The default is 2 or 3 for :doc:`2d or 3d
systems <dimension>` which is a correction factor for an ensemble of
velocities with zero total linear momentum. For compute temp/partial,
if one or more velocity components are excluded, the value used for
*extra* is scaled accordingly. You can use a negative number for the
*extra* parameter if you need to add degrees-of-freedom. See the
:doc:`compute temp/asphere <compute_temp_asphere>` command for an
example.
The *dynamic/dof* or *dynamic* keyword determines whether the number
of atoms :math:`N` in the compute group and their associated degrees of
freedom (DOF) are re-computed each time a temperature is computed. Only
compute styles that calculate a temperature use this option. By
default, :math:`N` and their DOF are assumed to be constant. If you are
adding atoms or molecules to the system (see the :doc:`fix pour <fix_pour>`,
:doc:`fix deposit <fix_deposit>`, and :doc:`fix gcmc <fix_gcmc>` commands) or
expect atoms or molecules to be lost (e.g., due to exiting the simulation box
or via :doc:`fix evaporate <fix_evaporate>`), then this option should be used
to ensure the temperature is correctly normalized.
of atoms :math:`N` in the compute group and their associated degrees
of freedom (DOF) are re-computed each time a temperature is computed.
Only compute styles that calculate a temperature use this option. By
default, :math:`N` and their DOF are assumed to be constant. If you
are adding atoms or molecules to the system (see the :doc:`fix pour
<fix_pour>`, :doc:`fix deposit <fix_deposit>`, and :doc:`fix gcmc
<fix_gcmc>` commands) or expect atoms or molecules to be lost
(e.g. due to exiting the simulation box or via :doc:`fix evaporate
<fix_evaporate>`), then this option should be used to insure the
temperature is correctly normalized.
.. note::

7
doc/src/compute_nbond_atom.rst
View File

@ -23,6 +23,8 @@ Examples
Description
"""""""""""
.. versionadded:: 4May2022
Define a computation that computes the number of bonds each atom is
part of. Bonds which are broken are not counted in the tally. See
the :doc:`Howto broken bonds <Howto_bpm>` page for more information.
@ -40,8 +42,9 @@ LAMMPS output options.
Restrictions
""""""""""""
This fix can only be used if LAMMPS was built with the BPM package.
See the :doc:`Build package <Build_package>` doc page for more info.
This compute is part of the BPM package. It is only enabled if LAMMPS was
built with that package. See the :doc:`Build package <Build_package>`
page for more info.
Related commands
""""""""""""""""

2
doc/src/compute_pair_local.rst
View File

@ -59,7 +59,7 @@ commands.
The value *dist* is the distance between the pair of atoms.
The values *dx*, *dy*, and *dz* are the :math:`(x,y,z)` components of the
*distance* between the pair of atoms. This value is always the
distance from the atom of lower to the one with the higher id.
distance from the atom of higher to the one with the lower atom ID.
The value *eng* is the interaction energy for the pair of atoms.

71
doc/src/compute_property_chunk.rst
View File

@ -12,7 +12,8 @@ Syntax
* ID, group-ID are documented in :doc:`compute <compute>` command
* property/chunk = style name of this compute command
* input = one or more attributes
* chunkID = ID of :doc:`compute chunk/atom <compute_chunk_atom>` command that defines the chunks
* input1,etc = one or more attributes
.. parsed-literal::
@ -26,8 +27,8 @@ Examples
.. code-block:: LAMMPS
compute 1 all property/chunk count
compute 1 all property/chunk ID coord1
compute 1 all property/chunk bin2d id count
compute 1 all property/chunk myChunks id coord1
Description
"""""""""""
@ -35,29 +36,28 @@ Description
Define a computation that stores the specified attributes of chunks of
atoms.
In LAMMPS, chunks are collections of atoms defined by a
:doc:`compute chunk/atom <compute_chunk_atom>` command, which assigns each atom
to a single chunk (or no chunk). The ID for this command is specified
as chunkID. For example, a single chunk could be the atoms in a molecule or
atoms in a spatial bin. See the :doc:`compute chunk/atom <compute_chunk_atom>`
and :doc:`Howto chunk <Howto_chunk>` doc pages for details of how chunks can be
defined and examples of how they can be used to measure properties of a system.
In LAMMPS, chunks are collections of atoms defined by a :doc:`compute
chunk/atom <compute_chunk_atom>` command, which assigns each atom to a
single chunk (or no chunk). The ID for this command is specified as
chunkID. For example, a single chunk could be the atoms in a molecule
or atoms in a spatial bin. See the :doc:`compute chunk/atom
<compute_chunk_atom>` and :doc:`Howto chunk <Howto_chunk>` doc pages
for details of how chunks can be defined and examples of how they can
be used to measure properties of a system.
This compute calculates and stores the specified attributes of chunks
as global data so they can be accessed by other
:doc:`output commands <Howto_output>` and used in conjunction with other
commands that generate per-chunk data, such as
:doc:`compute com/chunk <compute_com_chunk>` or
:doc:`compute msd/chunk <compute_msd_chunk>`.
as global data so they can be accessed by other :doc:`output commands
<Howto_output>` and used in conjunction with other commands that
generate per-chunk data, such as :doc:`compute com/chunk
<compute_com_chunk>` or :doc:`compute msd/chunk <compute_msd_chunk>`.
Note that only atoms in the specified group contribute to the
calculation of the *count* attribute. The
:doc:`compute chunk/atom <compute_chunk_atom>` command defines its own group;
atoms will have a chunk ID = 0 if they are not in that group,
signifying they are not assigned to a chunk, and will thus also not
contribute to this calculation. You can specify the "all" group for
this command if you simply want to include atoms with non-zero chunk
IDs.
calculation of the *count* attribute. The :doc:`compute chunk/atom
<compute_chunk_atom>` command defines its own group; atoms will have a
chunk ID = 0 if they are not in that group, signifying they are not
assigned to a chunk, and will thus also not contribute to this
calculation. You can specify the "all" group for this command if you
simply want to include atoms with non-zero chunk IDs.
The *count* attribute is the number of atoms in the chunk.
@ -66,21 +66,24 @@ can only be used if the *compress* keyword was set to *yes* for the
:doc:`compute chunk/atom <compute_chunk_atom>` command referenced by
chunkID. This means that the original chunk IDs (e.g., molecule IDs)
will have been compressed to remove chunk IDs with no atoms assigned
to them. Thus a compressed chunk ID of 3 may correspond to an original
chunk ID (molecule ID in this case) of 415. The *id* attribute will
then be 415 for the third chunk.
to them. Thus a compressed chunk ID of 3 may correspond to an
original chunk ID (molecule ID in this case) of 415. The *id*
attribute will then be 415 for the third chunk.
The *coordN* attributes can only be used if a *binning* style was used
in the :doc:`compute chunk/atom <compute_chunk_atom>` command referenced
by chunkID. For *bin/1d*, *bin/2d*, and *bin/3d* styles the attribute
is the center point of the bin in the corresponding dimension. Style
*bin/1d* only defines a *coord1* attribute. Style *bin/2d* adds a
*coord2* attribute. Style *bin/3d* adds a *coord3* attribute.
Note that if the value of the *units* keyword used in the :doc:`compute chunk/atom command <compute_chunk_atom>` is *box* or *lattice*, the
*coordN* attributes will be in distance :doc:`units <units>`. If the
value of the *units* keyword is *reduced*, the *coordN* attributes
will be in unitless reduced units (0--1).
in the :doc:`compute chunk/atom <compute_chunk_atom>` command
referenced by chunkID. For *bin/1d*, *bin/2d*, and *bin/3d* styles
the attribute is the center point of the bin in the corresponding
dimension. Style *bin/1d* only defines a *coord1* attribute. Style
*bin/2d* adds a *coord2* attribute. Style *bin/3d* adds a *coord3*
attribute.
Note that if the value of the *units* keyword used in the
:doc:`compute chunk/atom command <compute_chunk_atom>` is *box* or
*lattice*, the *coordN* attributes will be in distance :doc:`units
<units>`. If the value of the *units* keyword is *reduced*, the
*coordN* attributes will be in unitless reduced units (0-1).
The simplest way to output the results of the compute property/chunk
calculation to a file is to use the :doc:`fix ave/time <fix_ave_time>`

