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196 Commits

Author SHA1 Message Date
59d100ab57 final prep for 22Nov patch 2016-11-22 09:23:02 -07:00
61e71d23ed Merge pull request #288 from akohlmey/moltemplate-1.40
update bundled version of moltemplate to v1.40
2016-11-22 08:51:11 -07:00
b6f2f0e6e9 Merge pull request #287 from rbberger/pylammps/docs
Created PyLammps documentation
2016-11-22 08:50:29 -07:00
ff0441ac16 Merge pull request #286 from akohlmey/small-fixes-and-updates
Collected small fixes and updates
2016-11-22 08:49:46 -07:00
41907d3110 Merge pull request #285 from akohlmey/fix-ipi-update
update for fix ipi from michele ceriotti
2016-11-22 08:48:27 -07:00
b95f255af4 small changes to temper/grem commands 2016-11-22 08:47:44 -07:00
d7b542101a Merge pull request #283 from akohlmey/grem-feature
gREM generalized replica exchange feature for USER-MISC
2016-11-22 08:15:35 -07:00
0ffa50f8e8 tweaked author syntax 2016-11-22 08:15:13 -07:00
7893215964 small comment/whitespace tweak 2016-11-21 12:46:43 -05:00
3dff9f2018 removed extra file 2016-11-21 12:05:30 -05:00
dab232c542 modified temper_grem name to fit conventions, re-ran example to match 2016-11-21 12:02:17 -05:00
9e9d9d5aa5 update bundled version of moltemplate to v1.40 2016-11-21 11:34:42 -05:00
c982b174a2 Merge pull request #49 from epfl-cosmo/fix-ipi
i-PI interface fix
2016-11-19 19:36:13 -05:00
87a5a35bad A tiny bugfix for the reset flag, and a brief explanation of the changes 2016-11-20 00:44:23 +01:00
fd174ce2b1 Merge branch 'fix-ipi-update' of https://github.com/akohlmey/lammps into fix-ipi 2016-11-20 00:04:56 +01:00
b11f376a4f Merge branch 'master' of github.com:lammps/lammps 2016-11-19 23:25:51 +01:00
230b29eae6 correct accelerator flags for dpd styles in pair style overview 2016-11-19 11:47:12 -05:00
2383c31f15 Created PyLammps documentation
Based on material presented during MD Workshop at Temple University in
August 2016.
2016-11-18 23:58:57 -07:00
e175a18bdb be more thorough in initializing optional data in pair style dpd/fdt/energy 2016-11-18 16:18:47 -05:00
a5bde82e37 update .gitignore for recent addition 2016-11-18 15:38:11 -05:00
d787afcca9 also remove generated html files with 'make clean' in docs folder 2016-11-18 15:37:49 -05:00
176cde8ed3 minor cleanups 2016-11-18 15:36:38 -05:00
2862c20815 Merge branch 'master' into grem-feature 2016-11-18 14:51:46 -05:00
78e018829f Merge branch 'grem-feature' of https://github.com/dstelter92/lammps into grem-feature 2016-11-18 14:48:47 -05:00
c78914e7b3 update for fix ipi from michele ceriotti 2016-11-18 09:21:50 -05:00
635f3ce128 synchronize USER-SMD examples with code 2016-11-18 08:09:24 -05:00
81f68e06fd Merge branch 'master' into doc-updates 2016-11-17 20:44:07 -05:00
4b51719e67 new 17Nov16 patch and stable 2016-11-17 16:51:35 -07:00
25d7be5f3d compute pressure doc change 2016-11-17 16:11:30 -07:00
2a026c9ad8 revised temper_grem example, better file management 2016-11-17 12:53:25 -05:00
4a3091f844 modified temper_grem example with more exchanges 2016-11-17 11:24:29 -05:00
74c0e4dd5c Merge pull request #278 from akohlmey/pair-agni
Implementation of the AGNI manybody potential
2016-11-17 09:04:31 -07:00
073e8a0524 Merge pull request #276 from akohlmey/doc-updates
Small bugfixes and updates
2016-11-17 09:02:27 -07:00
5320bbf585 Merge pull request #275 from andeplane/IP_VORONOI
Initializing pointers in VORONOI
2016-11-17 09:01:46 -07:00
4448819824 Merge pull request #274 from andeplane/IP_POEMS
Initialize pointers in POEMS
2016-11-17 09:01:37 -07:00
300ac30332 Merge pull request #273 from akohlmey/auto-memalign
turn on -DLAMMPS_MEMALIGN=64 automatically when USER-INTEL is installed
2016-11-17 09:01:27 -07:00
2535e44991 Merge pull request #271 from akohlmey/tersoff-modc
pair style tersoff/mod/c
2016-11-17 09:00:52 -07:00
747c95c525 revised documentation, added temper_grem ref to fix_grem 2016-11-17 11:00:49 -05:00
cdae794383 Merge pull request #242 from andeplane/vashishta_kokkos
Added KOKKOS vashishta
2016-11-17 09:00:03 -07:00
8756a1017d Kokkos updates by Stan 2016-11-17 08:58:22 -07:00
5c64934bc8 added documention, re-ran temper_grem example 2016-11-17 10:40:10 -05:00
4e62e58d29 Merge pull request #47 from dstelter92/grem-feature
added internal tempering in grem with example
2016-11-17 10:04:43 -05:00
5ac2d9532e Re-run example with debug off 2016-11-17 09:43:44 -05:00
19ac9d2959 turned off dev mode by default in temper_grem 2016-11-17 09:31:07 -05:00
9f313aac75 shorter example 2016-11-16 20:43:41 -05:00
0102c5dadc file cleanup 2016-11-16 20:38:53 -05:00
07e46b797a added internal tempering in grem with example 2016-11-16 20:27:14 -05:00
b45d1e37ef integrate fix grem docs and update to match current conventions 2016-11-16 16:46:00 -05:00
2e7fd513d4 provide fix grem example input for nvt and npt 2016-11-16 16:42:01 -05:00
82364d10e3 Merge branch 'grem-feature' of https://github.com/dstelter92/lammps into grem-feature
Resolved merge conflicts and adapted logic to most recent changes in feature branch