114
doc/src/compute_property_grid.rst Normal file
View File

@ -0,0 +1,114 @@
.. index:: compute property/grid
compute property/grid command
=============================
Syntax
""""""
.. parsed-literal::
compute ID group-ID property/grid Nx Ny Nz input1 input2 ...
* ID, group-ID are documented in :doc:`compute <compute>` command
* property/grid = style name of this compute command
* Nx, Ny, Nz = grid size in each dimension
* input1,etc = one or more attributes
.. parsed-literal::
attributes = id, ix, iy, iz, x, y, z, xs, ys, zs, xc, yc, zc, xsc, ysc, zsc
id = ID of grid cell, x fastest, y next, z slowest
ix,iy,iz = grid indices in each dimension (1 to N inclusive)
x,y,z = coords of lower left corner of grid cell
xs,ys,zs = scaled coords of lower left corner of grid cell (0.0 to 1.0)
xc,yc,zc = coords of center point of grid cell
xsc,ysc,zsc = scaled coords of center point of grid cell (0.0 to 1.0)
Examples
""""""""
.. code-block:: LAMMPS
compute 1 all property/grid id ix iy iz
compute 1 all property/grid id xc yc zc
Description
"""""""""""
Define a computation that stores the specified attributes of a
distributed grid. In LAMMPS, distributed grids are regular 2d or 3d
grids which overlay a 2d or 3d simulation domain. Each processor owns
the grid cells whose center points lie within its sub-domain. See the
:doc:`Howto grid <Howto_grid>` doc page for details of how distributed
grids can be defined by various commands and referenced.
This compute stores the specified attributes of grids as per-grid data
so they can be accessed by other :doc:`output commands <Howto_output>`
such as :doc:`dump grid <dump>`.
*Nx*, *Ny*, and *Nz* define the size of the grid. For a 2d simulation
*Nz* must be 1. When this compute is used by :doc:`dump grid <dump>`,
to output per-grid values from other computes of fixes, the grid size
specified for this command must be consistent with the grid sizes
used by the other commands.
The *id* attribute stores the grid ID for each grid cell. For a
global grid of size Nx by Ny by Nz (in 3d simulations) the grid IDs
range from 1 to Nx*Ny*Nz. They are ordered with the X index of the 3d
grid varying fastest, then Y, then Z slowest. For 2d grids (in 2d
simulations), the grid IDs range from 1 to Nx*Ny, with X varying
fastest and Y slowest.
The *ix*, *iy*, *iz* attributes are the indices of a grid cell in
each dimension. They range from 1 to Nx inclusive in the X dimension,
and similar for Y and Z.
The *x*, *y*, *z* attributes are the coordinates of the lower left
corner point of each grid cell.
The *xs*, *ys*, *zs* attributes are also coordinates of the lower left
corner point of each grid cell, except in scaled coordinates, where
the lower-left corner of the entire simulation box is (0,0,0) and the
upper right corner is (1,1,1).
The *xc*, *yc*, *zc* attributes are the coordinates of the center
point of each grid cell.
The *xsc*, *ysc*, *zsc* attributes are also coordinates of the center
point each grid cell, except in scaled coordinates, where the
lower-left corner of the entire simulation box is (0,0,0) and the upper
right corner is (1,1,1).
For :doc:`triclinic simulation boxes <Howto_triclinic>`, the grid
point coordinates for (x,y,z) and (xc,yc,zc) will reflect the
triclinic geometry. For (xs,yz,zs) and (xsc,ysc,zsc), the coordinates
are the same for orthogonal versus triclinic boxes.
Output info
"""""""""""
This compute calculates a per-grid vector or array depending on the
number of input values. The length of the vector or number of array
rows (distributed across all processors) is Nx * Ny * Nz. For access
by other commands, the name of the single grid produced by this
command is "grid". The name of its per-grid data is "data".
The (x,y,z) and (xc,yc,zc) coordinates are in distance :doc:`units
<units>`.
Restrictions
""""""""""""
For 2d simulations, the attributes which refer to
the Z dimension cannot be used.
Related commands
""""""""""""""""
:doc:`dump grid <dump>`
Default
"""""""
none

27
doc/src/compute_property_local.rst
View File

@ -85,10 +85,11 @@ Description
"""""""""""
Define a computation that stores the specified attributes as local
data so it can be accessed by other :doc:`output commands <Howto_output>`. If the input attributes refer to bond
information, then the number of datums generated, aggregated across
all processors, equals the number of bonds in the system. Ditto for
pairs, angles, etc.
data so it can be accessed by other :doc:`output commands
<Howto_output>`. If the input attributes refer to bond information,
then the number of datums generated, aggregated across all processors,
equals the number of bonds in the system. Ditto for pairs, angles,
etc.
If multiple attributes are specified then they must all generate the
same amount of information, so that the resulting local array has the
@ -129,17 +130,20 @@ specified compute group. Likewise for angles, dihedrals, etc.
For bonds and angles, a bonds/angles that have been broken by setting
their bond/angle type to 0 will not be included. Bonds/angles that
have been turned off (see the :doc:`fix shake <fix_shake>` or
:doc:`delete_bonds <delete_bonds>` commands) by setting their bond/angle
type negative are written into the file. This is consistent with the
:doc:`compute bond/local <compute_bond_local>` and :doc:`compute angle/local <compute_angle_local>` commands
:doc:`delete_bonds <delete_bonds>` commands) by setting their
bond/angle type negative are written into the file. This is
consistent with the :doc:`compute bond/local <compute_bond_local>` and
:doc:`compute angle/local <compute_angle_local>` commands
Note that as atoms migrate from processor to processor, there will be
no consistent ordering of the entries within the local vector or array
from one timestep to the next. The only consistency that is
guaranteed is that the ordering on a particular timestep will be the
same for local vectors or arrays generated by other compute commands.
For example, output from the :doc:`compute bond/local <compute_bond_local>` command can be combined with bond
atom indices from this command and output by the :doc:`dump local <dump>` command in a consistent way.
For example, output from the :doc:`compute bond/local
<compute_bond_local>` command can be combined with bond atom indices
from this command and output by the :doc:`dump local <dump>` command
in a consistent way.
The *natom1* and *natom2* or *patom1* and *patom2* attributes refer
to the atom IDs of the 2 atoms in each pairwise interaction computed
@ -177,9 +181,8 @@ the array is the number of bonds, angles, etc. If a single input is
specified, a local vector is produced. If two or more inputs are
specified, a local array is produced where the number of columns = the
number of inputs. The vector or array can be accessed by any command
that uses local values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output
options.
that uses local values from a compute as input. See the :doc:`Howto
output <Howto_output>` page for an overview of LAMMPS output options.
The vector or array values will be integers that correspond to the
specified attribute.