Closes #46
2016-11-16 16:11:53 -05:00
16c8a307e5 removed leftover tex files 2016-11-16 15:39:02 -05:00
94f14ab051 spell check, minor typos 2016-11-16 15:34:32 -05:00
22d93fe8fb add restrict to CCFLAGS for makefiles intended for intel compilers 2016-11-16 14:31:10 -05:00
683f514fac simplify multi-replica run by passing per-replica parameters as variables on the command line 2016-11-16 14:22:20 -05:00
f617993944 need to apply fix_modify already in fix grem constructor 2016-11-16 13:52:27 -05:00
4641c9e568 Added basic documentation for grem fix 2016-11-16 13:36:13 -05:00
705f66aaee remove superfluous code 2016-11-16 13:24:41 -05:00
e57ae1ce3f compute scaled kinetic energy tensor without destroying the original data 2016-11-16 12:45:13 -05:00
950442b8b1 added check for nvt vs npt, enabled nvt simulation with fix_grem 2016-11-15 21:53:28 -05:00
1c68e42ecc fix_modify is not longer needed 2016-11-14 13:43:28 -05:00
5f94b31806 add multi-replica example for gREM 2016-11-14 10:12:48 -05:00
fdf5d68f9f allow to extract properties in NH integrator only when they are active 2016-11-14 09:27:33 -05:00
0c25f3b1d6 whitespace cleanup 2016-11-13 23:20:09 -05:00
14c7cf4197 retrieve target temperature and pressure from fix npt. add sanity checks. 2016-11-13 23:18:59 -05:00
26870f223d add example for gREM 2016-11-13 23:18:14 -05:00
09544d0698 bugfix for compute pressure/grem: must make a copy of argument strings 2016-11-13 19:19:52 -05:00
b5130a3b35 avoid NaN for variance from average output 2016-11-13 18:46:55 -05:00
20daf82463 initial import of adapted gREM code by David Stelter and Edyta Malolepsza
The following changes were made:
- the modifications to compute pressure were transferred to a derived class compute pressure/grem
- fix scaleforce was renamed to fix grem
- identifying the grem fix was simplified as fix grem passes an additional argument to compute pressure/grem
- dead code was removed in both files
- checking of arguments was tightened
2016-11-13 18:44:10 -05:00
57124b9b25 update documentation metadata files for recent changes 2016-11-12 09:18:21 -05:00
03b3834fe3 add documentation for pair style agni 2016-11-12 09:07:42 -05:00
d0124eac95 optimized data access and using approximate exponential for USER-OMP version 2016-11-12 08:36:27 -05:00
5685131fe2 add USER-OMP version of pair style agni 2016-11-11 19:08:01 -05:00
22fc92f9d8 use special ev_tally() function suitable for this kind of force compute 2016-11-11 18:32:55 -05:00
b9770766a8 add adatom and vacancy examples for AGNI pair style 2016-11-11 18:19:29 -05:00
9cc0c8badd error exit when requested element is not in potential file 2016-11-11 18:10:57 -05:00
6e1492a86c add potential file for pair style AGNI 2016-11-11 18:10:26 -05:00
9b0987d8c4 first complete implementation of AGNI pair style 2016-11-11 17:32:47 -05:00
e453adaf81 implemented parser for 1 element potential files 2016-11-11 15:53:37 -05:00
8e0fd88697 add example demonstrating the use of fix addtorque 2016-11-11 10:52:50 -05:00
fdcabd7d1d fix addtorque is compatible with dynamic groups 2016-11-11 09:01:18 -05:00
c5c8c50e97 initialize 'nper' 2016-11-11 07:47:42 -05:00
72b0841b28 Merge branch 'doc-updates' of github.com:akohlmey/lammps into doc-updates 2016-11-11 07:44:44 -05:00
801111a7ab dummy framework implementation for AGNI pair style 2016-11-10 15:00:36 -05:00
bfc478c320 simpler variant of the segfault workaround, that does not offend Clang c++. 2016-11-10 14:12:02 -05:00
2b75ee761d avoid segmentation fault, when creating a LAMMPS instance from the library interface. arg[] may be NULL. 2016-11-10 13:28:32 -05:00
352e177fcd Merge branch 'master' into small-fixes-and-updates 2016-11-10 13:26:00 -05:00
c20ee34c7b Initializing pointers in VORONOI 2016-11-10 09:30:07 +01:00
95a7f7160e Initialize pointers in POEMS 2016-11-10 09:26:52 +01:00
1f38e1a771 Merge branch 'master' into doc-updates 2016-11-09 18:18:05 -05:00
9806da69f3 Stan bug fixes for fix reaxc/bonds/kk 2016-11-09 15:47:50 -07:00
fec87c070d simplify compiling USER-INTEL package, by defaulting to -DLAMMPS_MEMALIGN=64 in case it is not set 2016-11-09 16:53:39 -05:00
3d3a99c082 added missing potential for tersoff/mod/c 2016-11-09 16:50:34 -05:00
3e36ec3754 remove unused class member 2016-11-09 16:17:46 -05:00
9ed5c4f0fa Merge branch 'master' into kokkos-vashishta 2016-11-09 15:15:10 -05:00
c55fd502e0 correct typo in formula 2016-11-09 15:04:24 -05:00
71ee2ecaa1 integrate pair style tersoff/mod/c contributed by Ganga P Purja Pun (GMU)
This includes docs, added testing and inclusion of USER-OMP support.
2016-11-09 14:52:39 -05:00
bfea3dce7d Merge pull request #268 from arielzn/born_dsf
pair styles born/coul/dsf and born/coul/dsf/cs added
2016-11-09 11:57:09 -07:00
eef862ee1c Merge pull request #267 from akohlmey/pager-help
use pager for help message, if connected to stdout
2016-11-09 11:53:43 -07:00
0cc2fbf1d6 Merge pull request #266 from andeplane/IP_USER_OMP
Initializing pointers in USER-OMP
2016-11-09 11:52:05 -07:00
ae00666994 Merge pull request #265 from andeplane/IP_DIFF_DPD
Initializing pointers in USER-DIFFRACTION and USER-DPD
2016-11-09 11:51:53 -07:00
51b3b5fb35 Merge pull request #264 from andeplane/IP_SNAP_SRD
Initialize pointers in SNAP and SRD
2016-11-09 11:51:44 -07:00
176f2c3aa1 Merge pull request #263 from andeplane/IP_RIGID_SHOCK
Initialize pointers in RIGID and SHOCK
2016-11-09 11:51:36 -07:00
3f71bfb185 Merge pull request #262 from andeplane/IP_PERI_QEQ_REPLICA
Initializing pointers in PERI, QEQ and REPLICA
2016-11-09 11:51:25 -07:00
cf3ab51679 Merge pull request #261 from andeplane/IP_MISC_MOLECULE
Initialized pointers in MISC and MOLECULE
2016-11-09 11:51:09 -07:00
59922f894b Merge pull request #260 from andeplane/IP_MANYBODY_MC
Initialize pointers in MANYBODY and MC
2016-11-09 11:51:01 -07:00
5e2b9d8bf3 Merge pull request #259 from andeplane/IP_KSPACE
Initialize pointers in KSPACE
2016-11-09 11:50:50 -07:00
2d132cad6b Merge pull request #258 from andeplane/IP_GRANULAR
Initialize pointers in GRANULAR
2016-11-09 11:50:41 -07:00
ef6801f8bf Merge pull request #257 from andeplane/IP_CORESHELL
Initialize pointers in CORESHELL
2016-11-09 11:50:31 -07:00
c81a723642 Merge pull request #256 from andeplane/IP_BODY
Initialized pointers in BODY
2016-11-09 11:50:23 -07:00
f9eb2a99ce Merge pull request #255 from andeplane/IP_ASPHERE
Initialize pointers in ASPHERE
2016-11-09 11:50:11 -07:00
16a02ef27d Merge pull request #254 from andeplane/IP_root
Initialized pointers in src folder
2016-11-09 11:47:21 -07:00
2c801320c2 fixed links in Section_intro.txt 2016-11-09 11:46:10 -07:00
d20b32092e Building correct shortlists and removed rsq test in force loops 2016-11-08 18:57:27 +01:00
9de1a2a08f added input using born/coul/dsf/cs to examples/coreshell 2016-11-08 18:27:44 +01:00
cdb5d47e9f add FLERR argument to force->bounds() in born/coul/dsf 2016-11-08 18:24:54 +01:00
a23b287a7a sync with SVN for creation of stable release 2016-11-08 09:05:50 -07:00
31204aab6a sync with SVN 2016-11-08 08:57:51 -07:00