32
doc/src/compute_temp.rst
View File

@ -29,8 +29,9 @@ Description
Define a computation that calculates the temperature of a group of
atoms. A compute of this style can be used by any command that
computes a temperature (e.g., :doc:`thermo_modify <thermo_modify>`,
:doc:`fix temp/rescale <fix_temp_rescale>`, :doc:`fix npt <fix_nh>`)
computes a temperature, e.g. :doc:`thermo_modify <thermo_modify>`,
:doc:`fix temp/rescale <fix_temp_rescale>`, :doc:`fix npt <fix_nh>`,
etc.
The temperature is calculated by the formula
@ -39,17 +40,17 @@ The temperature is calculated by the formula
\text{KE} = \frac{\text{dim}}{2} N k_B T,
where KE = total kinetic energy of the group of atoms (sum of
:math:`\frac12 m v^2`), dim = 2 or 3 is the dimensionality of the simulation,
:math:`N` is the number of atoms in the group, :math:`k_B` is the Boltzmann
constant, and :math:`T` is the absolute temperature.
:math:`\frac12 m v^2`), dim = 2 or 3 is the dimensionality of the
simulation, :math:`N` is the number of atoms in the group, :math:`k_B`
is the Boltzmann constant, and :math:`T` is the absolute temperature.
A kinetic energy tensor, stored as a six-element vector, is also
calculated by this compute for use in the computation of a pressure
tensor. The formula for the components of the tensor is the same as
the above formula, except that :math:`v^2` is replaced by
:math:`v_x v_y` for the :math:`xy` component, and so on.
The six components of the vector are ordered :math:`xx`, :math:`yy`,
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
the above formula, except that :math:`v^2` is replaced by :math:`v_x
v_y` for the :math:`xy` component, and so on. The six components of
the vector are ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`,
:math:`xz`, :math:`yz`.
The number of atoms contributing to the temperature is assumed to be
constant for the duration of the run; use the *dynamic* option of the
@ -85,11 +86,10 @@ Output info
"""""""""""
This compute calculates a global scalar (the temperature) and a global
vector of length six (KE tensor), which can be accessed by indices 1--6.
These values can be used by any command that uses global scalar or
vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output
options.
vector of length six (KE tensor), which can be accessed by indices
1--6. These values can be used by any command that uses global scalar
or vector values from a compute as input. See the :doc:`Howto output
<Howto_output>` page for an overview of LAMMPS output options.
The scalar value calculated by this compute is "intensive". The
vector values are "extensive".
@ -104,7 +104,9 @@ Restrictions
Related commands
""""""""""""""""
:doc:`compute temp/partial <compute_temp_partial>`, :doc:`compute temp/region <compute_temp_region>`, :doc:`compute pressure <compute_pressure>`
:doc:`compute temp/partial <compute_temp_partial>`,
:doc:`compute temp/region <compute_temp_region>`,
:doc:`compute pressure <compute_pressure>`
Default
"""""""

25
doc/src/create_box.rst
View File

@ -66,20 +66,21 @@ positive or negative values and are called "tilt factors" because they
are the amount of displacement applied to faces of an originally
orthogonal box to transform it into the parallelepiped.
By default, a *prism* region used with the create_box command must
have tilt factors :math:`(xy,xz,yz)` that do not skew the box more than half
By default, a *prism* region used with the create_box command must have
tilt factors :math:`(xy,xz,yz)` that do not skew the box more than half
the distance of the parallel box length. For example, if
:math:`x_\text{lo} = 2` and :math:`x_\text{hi} = 12`, then the :math:`x`
box length is 10 and the :math:`xy` tilt factor must be between :math:`-5` and
:math:`5`. Similarly, both :math:`xz` and :math:`yz` must be between
:math:`-(x_\text{hi}-x_\text{lo})/2` and :math:`+(y_\text{hi}-y_\text{lo})/2`.
Note that this is not a limitation, since if the maximum tilt factor is 5 (as
in this example), then configurations with tilt :math:`= \dots, -15`,
:math:`-5`, :math:`5`, :math:`15`, :math:`25, \dots`
are all geometrically equivalent. If you wish to define a box with tilt
factors that exceed these limits, you can use the :doc:`box tilt <box>`
command, with a setting of *large*\ ; a setting of *small* is the
default.
box length is 10 and the :math:`xy` tilt factor must be between
:math:`-5` and :math:`5`. Similarly, both :math:`xz` and :math:`yz`
must be between :math:`-(x_\text{hi}-x_\text{lo})/2` and
:math:`+(y_\text{hi}-y_\text{lo})/2`. Note that this is not a
limitation, since if the maximum tilt factor is 5 (as in this example),
then configurations with tilt :math:`= \dots, -15`, :math:`-5`,
:math:`5`, :math:`15`, :math:`25, \dots` are all geometrically
equivalent. Simulations with large tilt factors will run inefficiently,
since they require more ghost atoms and thus more communication. With
very large tilt factors, LAMMPS will eventually produce incorrect
trajectories and stop with errors due to lost atoms or similar.
See the :doc:`Howto triclinic <Howto_triclinic>` page for a
geometric description of triclinic boxes, as defined by LAMMPS, and

4
doc/src/delete_atoms.rst
View File

@ -135,7 +135,7 @@ number of atoms in the system. Note that this is not done for
molecular systems (see the :doc:`atom_style <atom_style>` command),
regardless of the *compress* setting, since it would foul up the bond
connectivity that has already been assigned. However, the
:doc:`reset_atom_ids <reset_atom_ids>` command can be used after this
:doc:`reset_atoms id <reset_atoms>` command can be used after this
command to accomplish the same thing.
Note that the re-assignment of IDs is not really a compression, where
@ -203,7 +203,7 @@ using molecule template files via the :doc:`molecule <molecule>` and
Related commands
""""""""""""""""
:doc:`create_atoms <create_atoms>`, :doc:`reset_atom_ids <reset_atom_ids>`
:doc:`create_atoms <create_atoms>`, :doc:`reset_atoms id <reset_atoms>`
Default
"""""""

4
doc/src/dihedral_table.rst
View File

@ -114,6 +114,10 @@ below.
----------
Suitable tables for use with this dihedral style can be created using
the Python code in the ``tools/tabulate`` folder of the LAMMPS source
code distribution.
The format of a tabulated file is as follows (without the
parenthesized comments). It can begin with one or more comment
or blank lines.

658
doc/src/dump.rst
View File

@ -3,6 +3,8 @@
.. index:: dump cfg
.. index:: dump custom
.. index:: dump dcd
.. index:: dump grid
.. index:: dump grid/vtk
.. index:: dump local
.. index:: dump xtc
.. index:: dump yaml
@ -57,46 +59,48 @@ Syntax
.. code-block:: LAMMPS
dump ID group-ID style N file args
dump ID group-ID style N file attribute1 attribute2 ...
* ID = user-assigned name for the dump
* group-ID = ID of the group of atoms to be dumped
* style = *atom* or *atom/adios* or *atom/gz* or *atom/zstd* or *atom/mpiio* or *cfg* or *cfg/gz* or *cfg/zstd* or *cfg/mpiio* or *cfg/uef* or *custom* or *custom/gz* or *custom/zstd* or *custom/mpiio* or *custom/adios* or *dcd* or *h5md* or *image* or *local* or *local/gz* or *local/zstd* or *molfile* or *movie* or *netcdf* or *netcdf/mpiio* or *vtk* or *xtc* or *xyz* or *xyz/gz* or *xyz/zstd* or *xyz/mpiio* or *yaml*
* style = *atom* or *atom/adios* or *atom/gz* or *atom/zstd* or *atom/mpiio* or *cfg* or *cfg/gz* or *cfg/zstd* or *cfg/mpiio* or *cfg/uef* or *custom* or *custom/gz* or *custom/zstd* or *custom/mpiio* or *custom/adios* or *dcd* or *grid* or *grid/vtk* or *h5md* or *image* or *local* or *local/gz* or *local/zstd* or *molfile* or *movie* or *netcdf* or *netcdf/mpiio* or *vtk* or *xtc* or *xyz* or *xyz/gz* or *xyz/zstd* or *xyz/mpiio* or *yaml*
* N = dump on timesteps which are multiples of N
* file = name of file to write dump info to
* args = list of arguments for a particular style
* attribute1,attribute2,... = list of attributes for a particular style
.. parsed-literal::
*atom* args = none
*atom/adios* args = none, discussed on :doc:`dump atom/adios <dump_adios>` page
*atom/gz* args = none
*atom/zstd* args = none
*atom/mpiio* args = none
*cfg* args = same as *custom* args, see below
*cfg/gz* args = same as *custom* args, see below
*cfg/zstd* args = same as *custom* args, see below
*cfg/mpiio* args = same as *custom* args, see below
*cfg/uef* args = same as *custom* args, discussed on :doc:`dump cfg/uef <dump_cfg_uef>` page
*custom*, *custom/gz*, *custom/zstd*, *custom/mpiio* args = see below
*custom/adios* args = same as *custom* args, discussed on :doc:`dump custom/adios <dump_adios>` page
*dcd* args = none
*h5md* args = discussed on :doc:`dump h5md <dump_h5md>` page
*image* args = discussed on :doc:`dump image <dump_image>` page
*local*, *local/gz*, *local/zstd* args = see below
*molfile* args = discussed on :doc:`dump molfile <dump_molfile>` page
*movie* args = discussed on :doc:`dump image <dump_image>` page
*netcdf* args = discussed on :doc:`dump netcdf <dump_netcdf>` page
*netcdf/mpiio* args = discussed on :doc:`dump netcdf <dump_netcdf>` page
*vtk* args = same as *custom* args, see below, also :doc:`dump vtk <dump_vtk>` page
*xtc* args = none
*xyz* args = none
*xyz/gz* args = none
*xyz/zstd* args = none
*xyz/mpiio* args = none
*yaml* args = same as *custom* args, see below
*atom* attributes = none
*atom/adios* attributes = none, discussed on :doc:`dump atom/adios <dump_adios>` page
*atom/gz* attributes = none
*atom/zstd* attributes = none
*atom/mpiio* attributes = none
*cfg* attributes = same as *custom* attributes, see below
*cfg/gz* attributes = same as *custom* attributes, see below
*cfg/zstd* attributes = same as *custom* attributes, see below
*cfg/mpiio* attributes = same as *custom* attributes, see below
*cfg/uef* attributes = same as *custom* attributes, discussed on :doc:`dump cfg/uef <dump_cfg_uef>` page
*custom*, *custom/gz*, *custom/zstd*, *custom/mpiio* attributes = see below
*custom/adios* attributes = same as *custom* attributes, discussed on :doc:`dump custom/adios <dump_adios>` page
*dcd* attributes = none
*h5md* attributes = discussed on :doc:`dump h5md <dump_h5md>` page
*grid* attributes = see below
*grid/vtk* attributes = see below
*image* attributes = discussed on :doc:`dump image <dump_image>` page
*local*, *local/gz*, *local/zstd* attributes = see below
*molfile* attributes = discussed on :doc:`dump molfile <dump_molfile>` page
*movie* attributes = discussed on :doc:`dump image <dump_image>` page
*netcdf* attributes = discussed on :doc:`dump netcdf <dump_netcdf>` page
*netcdf/mpiio* attributes = discussed on :doc:`dump netcdf <dump_netcdf>` page
*vtk* attributes = same as *custom* attributes, see below, also :doc:`dump vtk <dump_vtk>` page
*xtc* attributes = none
*xyz* attributes = none
*xyz/gz* attributes = none
*xyz/zstd* attributes = none
*xyz/mpiio* attributes = none
*yaml* attributes = same as *custom* attributes, see below
* *custom* or *custom/gz* or *custom/zstd* or *custom/mpiio* or *cfg* or *cfg/gz* or *cfg/zstd* or *cfg/mpiio* or *cfg/uef* or *netcdf* or *netcdf/mpiio* or *yaml* args = list of atom attributes
* *custom* or *custom/gz* or *custom/zstd* or *custom/mpiio* or *cfg* or *cfg/gz* or *cfg/zstd* or *cfg/mpiio* or *cfg/uef* or *netcdf* or *netcdf/mpiio* or *yaml* attributes:
.. parsed-literal::
@ -143,7 +147,7 @@ Syntax
i2_name[I] = Ith column of custom integer array with name, I can include wildcard (see below)
d2_name[I] = Ith column of custom floating point vector with name, I can include wildcard (see below)
* *local* or *local/gz* or *local/zstd* args = list of local attributes
* *local* or *local/gz* or *local/zstd* attributes:
.. parsed-literal::
@ -154,6 +158,18 @@ Syntax
f_ID = local vector calculated by a fix with ID
f_ID[I] = Ith column of local array calculated by a fix with ID, I can include wildcard (see below)
* *grid* or *grid/vtk* attributes:
.. parsed-literal::
possible attributes = c_ID:gname:dname, c_ID:gname:dname[I], f_ID:gname:dname, f_ID:gname:dname[I]
gname = name of grid defined by compute or fix
dname = name of data field defined by compute or fix
c_ID = per-grid vector calculated by a compute with ID
c_ID[I] = Ith column of per-grid array calculated by a compute with ID, I can include wildcard (see below)
f_ID = per-grid vector calculated by a fix with ID
f_ID[I] = Ith column of per-grid array calculated by a fix with ID, I can include wildcard (see below)
Examples
""""""""
@ -176,24 +192,32 @@ Examples
Description
"""""""""""
Dump a snapshot of atom quantities to one or more files once every
:math:`N` timesteps in one of several styles. The *image* and *movie*
styles are the exception: the *image* style renders a JPG, PNG, or PPM
image file of the atom configuration every :math:`N` timesteps while
the *movie* style combines and compresses them into a movie file; both
are discussed in detail on the :doc:`dump image <dump_image>` page.
The timesteps on which dump output is written can also be controlled
by a variable. See the :doc:`dump_modify every <dump_modify>`
command.
Dump a snapshot of quantities to one or more files once every
:math:`N` timesteps in one of several styles. The timesteps on which
dump output is written can also be controlled by a variable. See the
:doc:`dump_modify every <dump_modify>` command.
Almost all the styles output per-atom data, i.e. one or more values
per atom. The exceptions are as follows. The *local* styles output
one or more values per bond (angle, dihedral, improper) or per pair of
interacting atoms (force or neighbor interactions). The *grid* styles
output one or more values per grid cell, which are produced by other
commands which overlay the simulation domain with a regular grid. See
the :doc:`Howto grid <Howto_grid>` doc page for details. The *image*
style renders a JPG, PNG, or PPM image file of the system for each
snapshot, while the *movie* style combines and compresses the series
of images into a movie file; both styles are discussed in detail on
the :doc:`dump image <dump_image>` page.
Only information for atoms in the specified group is dumped. The
:doc:`dump_modify thresh and region and refresh <dump_modify>` commands
can also alter what atoms are included. Not all styles support
these options; see details on the :doc:`dump_modify <dump_modify>` doc page.
:doc:`dump_modify thresh and region and refresh <dump_modify>`
commands can also alter what atoms are included. Not all styles
support these options; see details on the :doc:`dump_modify
<dump_modify>` doc page.
As described below, the filename determines the kind of output (text
or binary or gzipped, one big file or one per timestep, one big file
or multiple smaller files).
As described below, the filename determines the kind of output: text
or binary or gzipped, one big file or one per timestep, one file for
all the processors or multiple smaller files.
.. note::
@ -202,79 +226,66 @@ or multiple smaller files).
to a dump file may be slightly outside the simulation box.