25e7d074cf documentation added for born/coul/dsf and born/coul/dsf/cs styles 2016-11-08 16:51:54 +01:00
667f4dfe28 pair style born/coul/dsf added with its coreshell version 2016-11-08 11:32:38 +01:00
21694ca3a8 improve help and it through a pager, when screen == stdout 2016-11-07 17:10:12 -05:00
9b910d5511 make name of the actual executable (i.e. arg[0]) accessible 2016-11-07 17:07:40 -05:00
054ab6bff3 Initializing pointers in USER-OMP 2016-11-07 21:07:10 +01:00
616420cda8 Initializing pointers in USER-DIFFRACTION and USER-DPD 2016-11-07 20:51:36 +01:00
fb3ac9afba Initialize pointers in SNAP and SRD 2016-11-07 20:30:38 +01:00
7cd7cda2d4 Initialize pointers in RIGID and SHOCK 2016-11-07 20:22:04 +01:00
db0524278a Initializing pointers in PERI, QEQ and REPLICA 2016-11-07 19:58:27 +01:00
1ff75eaba2 Initialized pointers in MISC and MOLECULE 2016-11-07 17:15:48 +01:00
30dede867a Initialize pointers in MANYBODY and MC 2016-11-07 17:02:32 +01:00
a5c6104d64 Initialize pointers in KSPACE 2016-11-07 16:54:59 +01:00
c5869bdee2 Initialize pointers in GRANULAR 2016-11-07 16:33:50 +01:00
e7a2c6b5d1 Initialize pointers in CORESHELL 2016-11-07 16:26:16 +01:00
06959a9c59 Initialized pointers in BODY 2016-11-07 16:21:08 +01:00
cd65d44d95 Initialize pointers in ASPHERE 2016-11-07 16:15:39 +01:00
45f2e86dd6 NULLed ptrs in files 2016-11-07 16:07:37 +01:00
f8226e8ae5 NULL ptrs in dump_custom and dump_image 2016-11-07 15:56:47 +01:00
b221b15d24 NULLing ptrs in comm_brick and dump*.cpp 2016-11-07 15:50:18 +01:00
3a3d96b877 info styles also prints out pair styles 2016-11-04 18:18:40 -04:00
77bbf03f0f Merge pull request #252 from akohlmey/preinstalled-vs-scm
remove the misleading "(which it is by default)" from several doc files
2016-11-04 10:59:06 -06:00
7cff08ca0a Merge pull request #249 from lammps/unstable
Incorporate merge commits from "unstable" into "master"
2016-11-04 10:58:55 -06:00
f0131393e0 Merge pull request #248 from akohlmey/collected-small-fixes
collected small bugfixes and updates
2016-11-04 10:58:42 -06:00
32e0a58343 Merge pull request #247 from akohlmey/bounds-error-with-code-line
Propagate error error locations for a few more utility functions
2016-11-04 10:58:14 -06:00
60908eeab4 Merge pull request #246 from akohlmey/manybody-short-neighbor-list
Manybody short neighbor list
2016-11-04 10:57:43 -06:00
8214555b29 Merge pull request #244 from ketankhare/patch-2
Enable write_data for dihedral style fourier
2016-11-04 10:57:20 -06:00
f48b71f46b added examples/threebody, fix reaxc/speceies/kk 2016-11-04 10:56:04 -06:00
6cc4eb19af remove the misleading "(which it is by default)" from several doc files 2016-11-04 12:20:17 -04:00
7d23a0737e add thorough checking for valid arguments to -partition or -p 2016-11-04 00:42:23 -04:00
02510ec321 add temporary force accumulation to local variables for vashishta styles 2016-11-02 22:32:30 -04:00
33140e5004 accumulate forces in temporary local variables for tersoff 2016-11-02 22:16:53 -04:00
639fb6f444 use local variables for more efficient force accumulation 2016-11-02 17:20:56 -04:00
b156771721 build short neighbor list for sw on based on ij parameters only 2016-11-02 17:09:32 -04:00
5d787f7f16 avoid tiny memory leak, when the restart command is specified multiple times 2016-11-01 21:39:12 -04:00
c8f4b55588 avoid uninitialized data for using ewald/disp with lj only 2016-11-01 16:48:30 -04:00
e13e4031cf avoid memory leak in pppm/disp/omp 2016-11-01 16:48:00 -04:00
782a328080 avoid memory leaks when using kspace solvers for lennard-jones 2016-11-01 14:55:13 -04:00
e81ae21dbd do not access uninitialized data for ewald/disp and pppm/disp 2016-11-01 14:54:16 -04:00
7fdd6e2807 remove work repetitions for 'the' 2016-11-01 11:40:07 -04:00
2e0d304c7e remove word repetitions for 'a' 2016-11-01 11:36:11 -04:00
f333d659c2 Using short neighborlists in neigh full 2016-10-29 22:54:43 +02:00
51e2313fac Using short neighbor lists 2016-10-29 22:35:29 +02:00
e37d2b5c94 Calculating short neighbor lists 2016-10-29 22:20:37 +02:00
c4b86a25a7 Merge branch 'master' into manybody-short-neighbor-list 2016-10-28 11:12:21 -04:00
218e121b41 Merge branch 'master' into bounds-error-with-code-line 2016-10-28 11:11:28 -04:00
93d393aa69 permission cleanup in tools folder 2016-10-28 10:48:35 -04:00
4216be49f3 Merge branch 'master' into collected-small-fixes 2016-10-28 10:46:33 -04:00
3870780894 Merge branch 'master' into kokkos-vashishta 2016-10-28 10:43:05 -04:00
c3a1e72183 Version 27 Oct 2016 2016-10-27 11:40:36 -04:00
f9a9e27f5a add error location propagation to atom->set_mass() and atom->check_mass() 2016-10-26 16:01:40 -04:00
35753b8f08 add error location propagation to force->bounds() and force->boundsbig() 2016-10-26 15:53:02 -04:00
f028a9a967 region cylinder is compatible with open_faces[2], so do not disallow it. 2016-10-26 15:04:18 -04:00
ef9f7c818e fix off-by-one bug in buffer re-allocator 2016-10-26 10:14:08 -04:00
8e61bed2d8 add USER-OMP variant of manybody short neighbor list 2016-10-26 09:51:52 -04:00
3267b34590 simplify short neighbor list implementation. remove unneeded class member 2016-10-26 09:29:27 -04:00
0a417b4016 add short neighbor list support to pair style tersoff 2016-10-26 07:06:38 -04:00
399c0af150 consistent short neighbor list for vashishta and vashishta/table 2016-10-25 23:46:25 -04:00
e8b3f79690 fully tested multi-element compatible short neighbor list for Stillinger-Weber 2016-10-25 23:18:14 -04:00
21619f6a2f Recommitting reverted change
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15794 f3b2605a-c512-4ea7-a41b-209d697bcdaa
(cherry picked from commit c0b98f5299)
2016-10-25 15:25:39 -04:00
039bda9b61 Added updated vashishta for KOKKOS support
(cherry picked from commit 96089a42547f625e70aa2ac3933d248d2731b731)
2016-10-25 15:07:10 -04:00
6929603eef Added KOKKOS vashishta
(cherry picked from commit 5edc474bf0be574ddba96d00bb63894edf400ddb)
2016-10-25 15:07:10 -04:00
7f3f5e8c38 Clean whitespace 2016-10-25 14:46:44 -04:00
f350500e69 Enable write_data 2016-10-25 14:43:12 -04:00
d7c77a419d Enable write_data for dihedral_fourier 2016-10-25 14:36:18 -04:00
d2da0fabb4 Version 20 Oct 2016 2016-10-19 15:29:13 -04:00
13ce1037f2 Version 18 Oct 2016 2016-10-18 15:46:56 -04:00
fa984b2c3b Version 13 Oct 2016 2016-10-13 19:56:33 -04:00
8540a9f038 Version 11 Oct 2016 2016-10-11 17:10:24 -04:00
13b6eb1bae Version 6 Oct 2016 2016-10-06 19:12:58 -04:00
d80a9def17 Version 5 Oct 2016 2016-10-05 18:49:08 -04:00
be4734bdce Version 30 Sep 2016 2016-09-30 11:57:15 -04:00
2551619b07 Version 29 Sep 2016 2016-09-29 10:55:26 -04:00
d8bf149edc Version 28 Sep 2016 2016-09-29 10:55:18 -04:00
473b12ded4 Version 26 Sep 2016 2016-09-29 10:55:10 -04:00
27c3149590 Version 21 Sep 2016 2016-09-29 10:54:59 -04:00
3b408d71fe Version 20 Sep 2016 2016-09-29 10:53:40 -04:00
0229556b03 Merge branch 'master' of github.com:lammps/lammps 2015-07-03 15:43:29 +02:00
357d4517e8 Merge branch 'master' of github.com:lammps/lammps 2015-04-08 10:46:50 +02:00
a4a97de84f A few GLE fixes 2015-04-08 10:45:49 +02:00
878 changed files with 42831 additions and 2612 deletions