Re-neighbor timesteps will not typically coincide with the
timesteps dump snapshots are written. See the :doc:`dump_modify
pbc <dump_modify>` command if you with to force coordinates to be
pbc <dump_modify>` command if you wish to force coordinates to be
strictly inside the simulation box.
.. note::
Unless the :doc:`dump_modify sort <dump_modify>` option is
invoked, the lines of atom information written to dump files
(typically one line per atom) will be in an indeterminate order for
each snapshot. This is even true when running on a single processor,
if the :doc:`atom_modify sort <atom_modify>` option is on, which it is
by default. In this case atoms are re-ordered periodically during a
simulation, due to spatial sorting. It is also true when running in
parallel, because data for a single snapshot is collected from
multiple processors, each of which owns a subset of the atoms.
Unless the :doc:`dump_modify sort <dump_modify>` option is invoked,
the lines of atom or grid information written to dump files
(typically one line per atom or grid cell) will be in an
indeterminate order for each snapshot. This is even true when
running on a single processor, if the :doc:`atom_modify sort
<atom_modify>` option is on, which it is by default. In this case
atoms are re-ordered periodically during a simulation, due to
spatial sorting. It is also true when running in parallel, because
data for a single snapshot is collected from multiple processors,
each of which owns a subset of the atoms.
For the *atom*, *custom*, *cfg*, and *local* styles, sorting is off by
default. For the *dcd*, *xtc*, *xyz*, and *molfile* styles, sorting
by atom ID is on by default. See the :doc:`dump_modify <dump_modify>`
page for details.
For the *atom*, *custom*, *cfg*, *grid*, and *local* styles, sorting
is off by default. For the *dcd*, *grid/vtk*, *xtc*, *xyz*, and
*molfile* styles, sorting by atom ID or grid ID is on by default. See
the :doc:`dump_modify <dump_modify>` page for details.
The *atom/gz*, *cfg/gz*, *custom/gz*, *local/gz*, and *xyz/gz* styles
are identical in command syntax to the corresponding styles without
"gz", however, they generate compressed files using the zlib
library. Thus the filename suffix ".gz" is mandatory. This is an
alternative approach to writing compressed files via a pipe, as done by
the regular dump styles, which may be required on clusters where the
interface to the high-speed network disallows using the fork() library
call (which is needed for a pipe). For the remainder of this page, you
should thus consider the *atom* and *atom/gz* styles (etc.) to be
inter-changeable, with the exception of the required filename suffix.
The *style* keyword determines what kind of data is written to the
dump file(s) and in what format.
Similarly, the *atom/zstd*, *cfg/zstd*, *custom/zstd*, *local/zstd*, and
*xyz/zstd* styles are identical to the gz styles, but use the Zstd
compression library instead and require the ".zst" suffix. See the
:doc:`dump_modify <dump_modify>` page for details on how to control the
compression level in both variants.
Note that *atom*, *custom*, *dcd*, *xtc*, *xyz*, and *yaml* style dump
files can be read directly by `VMD <https://www.ks.uiuc.edu/Research/vmd>`_,
a popular tool for visualizing and analyzing trajectories from atomic
and molecular systems. For reading *netcdf* style dump files, the
netcdf plugin needs to be recompiled from source using a NetCDF version
compatible with the one used by LAMMPS. The bundled plugin binary
uses a very old version of NetCDF that is not compatible with LAMMPS.
As explained below, the *atom/mpiio*, *cfg/mpiio*, *custom/mpiio*, and
*xyz/mpiio* styles are identical in command syntax and in the format of
the dump files they create, to the corresponding styles without "mpiio",
except the single dump file they produce is written in parallel via the
MPI-IO library. For the remainder of this page, you should thus
consider the *atom* and *atom/mpiio* styles (etc.) to be
inter-changeable. The one exception is how the filename is specified
for the MPI-IO styles, as explained below.
Likewise the `OVITO visualization package <https://www.ovito.org>`_,
popular for materials modeling, can read the *atom*, *custom*,
*local*, *xtc*, *cfg*, *netcdf*, and *xyz* style atom dump files
directly. With version 3.8 and above, OVITO can also read and
visualize *grid* style dump files with grid cell data, including
iso-surface images of the grid cell values.
.. warning::
The MPIIO package is currently unmaintained and has become
unreliable. Use with caution.
The precision of values output to text-based dump files can be
controlled by the :doc:`dump_modify format <dump_modify>` command and
its options.
Note that settings made via the :doc:`dump_modify <dump_modify>`
command can also alter the format of individual values and content of
the dump file itself. This includes the precision of values output to
text-based dump files which is controlled by the :doc:`dump_modify
format <dump_modify>` command and its options.
----------
The *style* keyword determines what atom quantities are written to the
file and in what format. Settings made via the
:doc:`dump_modify <dump_modify>` command can also alter the format of
individual values and the file itself.
Format of native LAMMPS format dump files:
The *atom*, *local*, and *custom* styles create files in a simple text
format that is self-explanatory when viewing a dump file. Some of the
LAMMPS post-processing tools described on the :doc:`Tools <Tools>` doc
page, including `Pizza.py <https://lammps.github.io/pizza>`_,
work with this format, as does the :doc:`rerun <rerun>` command.
The *atom*, *custom*, *grid*, and *local* styles create files in a
simple LAMMPS-specific text format that is self-explanatory when
viewing a dump file. Many post-processing tools either included with
LAMMPS or third-party tools can read this format, as does the
:doc:`rerun <rerun>` command. See tools described on the :doc:`Tools
<Tools>` doc page for examples, including `Pizza.py
<https://lammps.github.io/pizza>`_.
For post-processing purposes the *atom*, *local*, and *custom* text
files are self-describing in the following sense.
The dimensions of the simulation box are included in each snapshot.
For an orthogonal simulation box this information is formatted as:
For all these styles, the dimensions of the simulation box are
included in each snapshot. For an orthogonal simulation box this
information is formatted as:
.. parsed-literal::
@ -316,10 +327,13 @@ bounding box extents (xlo_bound, xhi_bound, etc.) are calculated from the
triclinic parameters, and how to transform those parameters to and
from other commonly used triclinic representations.
The "ITEM: ATOMS" line in each snapshot lists column descriptors for
the per-atom lines that follow. For example, the descriptors would be
"id type xs ys zs" for the default *atom* style, and would be the atom
attributes you specify in the dump command for the *custom* style.
The *atom* and *custom* styles output a "ITEM: NUMBER OF ATOMS" line
with the count of atoms in the snapshot. Likewise they output an
"ITEM: ATOMS" line which includes column descriptors for the per-atom
lines that follow. For example, the descriptors would be "id type xs
ys zs" for the default *atom* style, and would be the atom attributes
you specify in the dump command for the *custom* style. Each
subsequent line will list the data for a single atom.
For style *atom*, atom coordinates are written to the file, along with
the atom ID and atom type. By default, atom coords are written in a
@ -332,12 +346,31 @@ added for each atom via dump_modify.
Style *custom* allows you to specify a list of atom attributes to be
written to the dump file for each atom. Possible attributes are
listed above and will appear in the order specified. You cannot
specify a quantity that is not defined for a particular simulation---such as
*q* for atom style *bond*, since that atom style does not
assign charges. Dumps occur at the very end of a timestep, so atom
attributes will include effects due to fixes that are applied during
the timestep. An explanation of the possible dump custom attributes
is given below.
specify a quantity that is not defined for a particular
simulation---such as *q* for atom style *bond*, since that atom style
does not assign charges. Dumps occur at the very end of a timestep,
so atom attributes will include effects due to fixes that are applied
during the timestep. An explanation of the possible dump custom
attributes is given below.
.. versionadded:: 22Dec2022
For style *grid* the extent of the Nx by Ny by Nz grid that overlays
the simulation domain is output with each snapshot:
.. parsed-literal::
ITEM: GRID EXTENT
nx ny nz
For 2d simulations, nz will be 1. There will also be an "ITEM: GRID
DATA" line which includes column descriptors for the per grid cell
data. Each subsequent line (Nx * Ny * Nz lines) will list the data
for a single grid cell. If grid cell IDs are included in the output
via the :doc:`compute property/grid <compute_property_grid>` command,
then the IDs will range from 1 to N = Nx*Ny*Nz. The ordering of IDs
is with the x index varying fastest, then the y index, and the z index
varying slowest.
For style *local*, local output generated by :doc:`computes <compute>`
and :doc:`fixes <fix>` is used to generate lines of output that is
@ -351,6 +384,17 @@ generate information on bonds, angles, etc. that can be cut and pasted
directly into a data file read by the :doc:`read_data <read_data>`
command.
----------
Dump files in other popular formats:
.. note::
This section only discusses file formats relevant to this doc page.
The top of this page has links to other dump commands (with their
own pages) which write files in additional popular formats.
Style *cfg* has the same command syntax as style *custom* and writes
extended CFG format files, as used by the `AtomEye
<http://li.mit.edu/Archive/Graphics/A/>`_ visualization package.
@ -387,15 +431,15 @@ periodic box. Note that these coordinates may thus be far outside
the box size stored with the snapshot.
The *xtc* style writes XTC files, a compressed trajectory format used
by the GROMACS molecular dynamics package, and described
`here <https://manual.gromacs.org/current/reference-manual/file-formats.html#xtc>`_.
by the GROMACS molecular dynamics package, and described `here
<https://manual.gromacs.org/current/reference-manual/file-formats.html#xtc>`_.
The precision used in XTC files can be adjusted via the
:doc:`dump_modify <dump_modify>` command. The default value of 1000
means that coordinates are stored to 1/1000 nanometer accuracy. XTC
files are portable binary files written in the NFS XDR data format,
so that any machine which supports XDR should be able to read them.
The number of atoms per snapshot cannot change with the *xtc* style.
The *unwrap* option of the :doc:`dump_modify <dump_modify>` command allows
files are portable binary files written in the NFS XDR data format, so
that any machine which supports XDR should be able to read them. The
number of atoms per snapshot cannot change with the *xtc* style. The
*unwrap* option of the :doc:`dump_modify <dump_modify>` command allows
XTC coordinates to be written "unwrapped" by the image flags for each
atom. Unwrapped means that if the atom has passed through a periodic
boundary one or more times, the value is printed for what the
@ -404,27 +448,41 @@ box. Note that these coordinates may thus be far outside the box size
stored with the snapshot.
The *xyz* style writes XYZ files, which is a simple text-based
coordinate format that many codes can read. Specifically it has
a line with the number of atoms, then a comment line that is
usually ignored followed by one line per atom with the atom type
and the :math:`x`-, :math:`y`-, and :math:`z`-coordinate of that atom.
You can use the :doc:`dump_modify element <dump_modify>` option to change the
output from using the (numerical) atom type to an element name (or some other
label). This will help many visualization programs to guess bonds and colors.
coordinate format that many codes can read. Specifically it has a line
with the number of atoms, then a comment line that is usually ignored
followed by one line per atom with the atom type and the :math:`x`-,
:math:`y`-, and :math:`z`-coordinate of that atom. You can use the
:doc:`dump_modify element <dump_modify>` option to change the output
from using the (numerical) atom type to an element name (or some other
label). This will help many visualization programs to guess bonds and
colors.
.. versionadded:: 22Dec2022
The *grid/vtk* style writes VTK files for grid data on a regular
rectilinear grid. Its content is conceptually similar to that of the
text file produced by the *grid* style, except that it in an XML-based
format which visualization programs which support the VTK format can
read, e.g. the `ParaView tool <https://www.paraview.org>`_. For this
style, there can only be 1 or 3 per grid cell attributes specified.
If it is a single value, it is a scalar quantity. If 3 values are
specified it is encoded in the VTK file as a vector quantity (for each
grid cell). The filename for this style must include a "\*" wildcard
character to produce one file per snapshot; see details below.
.. versionadded:: 4May2022
Dump style *yaml* has the same command syntax as style *custom* and
writes YAML format files that can be easily parsed by a variety of data
processing tools and programming languages. Each timestep will be
written as a YAML "document" (i.e., starts with "---" and ends with
writes YAML format files that can be easily parsed by a variety of
data processing tools and programming languages. Each timestep will
be written as a YAML "document" (i.e., starts with "---" and ends with
"..."). The style supports writing one file per timestep through the
"\*" wildcard but not multi-processor outputs with the "%" token in the
filename. In addition to per-atom data, :doc:`thermo <thermo>` data can
be included in the *yaml* style dump file using the :doc:`dump_modify
thermo yes <dump_modify>`. The data included in the dump file uses the
"thermo" tag and is otherwise identical to data specified by the
:doc:`thermo_style <thermo_style>` command.
"\*" wildcard but not multi-processor outputs with the "%" token in
the filename. In addition to per-atom data, :doc:`thermo <thermo>`
data can be included in the *yaml* style dump file using the
:doc:`dump_modify thermo yes <dump_modify>`. The data included in the
dump file uses the "thermo" tag and is otherwise identical to data
specified by the :doc:`thermo_style <thermo_style>` command.
Below is an example for a YAML format dump created by the following commands.
@ -435,13 +493,13 @@ Below is an example for a YAML format dump created by the following commands.
The tags "time", "units", and "thermo" are optional and enabled by the
dump_modify command. The list under the "box" tag has three lines for
orthogonal boxes and four lines for triclinic boxes, where the first three are
the box boundaries and the fourth the three tilt factors (:math:`xy`,
:math:`xz`, :math:`yz`). The "thermo" data follows the format of the *yaml*
thermo style. The "keywords" tag lists the per-atom properties contained in
the "data" columns, which contain a list with one line per atom. The keywords
may be renamed using the dump_modify command same as for the *custom* dump
style.
orthogonal boxes and four lines for triclinic boxes, where the first
three are the box boundaries and the fourth the three tilt factors
(:math:`xy`, :math:`xz`, :math:`yz`). The "thermo" data follows the
format of the *yaml* thermo style. The "keywords" tag lists the
per-atom properties contained in the "data" columns, which contain a
list with one line per atom. The keywords may be renamed using the
dump_modify command same as for the *custom* dump style.
.. code-block:: yaml
@ -479,11 +537,7 @@ style.
----------
Note that *atom*, *custom*, *dcd*, *xtc*, and *xyz* style dump files
can be read directly by `VMD <https://www.ks.uiuc.edu/Research/vmd>`_, a
popular molecular viewing program.
----------
Frequency of dump output:
Dumps are performed on timesteps that are a multiple of :math:`N`
(including timestep 0) and on the last timestep of a minimization if
@ -508,29 +562,35 @@ every/time <dump_modify>` command can be used. This can be useful
when the timestep size varies during a simulation run, e.g. by use of
the :doc:`fix dt/reset <fix_dt_reset>` command.
The specified filename determines how the dump file(s) is written.
The default is to write one large text file, which is opened when the
dump command is invoked and closed when an :doc:`undump <undump>`
command is used or when LAMMPS exits. For the *dcd* and *xtc* styles,
this is a single large binary file.
----------
Dump filenames can contain two wildcard characters. If a "\*"
character appears in the filename, then one file per snapshot is
written and the "\*" character is replaced with the timestep value.
For example, tmp.dump.\* becomes tmp.dump.0, tmp.dump.10000,
tmp.dump.20000, etc. This option is not available for the *dcd* and