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@ -43,7 +43,7 @@ clean-all:
rm -rf $(BUILDDIR)/* utils/txt2html/txt2html.exe
clean:
rm -rf $(RSTDIR)
rm -rf $(RSTDIR) html
html: $(OBJECTS)
@(\

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\documentclass[12pt]{article}
\begin{document}
$$
T_{eff} = \lambda + \eta (H - H_0)
$$
\end{document}

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\documentclass[12pt]{article}
\pagestyle{empty}
\begin{document}
\begin{eqnarray*}
V_{ij} & = & f_C(r_{ij}) \left[ f_R(r_{ij}) + b_{ij} f_A(r_{ij}) + c_0 \right]
\end{eqnarray*}
\end{document}

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\begin{document}
$$
P = \frac{N k_B T}{V} + \frac{\sum_{i}^{N} r_i \bullet f_i}{dV}
P = \frac{N k_B T}{V} + \frac{\sum_{i}^{N'} r_i \bullet f_i}{dV}
$$
\end{document}

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$$
P_{IJ} = \frac{\sum_{k}^{N} m_k v_{k_I} v_{k_J}}{V} +
\frac{\sum_{k}^{N} r_{k_I} f_{k_J}}{V}
\frac{\sum_{k}^{N'} r_{k_I} f_{k_J}}{V}
$$
\end{document}

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@ -1,7 +1,7 @@
<!-- HTML_ONLY -->
<HEAD>
<TITLE>LAMMPS Users Manual</TITLE>
<META NAME="docnumber" CONTENT="27 Oct 2016 version">
<META NAME="docnumber" CONTENT="22 Nov 2016 version">
<META NAME="author" CONTENT="http://lammps.sandia.gov - Sandia National Laboratories">
<META NAME="copyright" CONTENT="Copyright (2003) Sandia Corporation. This software and manual is distributed under the GNU General Public License.">
</HEAD>
@ -21,7 +21,7 @@
<H1></H1>
LAMMPS Documentation :c,h3
27 Oct 2016 version :c,h4
22 Nov 2016 version :c,h4
Version info: :h4

View File

@ -531,7 +531,8 @@ package"_Section_start.html#start_3.
"dump nc"_dump_nc.html,
"dump nc/mpiio"_dump_nc.html,
"group2ndx"_group2ndx.html,
"ndx2group"_group2ndx.html :tb(c=3,ea=c)
"ndx2group"_group2ndx.html,
"temper/grem"_temper_grem.html :tb(c=3,ea=c)
:line
@ -631,7 +632,7 @@ USER-INTEL, k = KOKKOS, o = USER-OMP, t = OPT.
"rigid/npt (o)"_fix_rigid.html,
"rigid/nve (o)"_fix_rigid.html,
"rigid/nvt (o)"_fix_rigid.html,
"rigid/small (o)"_fix_rigid.html,
<"rigid/small (o)"_fix_rigid.html,
"rigid/small/nph"_fix_rigid.html,
"rigid/small/npt"_fix_rigid.html,
"rigid/small/nve"_fix_rigid.html,
@ -687,6 +688,7 @@ package"_Section_start.html#start_3.
"eos/table/rx"_fix_eos_table_rx.html,
"flow/gauss"_fix_flow_gauss.html,
"gle"_fix_gle.html,
"grem"_fix_grem.html,
"imd"_fix_imd.html,
"ipi"_fix_ipi.html,
"langevin/drude"_fix_langevin_drude.html,
@ -886,6 +888,8 @@ KOKKOS, o = USER-OMP, t = OPT.
"body"_pair_body.html,
"bop"_pair_bop.html,
"born (go)"_pair_born.html,
"born/coul/dsf"_pair_born.html,
"born/coul/dsf/cs"_pair_born.html,
"born/coul/long (go)"_pair_born.html,
"born/coul/long/cs"_pair_born.html,
"born/coul/msm (o)"_pair_born.html,
@ -909,8 +913,8 @@ KOKKOS, o = USER-OMP, t = OPT.
"coul/msm"_pair_coul.html,
"coul/streitz"_pair_coul.html,
"coul/wolf (ko)"_pair_coul.html,
"dpd (o)"_pair_dpd.html,
"dpd/tstat (o)"_pair_dpd.html,
"dpd (go)"_pair_dpd.html,
"dpd/tstat (go)"_pair_dpd.html,
"dsmc"_pair_dsmc.html,
"eam (gkot)"_pair_eam.html,
"eam/alloy (gkot)"_pair_eam.html,
@ -979,11 +983,12 @@ KOKKOS, o = USER-OMP, t = OPT.
"table (gko)"_pair_table.html,
"tersoff (gkio)"_pair_tersoff.html,
"tersoff/mod (gko)"_pair_tersoff_mod.html,
"tersoff/mod/c (o)"_pair_tersoff_mod.html,
"tersoff/zbl (gko)"_pair_tersoff_zbl.html,
"tip4p/cut (o)"_pair_coul.html,
"tip4p/long (o)"_pair_coul.html,
"tri/lj"_pair_tri_lj.html,
"vashishta (o)"_pair_vashishta.html,
"vashishta (ko)"_pair_vashishta.html,
"vashishta/table (o)"_pair_vashishta.html,
"yukawa (go)"_pair_yukawa.html,
"yukawa/colloid (go)"_pair_yukawa_colloid.html,
@ -993,6 +998,7 @@ These are additional pair styles in USER packages, which can be used
if "LAMMPS is built with the appropriate
package"_Section_start.html#start_3.
"agni (o)"_pair_agni.html,
"awpmd/cut"_pair_awpmd.html,
"buck/mdf"_pair_mdf.html,
"coul/cut/soft (o)"_pair_lj_soft.html,

View File

@ -2729,7 +2729,7 @@ production runs and is only required during equilibration. This way one
is consistent with literature (based on the code packages DL_POLY or
GULP for instance).
The mentioned energy transfer will typically lead to a a small drift
The mentioned energy transfer will typically lead to a small drift
in total energy over time. This internal energy can be monitored
using the "compute chunk/atom"_compute_chunk_atom.html and "compute
temp/chunk"_compute_temp_chunk.html commands. The internal kinetic
@ -2830,7 +2830,7 @@ temp/drude"_compute_temp_drude.html. This requires also to use the
command {comm_modify vel yes}.
Short-range damping of the induced dipole interactions can be achieved
using Thole functions through the the "pair style
using Thole functions through the "pair style
thole"_pair_thole.html in "pair_style hybrid/overlay"_pair_hybrid.html
with a Coulomb pair style. It may be useful to use {coul/long/cs} or
similar from the CORESHELL package if the core and Drude particle come

View File

@ -366,11 +366,11 @@ complementary modeling tasks.
"DL_POLY"_dlpoly
"Tinker"_tinker :ul
:link(charmm,http://www.scripps.edu/brooks)
:link(amber,http://amber.scripps.edu)
:link(charmm,http://www.charmm.org)
:link(amber,http://ambermd.org)
:link(namd,http://www.ks.uiuc.edu/Research/namd/)
:link(nwchem,http://www.emsl.pnl.gov/docs/nwchem/nwchem.html)
:link(dlpoly,http://www.cse.clrc.ac.uk/msi/software/DL_POLY)
:link(dlpoly,http://www.ccp5.ac.uk/DL_POLY_CLASSIC)
:link(tinker,http://dasher.wustl.edu/tinker)
CHARMM, AMBER, NAMD, NWCHEM, and Tinker are designed primarily for