*xtc* styles. Note that the :doc:`dump_modify pad <dump_modify>`
command can be used to insure all timestep numbers are the same length
(e.g., 00010), which can make it easier to read a series of dump files
in order with some post-processing tools.
Dump filenames:
The specified dump filename determines how the dump file(s) is
written. The default is to write one large text file, which is opened
when the dump command is invoked and closed when an :doc:`undump
<undump>` command is used or when LAMMPS exits. For the *dcd* and
*xtc* styles, this is a single large binary file.
Many of the styles allow dump filenames to contain either or both of
two wildcard characters. If a "\*" character appears in the filename,
then one file per snapshot is written and the "\*" character is
replaced with the timestep value. For example, tmp.dump.\* becomes
tmp.dump.0, tmp.dump.10000, tmp.dump.20000, etc. This option is not
available for the *dcd* and *xtc* styles. Note that the
:doc:`dump_modify pad <dump_modify>` command can be used to insure all
timestep numbers are the same length (e.g., 00010), which can make it
easier to read a series of dump files in order with some
post-processing tools.
If a "%" character appears in the filename, then each of P processors
writes a portion of the dump file, and the "%" character is replaced
with the processor ID from :math:`0` to :math:`P-1`. For example, tmp.dump.%
becomes tmp.dump.0, tmp.dump.1, ... tmp.dump.:math:`P-1`, etc. This creates
smaller files and can be a fast mode of output on parallel machines that
support parallel I/O for output. This option is **not** available for the
*dcd*, *xtc*, *xyz*, and *yaml* styles.
with the processor ID from :math:`0` to :math:`P-1`. For example,
tmp.dump.% becomes tmp.dump.0, tmp.dump.1, ... tmp.dump.:math:`P-1`,
etc. This creates smaller files and can be a fast mode of output on
parallel machines that support parallel I/O for output. This option is
**not** available for the *dcd*, *xtc*, *xyz*, *grid/vtk*, and *yaml*
styles.
By default, :math:`P` is the the number of processors, meaning one file per
processor, but :math:`P` can be set to a smaller value via the *nfile* or
@ -541,47 +601,41 @@ when running on large numbers of processors.
Note that using the "\*" and "%" characters together can produce a
large number of small dump files!
For the *atom/mpiio*, *cfg/mpiio*, *custom/mpiio*, and *xyz/mpiio*
styles, a single dump file is written in parallel via the MPI-IO
library, which is part of the MPI standard for versions 2.0 and above.
Using MPI-IO requires two steps. First, build LAMMPS with its MPIIO
package installed, viz.,
.. code-block:: bash
make yes-mpiio # installs the MPIIO package
make mpi # build LAMMPS for your platform
Second, use a dump filename which contains ".mpiio". Note that it does
not have to end in ".mpiio", just contain those characters. Unlike
MPI-IO restart files, which must be both written and read using MPI-IO,
the dump files produced by these MPI-IO styles are identical in format
to the files produced by their non-MPI-IO style counterparts. This
means you can write a dump file using MPI-IO and use the :doc:`read_dump
For styles that end with *mpiio* an ".mpiio" must appear somewhere in
the specified filename. These styles write their dump file in
parallel via the MPI-IO library, which is part of the MPI standard for
versions 2.0 and above. Note these styles are identical in command
syntax to the corresponding styles without "mpiio". Likewise, the
dump files produced by these MPI-IO styles are identical in format to
the files produced by their non-MPI-IO style counterparts. This means
you can write a dump file using MPI-IO and use the :doc:`read_dump
<read_dump>` command or perform other post-processing, just as if the
dump file was not written using MPI-IO.
Because MPI-IO dump files are one large file which all processors
write to, you cannot use the "%" wildcard character described above in
the filename. However you can use the ".bin" or ".lammpsbin" suffix
described below. Again, this file will be written in parallel and
have the same binary format as if it were written without MPI-IO.
.. warning::
The MPIIO package is currently unmaintained and has become
unreliable. Use with caution.
The MPIIO package within LAMMPS is currently unmaintained and has
become unreliable. Use with caution.
Note that MPI-IO dump files are one large file which all processors
write to. You thus cannot use the "%" wildcard character described
above in the filename since that specifies generation of multiple files.
You can use the ".bin" or ".lammpsbin" suffix described below in an
MPI-IO dump file; again this file will be written in parallel and have
the same binary format as if it were written without MPI-IO.
----------
If the filename ends with ".bin" or ".lammpsbin", the dump file (or
files, if "\*" or "%" is also used) is written in binary format. A
binary dump file will be about the same size as a text version, but will
typically write out much faster. Of course, when post-processing, you
will need to convert it back to text format (see the :ref:`binary2txt
tool <binary>`) or write your own code to read the binary file. The
format of the binary file can be understood by looking at the
:file:`tools/binary2txt.cpp` file. This option is only available for
the *atom* and *custom* styles.
Compression of dump file data:
If the specified filename ends with ".bin" or ".lammpsbin", the dump
file (or files, if "\*" or "%" is also used) is written in binary
format. A binary dump file will be about the same size as a text
version, but will typically write out much faster. Of course, when
post-processing, you will need to convert it back to text format (see
the :ref:`binary2txt tool <binary>`) or write your own code to read
the binary file. The format of the binary file can be understood by
looking at the :file:`tools/binary2txt.cpp` file. This option is only
available for the *atom* and *custom* styles.
If the filename ends with ".gz", the dump file (or files, if "\*" or "%"
is also used) is written in gzipped format. A gzipped dump file will be
@ -589,19 +643,40 @@ about :math:`3\times` smaller than the text version, but will also take
longer to write. This option is not available for the *dcd* and *xtc*
styles.
Note that styles that end with *gz* are identical in command syntax to
the corresponding styles without "gz", however, they generate
compressed files using the zlib library. Thus the filename suffix
".gz" is mandatory. This is an alternative approach to writing
compressed files via a pipe, as done by the regular dump styles, which
may be required on clusters where the interface to the high-speed
network disallows using the fork() library call (which is needed for a
pipe). For the remainder of this page, you should thus consider the
*atom* and *atom/gz* styles (etc.) to be inter-changeable, with the
exception of the required filename suffix.
Similarly, styles that end with *zstd* are identical to the gz styles,
but use the Zstd compression library instead and require a ".zst"
suffix. See the :doc:`dump_modify <dump_modify>` page for details on
how to control the compression level in both variants.
----------
Note that in the discussion which follows, for styles which can
reference values from a compute or fix or custom atom property, like the
*custom*\ , *cfg*\ , or *local* styles, the bracketed index :math:`i`
can be specified using a wildcard asterisk with the index to effectively
specify multiple values. This takes the form "\*" or "\*n" or "m\*" or
"m\*n". If :math:`N` is the number of columns in the array, then an
asterisk with no numeric values means all column indices from 1 to
:math:`N`. A leading asterisk means all indices from 1 to n
(inclusive). A trailing asterisk means all indices from m to :math:`N`
(inclusive). A middle asterisk means all indices from m to n
(inclusive).
Arguments for different styles:
The sections below describe per-atom, local, and per grid cell
attributes which can be used as arguments to the various styles.
Note that in the discussion below, for styles which can reference
values from a compute or fix or custom atom property, like the
*custom*\ , *cfg*\ , *grid* or *local* styles, the bracketed index
:math:`i` can be specified using a wildcard asterisk with the index to
effectively specify multiple values. This takes the form "\*" or
"\*n" or "m\*" or "m\*n". If :math:`N` is the number of columns in
the array, then an asterisk with no numeric values means all column
indices from 1 to :math:`N`. A leading asterisk means all indices
from 1 to n (inclusive). A trailing asterisk means all indices from m
to :math:`N` (inclusive). A middle asterisk means all indices from m
to n (inclusive).
Using a wildcard is the same as if the individual columns of the array
had been listed one by one. For example, these two dump commands are
@ -617,63 +692,7 @@ command creates a per-atom array with six columns:
----------
This section explains the local attributes that can be specified as
part of the *local* style.
The *index* attribute can be used to generate an index number from 1
to :math:`N` for each line written into the dump file, where :math:`N` is the
total number of local datums from all processors, or lines of output that
will appear in the snapshot. Note that because data from different
processors depend on what atoms they currently own, and atoms migrate
between processor, there is no guarantee that the same index will be
used for the same info (e.g., a particular bond) in successive snapshots.
The *c_ID* and *c_ID[I]* attributes allow local vectors or arrays
calculated by a :doc:`compute <compute>` to be output. The ID in the
attribute should be replaced by the actual ID of the compute that has
been defined previously in the input script. See the
:doc:`compute <compute>` command for details. There are computes for
calculating local information such as indices, types, and energies for
bonds and angles.
Note that computes which calculate global or per-atom quantities, as
opposed to local quantities, cannot be output in a dump local command.
Instead, global quantities can be output by the :doc:`thermo_style
custom <thermo_style>` command, and per-atom quantities can be output
by the dump custom command.
If *c_ID* is used as a attribute, then the local vector calculated by
the compute is printed. If *c_ID[i]* is used, then :math:`i` must be in the
range from :math:`1-M`, which will print the Ith column of the local array
with :math:`M` columns calculated by the compute. See the discussion above
for how :math:`i` can be specified with a wildcard asterisk to effectively
specify multiple values.
The *f_ID* and *f_ID[I]* attributes allow local vectors or arrays
calculated by a :doc:`fix <fix>` to be output. The ID in the attribute
should be replaced by the actual ID of the fix that has been defined
previously in the input script.
If *f_ID* is used as a attribute, then the local vector calculated by
the fix is printed. If *f_ID[i]* is used, then :math:`i` must be in the
range :math:`1`--:math:`M`, which will print the :math:`i`\ th column of the
local with :math:`M` columns calculated by the fix. See the discussion above
for how :math:`i` can be specified with a wildcard asterisk to effectively
specify multiple values.
Here is an example of how to dump bond info for a system, including
the distance and energy of each bond:
.. code-block:: LAMMPS
compute 1 all property/local batom1 batom2 btype
compute 2 all bond/local dist eng
dump 1 all local 1000 tmp.dump index c_1[1] c_1[2] c_1[3] c_2[1] c_2[2]
----------
This section explains the atom attributes that can be specified as
part of the *custom* and *cfg* styles.
Per-atom attributes used as arguments to the *custom* and *cfg* styles:
The *id*, *mol*, *proc*, *procp1*, *type*, *element*, *mass*, *vx*,
*vy*, *vz*, *fx*, *fy*, *fz*, *q* attributes are self-explanatory.
@ -808,6 +827,97 @@ which could then be output into dump files.
----------
Attributes used as arguments to the *local* style:
The *index* attribute can be used to generate an index number from 1
to N for each line written into the dump file, where N is the total
number of local datums from all processors, or lines of output that
will appear in the snapshot. Note that because data from different
processors depend on what atoms they currently own, and atoms migrate
between processor, there is no guarantee that the same index will be
used for the same info (e.g. a particular bond) in successive
snapshots.
The *c_ID* and *c_ID[I]* attributes allow local vectors or arrays
calculated by a :doc:`compute <compute>` to be output. The ID in the
attribute should be replaced by the actual ID of the compute that has
been defined previously in the input script. See the
:doc:`compute <compute>` command for details. There are computes for
calculating local information such as indices, types, and energies for
bonds and angles.
Note that computes which calculate global or per-atom quantities, as
opposed to local quantities, cannot be output in a dump local command.
Instead, global quantities can be output by the :doc:`thermo_style
custom <thermo_style>` command, and per-atom quantities can be output
by the dump custom command.
If *c_ID* is used as a attribute, then the local vector calculated by
the compute is printed. If *c_ID[I]* is used, then I must be in the
range from 1-M, which will print the Ith column of the local array
with M columns calculated by the compute. See the discussion above
for how I can be specified with a wildcard asterisk to effectively
specify multiple values.
The *f_ID* and *f_ID[I]* attributes allow local vectors or arrays
calculated by a :doc:`fix <fix>` to be output. The ID in the attribute
should be replaced by the actual ID of the fix that has been defined
previously in the input script.
If *f_ID* is used as a attribute, then the local vector calculated by
the fix is printed. If *f_ID[I]* is used, then I must be in the
range from 1-M, which will print the Ith column of the local with M
columns calculated by the fix. See the discussion above for how I can
be specified with a wildcard asterisk to effectively specify multiple
values.
Here is an example of how to dump bond info for a system, including
the distance and energy of each bond:
.. code-block:: LAMMPS
compute 1 all property/local batom1 batom2 btype
compute 2 all bond/local dist eng
dump 1 all local 1000 tmp.dump index c_1[1] c_1[2] c_1[3] c_2[1] c_2[2]
----------
Attributes used as arguments to the *grid* and *grid/vtk* styles:
The attributes that begin with *c_ID* and *f_ID* both take
colon-separated fields *gname* and *dname*. These refer to a grid
name and data field name which is defined by the compute or fix. Note
that a compute or fix can define one or more grids (of different
sizes) and one or more data fields for each of those grids. The sizes
of all grids output in a single dump grid command must be the same.
The *c_ID:gname:dname* and *c_ID:gname:dname[I]* attributes allow
per-grid vectors or arrays calculated by a :doc:`compute <compute>` to
be output. The ID in the attribute should be replaced by the actual
ID of the compute that has been defined previously in the input
script.
If *c_ID:gname:dname* is used as a attribute, then the per-grid vector
calculated by the compute is printed. If *c_ID:gname:dname[I]* is
used, then I must be in the range from 1-M, which will print the Ith
column of the per-grid array with M columns calculated by the compute.
See the discussion above for how I can be specified with a wildcard
asterisk to effectively specify multiple values.
The *f_ID:gname:dname* and *f_ID:gname:dname[I]* attributes allow
per-grid vectors or arrays calculated by a :doc:`fix <fix>` to be
output. The ID in the attribute should be replaced by the actual ID
of the fix that has been defined previously in the input script.
If *f_ID:gname:dname* is used as a attribute, then the per-grid vector
calculated by the fix is printed. If *f_ID:gname:dname[I]* is used,
then I must be in the range from 1-M, which will print the Ith column
of the per-grid with M columns calculated by the fix. See the
discussion above for how I can be specified with a wildcard asterisk
to effectively specify multiple values.
----------
Restrictions
""""""""""""
@ -816,9 +926,9 @@ To write gzipped dump files, you must either compile LAMMPS with the
See the :doc:`Build settings <Build_settings>` page for details.
While a dump command is active (i.e., has not been stopped by using
the :doc:`undump command <undump>`), no commands may be used that will change
the timestep (e.g., :doc:`reset_timestep <reset_timestep>`). LAMMPS
will terminate with an error otherwise.
the :doc:`undump command <undump>`), no commands may be used that will
change the timestep (e.g., :doc:`reset_timestep <reset_timestep>`).
LAMMPS will terminate with an error otherwise.
The *atom/gz*, *cfg/gz*, *custom/gz*, and *xyz/gz* styles are part of
the COMPRESS package. They are only enabled if LAMMPS was built with

Some files were not shown because too many files have changed in this diff Show More