View File

@ -8,19 +8,26 @@
11. Python interface to LAMMPS :h3
LAMMPS can work together with Python in two ways. First, Python can
LAMMPS can work together with Python in three ways. First, Python can
wrap LAMMPS through the "LAMMPS library
interface"_Section_howto.html#howto_19, so that a Python script can
create one or more instances of LAMMPS and launch one or more
simulations. In Python lingo, this is "extending" Python with LAMMPS.
Second, LAMMPS can use the Python interpreter, so that a LAMMPS input
Second, the low-level Python interface can be used indirectly through the
PyLammps and IPyLammps wrapper classes in Python. These wrappers try to
simplify the usage of LAMMPS in Python by providing an object-based interface
to common LAMMPS functionality. It also reduces the amount of code necessary to
parameterize LAMMPS scripts through Python and makes variables and computes
directly accessible. See "PyLammps interface"_#py_9 for more details.
Third, LAMMPS can use the Python interpreter, so that a LAMMPS input
script can invoke Python code, and pass information back-and-forth
between the input script and Python functions you write. The Python
code can also callback to LAMMPS to query or change its attributes.
In Python lingo, this is "embedding" Python in LAMMPS.
This section describes how to do both.
This section describes how to use these three approaches.
11.1 "Overview of running LAMMPS from Python"_#py_1
11.2 "Overview of using Python from a LAMMPS script"_#py_2
@ -29,7 +36,8 @@ This section describes how to do both.
11.5 "Extending Python with MPI to run in parallel"_#py_5
11.6 "Testing the Python-LAMMPS interface"_#py_6
11.7 "Using LAMMPS from Python"_#py_7
11.8 "Example Python scripts that use LAMMPS"_#py_8 :ul
11.8 "Example Python scripts that use LAMMPS"_#py_8
11.9 "PyLammps interface"_#py_9 :ul
If you are not familiar with it, "Python"_http://www.python.org is a
powerful scripting and programming language which can essentially do
@ -824,3 +832,7 @@ different visualization package options. Click to see larger images:
:image(JPG/screenshot_atomeye_small.jpg,JPG/screenshot_atomeye.jpg)
:image(JPG/screenshot_pymol_small.jpg,JPG/screenshot_pymol.jpg)
:image(JPG/screenshot_vmd_small.jpg,JPG/screenshot_vmd.jpg)
11.9 PyLammps interface :link(py_9),h4
Please see the "PyLammps Tutorial"_tutorial_pylammps.html.

View File

@ -706,7 +706,7 @@ future changes to LAMMPS.
User packages, such as user-atc or user-omp, have been contributed by
users, and always begin with the user prefix. If they are a single
command (single file), they are typically in the user-misc package.
Otherwise, they are a a set of files grouped together which add a
Otherwise, they are a set of files grouped together which add a
specific functionality to the code.
User packages don't necessarily meet the requirements of the standard

View File

@ -74,7 +74,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -61,7 +61,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -66,7 +66,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -74,7 +74,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -66,7 +66,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -65,11 +65,11 @@ more instructions on how to use the accelerated styles effectively.
:line
[Restrictions:] none
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
MOLECULE package. See the "Making LAMMPS"_Section_start.html#start_3
section for more info on packages.
[Related commands:]

View File

@ -76,7 +76,7 @@ for specific angle types.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other angle styles, the hybrid angle style does not store angle

View File

@ -147,7 +147,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This angle style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -70,7 +70,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
You typically should specify "special_bonds fene"_special_bonds.html

View File

@ -73,7 +73,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
You typically should specify "special_bonds fene"_special_bonds.html

View File

@ -65,7 +65,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -59,7 +59,7 @@ bond types.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other bond styles, the hybrid bond style does not store bond

View File

@ -64,7 +64,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -64,7 +64,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -99,7 +99,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
The {quartic} style requires that "special_bonds"_special_bonds.html

View File

@ -144,7 +144,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This bond style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -114,7 +114,7 @@ local defects surrounding the central atom, as described above. For
the {axes yes} case, the vector components are also unitless, since
they represent spatial directions.
Here are typical centro-symmetry values, from a a nanoindentation
Here are typical centro-symmetry values, from a nanoindentation
simulation into gold (FCC). These were provided by Jon Zimmerman
(Sandia):

View File

@ -536,7 +536,7 @@ For the {bin/cylinder} style the details are as follows. If {discard}
is set to {yes}, an out-of-domain atom will have its chunk ID set to
0. If {discard} is set to {no}, the atom will have its chunk ID set
to the first or last bin in both the radial and axis dimensions. If
{discard} is set to {mixed}, which is the default, the the radial
{discard} is set to {mixed}, which is the default, the radial
dimension is treated the same as for {discard} = no. But for the axis
dimensinon, it will only have its chunk ID set to the first or last
bin if bins extend to the simulation box boundary in the axis

View File

@ -37,12 +37,18 @@ The pressure is computed by the formula
where N is the number of atoms in the system (see discussion of DOF
below), Kb is the Boltzmann constant, T is the temperature, d is the
dimensionality of the system (2 or 3 for 2d/3d), V is the system
volume (or area in 2d), and the second term is the virial, computed
within LAMMPS for all pairwise as well as 2-body, 3-body, and 4-body,
and long-range interactions. "Fixes"_fix.html that impose constraints
(e.g. the "fix shake"_fix_shake.html command) also contribute to the
virial term.
dimensionality of the system (2 or 3 for 2d/3d), and V is the system
volume (or area in 2d). The second term is the virial, equal to
-dU/dV, computed for all pairwise as well as 2-body, 3-body, 4-body,
manybody, and long-range interactions, where r_i and f_i are the
position and force vector of atom i, and the black dot indicates a dot
product. When periodic boundary conditions are used, N' necessarily
includes periodic image (ghost) atoms outside the central box, and the
position and force vectors of ghost atoms are thus included in the
summation. When periodic boundary conditions are not used, N' = N =
the number of atoms in the system. "Fixes"_fix.html that impose
constraints (e.g. the "fix shake"_fix_shake.html command) also
contribute to the virial term.
A symmetric pressure tensor, stored as a 6-element vector, is also
calculated by this compute. The 6 components of the vector are
@ -62,8 +68,9 @@ compute temperature or ke and/or the virial. The {virial} keyword
means include all terms except the kinetic energy {ke}.
Details of how LAMMPS computes the virial efficiently for the entire
system, including the effects of periodic boundary conditions is
discussed in "(Thompson)"_#Thompson.
system, including for manybody potentials and accounting for the
effects of periodic boundary conditions are discussed in
"(Thompson)"_#Thompson.
The temperature and kinetic energy tensor is not calculated by this
compute, but rather by the temperature compute specified with the

View File

@ -60,7 +60,7 @@ produced by a small set of atoms (e.g. 4 atoms in a dihedral or 3
atoms in a Tersoff 3-body interaction) is assigned in equal portions
to each atom in the set. E.g. 1/4 of the dihedral virial to each of
the 4 atoms, or 1/3 of the fix virial due to SHAKE constraints applied
to atoms in a a water molecule via the "fix shake"_fix_shake.html
to atoms in a water molecule via the "fix shake"_fix_shake.html
command.
If no extra keywords are listed, all of the terms in this formula are

View File

@ -69,8 +69,8 @@ velocity for each atom. Note that if there is only one atom in the
bin, its thermal velocity will thus be 0.0.
After the spatially-averaged velocity field has been subtracted from
each atom, the temperature is calculated by the formula KE = (dim/2 N
- dim*Nx*Ny*Nz) k T, where KE = total kinetic energy of the group of
each atom, the temperature is calculated by the formula KE = (dim*N
- dim*Nx*Ny*Nz) k T/2, where KE = total kinetic energy of the group of
atoms (sum of 1/2 m v^2), dim = 2 or 3 = dimensionality of the
simulation, N = number of atoms in the group, k = Boltzmann constant,
and T = temperature. The dim*Nx*Ny*Nz term are degrees of freedom

View File

@ -109,7 +109,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This dihedral style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -76,7 +76,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This dihedral style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -69,7 +69,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This dihedral style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -77,7 +77,7 @@ for specific dihedral types.
[Restrictions:]
This dihedral style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other dihedral styles, the hybrid dihedral style does not store

View File

@ -63,7 +63,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This dihedral style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -71,7 +71,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This dihedral style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -154,7 +154,7 @@ radians instead of degrees. (Note: This changes the way the forces
are scaled in the 4th column of the data file.)
The optional "CHECKU" keyword is followed by a filename. This allows
the user to save all of the the {Ntable} different entries in the
the user to save all of the {Ntable} different entries in the
interpolated energy table to a file to make sure that the interpolated
function agrees with the user's expectations. (Note: You can
temporarily increase the {Ntable} parameter to a high value for this

View File

@ -165,7 +165,7 @@ extra buffering.
:line
The {element} keyword applies only to the the dump {cfg}, {xyz}, and
The {element} keyword applies only to the dump {cfg}, {xyz}, and
{image} styles. It associates element names (e.g. H, C, Fe) with
LAMMPS atom types. See the list of element names at the bottom of
this page.
@ -574,7 +574,7 @@ e.g. its x-component of velocity if the atom-attribute "vx" was
specified.
The basic idea of a color map is that the atom-attribute will be
within a range of values, and that range is associated with a a series
within a range of values, and that range is associated with a series
of colors (e.g. red, blue, green). An atom's specific value (vx =
-3.2) can then mapped to the series of colors (e.g. halfway between
red and blue), and a specific color is determined via an interpolation

View File

@ -113,7 +113,7 @@ quantity being minimized), you MUST enable the
[Restrictions:]
This fix can only be used if LAMMPS was built with the MOLECULE
package (which it is by default). See the "Making
package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -150,7 +150,7 @@ initial box length is 100 Angstroms, and V is 10 Angstroms/psec, then
after 10 psec, the box length will have doubled. After 20 psec, it
will have tripled.
The {erate} style changes a dimension of the the box at a "constant
The {erate} style changes a dimension of the box at a "constant
engineering strain rate". The units of the specified strain rate are
1/time. See the "units"_units.html command for the time units
associated with different choices of simulation units,

111
doc/src/fix_grem.txt Normal file
View File

@ -0,0 +1,111 @@
"LAMMPS WWW Site"_lws - "LAMMPS Documentation"_ld - "LAMMPS Commands"_lc :c
:link(lws,http://lammps.sandia.gov)
:link(ld,Manual.html)
:link(lc,Section_commands.html#comm)
:line
fix grem command :h3
[Syntax:]
fix ID group-ID grem lambda eta H0 thermostat-ID :pre
ID, group-ID are documented in "fix"_fix.html command :ulb,l
grem = style name of this fix command :l
lambda = intercept parameter of linear effective temperature function :l
eta = slope parameter of linear effective temperature function :l
H0 = shift parameter of linear effective temperature function :l
thermostat-ID = ID of Nose-Hoover thermostat or barostat used in simulation :l,ule
[Examples:]
fix fxgREM all grem 400 -0.01 -30000 fxnpt
thermo_modify press fxgREM_press :pre
fix fxgREM all grem 502 -0.15 -80000 fxnvt :pre
[Description:]
This fix implements the molecular dynamics version of the generalized
replica exchange method (gREM) originally developed by "(Kim)"_#Kim,
which uses non-Boltzmann ensembles to sample over first order phase
transitions. The is done by defining replicas with an enthalpy
dependent effective temperature
:c,image(Eqs/fix_grem.jpg)
with {eta} negative and steep enough to only intersect the
characteristic microcanonical temperature (Ts) of the system once,
ensuring a unimodal enthalpy distribution in that replica. {Lambda} is
the intercept and effects the generalized ensemble similar to how
temperature effects a Boltzmann ensemble. {H0} is a reference
enthalpy, and is typically set as the lowest desired sampled enthalpy.
Further explanation can be found in our recent papers
"(Malolepsza)"_#Malolepsza.
This fix requires a Nose-Hoover thermostat fix reference passed to the
grem as {thermostat-ID}. Two distinct temperatures exist in this
generalized ensemble, the effective temperature defined above, and a
kinetic temperature that controls the velocity distribution of
particles as usual. Either constant volume or constant pressure
algorithms can be used.
The fix enforces a generalized ensemble in a single replica
only. Typically, this ideaology is combined with replica exchange with
replicas differing by {lambda} only for simplicity, but this is not
required. A multi-replica simulation can be run within the LAMMPS
environment using the "temper/grem"_temper_grem.html command. This
utilizes LAMMPS partition mode and requires the number of available
processors be on the order of the number of desired replicas. A
100-replica simulation would require at least 100 processors (1 per
world at minimum). If a many replicas are needed on a small number of
processors, multi-replica runs can be run outside of LAMMPS. An
example of this can be found in examples/USER/misc/grem and has no
limit on the number of replicas per processor. However, this is very
inefficient and error prone and should be avoided if possible.
In general, defining the generalized ensembles is unique for every
system. When starting a many-replica simulation without any knowledge
of the underlying microcanonical temperature, there are several tricks
we have utilized to optimize the process. Choosing a less-steep {eta}
yields broader distributions, requiring fewer replicas to map the
microcanonical temperature. While this likely struggles from the same
sampling problems gREM was built to avoid, it provides quick insight
to Ts. Initially using an evenly-spaced {lambda} distribution
identifies regions where small changes in enthalpy lead to large
temperature changes. Replicas are easily added where needed.
:line
[Restart, fix_modify, output, run start/stop, minimize info:]
No information about this fix is written to "binary restart
files"_restart.html.
The "thermo_modify"_thermo_modify.html {press} option is supported
by this fix to add the rescaled kinetic pressure as part of
"thermodynamic output"_thermo_style.html.
[Restrictions:]
This fix is part of the USER-MISC package. It is only enabled if
LAMMPS was built with that package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info.
[Related commands:]
"temper/grem"_temper_grem.html, "fix nvt"_fix_nh.html, "fix
npt"_fix_nh.html, "thermo_modify"_thermo_modify.html
[Default:] none
:line
:link(Kim)
[(Kim)] Kim, Keyes, Straub, J Chem. Phys, 132, 224107 (2010).
:link(Malolepsza)
[(Malolepsza)] Malolepsza, Secor, Keyes, J Phys Chem B 119 (42),
13379-13384 (2015).

View File

@ -10,18 +10,19 @@ fix ipi command :h3
[Syntax:]
fix ID group-ID ipi address port \[unix\] :pre
fix ID group-ID ipi address port \[unix\] \[reset\] :pre
ID, group-ID are documented in "fix"_fix.html command
ipi = style name of this fix command
address = internet address (FQDN or IP), or UNIX socket name
port = port number (ignored for UNIX sockets)
optional keyword = {unix}, if present uses a unix socket :ul
optional keyword = {unix}, if present uses a unix socket
optional keyword = {reset}, if present reset electrostatics at each call :ul
[Examples:]
fix 1 all ipi my.server.com 12345
fix 1 all ipi mysocket 666 unix
fix 1 all ipi mysocket 666 unix reset
[Description:]
@ -57,6 +58,15 @@ input are listed in the same order as in the data file of LAMMPS. The
initial configuration is ignored, as it will be substituted with the
coordinates received from i-PI before forces are ever evaluated.
A note of caution when using potentials that contain long-range
electrostatics, or that contain parameters that depend on box size:
all of these options will be initialized based on the cell size in the
LAMMPS-side initial configuration and kept constant during the run.
This is required to e.g. obtain reproducible and conserved forces.
If the cell varies too wildly, it may be advisable to reinitialize
these interactions at each call. This behavior can be requested by
setting the {reset} switch.
[Restart, fix_modify, output, run start/stop, minimize info:]
There is no restart information associated with this fix, since all

View File

@ -237,7 +237,7 @@ described in the papers cited below, the purpose of this method is to
enable longer timesteps to be used (up to the numerical stability
limit of the integrator), while still producing the correct Boltzmann
distribution of atom positions. It is implemented within LAMMPS, by
changing how the the random force is applied so that it is composed of
changing how the random force is applied so that it is composed of
the average of two random forces representing half-contributions from
the previous and current time intervals.

View File

@ -233,7 +233,7 @@ present, the speed of sound squared is set equal to (1/3)*(dx/dt)^2.
Setting a0 > (dx/dt)^2 is not allowed, as this may lead to
instabilities.
If the {noise} keyword is used, followed by a a positive temperature
If the {noise} keyword is used, followed by a positive temperature
value, and a positive integer random number seed, a thermal
lattice-Boltzmann algorithm is used. If {LBtype} is set equal to 1
(i.e. the standard LB integrator is chosen), the thermal LB algorithm

View File

@ -8,6 +8,7 @@
fix reax/bonds command :h3
fix reax/c/bonds command :h3
fix reax/c/bonds/kk command :h3
[Syntax:]
@ -47,6 +48,31 @@ commands"_Section_howto.html#howto_15. No parameter of this fix can
be used with the {start/stop} keywords of the "run"_run.html command.
This fix is not invoked during "energy minimization"_minimize.html.
:line
Styles with a {gpu}, {intel}, {kk}, {omp}, or {opt} suffix are
functionally the same as the corresponding style without the suffix.
They have been optimized to run faster, depending on your available
hardware, as discussed in "Section_accelerate"_Section_accelerate.html
of the manual. The accelerated styles take the same arguments and
should produce the same results, except for round-off and precision
issues.
These accelerated styles are part of the GPU, USER-INTEL, KOKKOS,
USER-OMP and OPT packages, respectively. They are only enabled if
LAMMPS was built with those packages. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info.
You can specify the accelerated styles explicitly in your input script
by including their suffix, or you can use the "-suffix command-line
switch"_Section_start.html#start_7 when you invoke LAMMPS, or you can
use the "suffix"_suffix.html command in your input script.
See "Section_accelerate"_Section_accelerate.html of the manual for
more instructions on how to use the accelerated styles effectively.
:line
[Restrictions:]
The fix reax/bonds command requires that the "pair_style

View File

@ -7,6 +7,7 @@
:line
fix reax/c/species command :h3
fix reax/c/species/kk command :h3
[Syntax:]
@ -129,6 +130,31 @@ No parameter of this fix can be used with the {start/stop} keywords of
the "run"_run.html command. This fix is not invoked during "energy
minimization"_minimize.html.
:line
Styles with a {gpu}, {intel}, {kk}, {omp}, or {opt} suffix are
functionally the same as the corresponding style without the suffix.
They have been optimized to run faster, depending on your available
hardware, as discussed in "Section_accelerate"_Section_accelerate.html
of the manual. The accelerated styles take the same arguments and
should produce the same results, except for round-off and precision
issues.
These accelerated styles are part of the GPU, USER-INTEL, KOKKOS,
USER-OMP and OPT packages, respectively. They are only enabled if
LAMMPS was built with those packages. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info.
You can specify the accelerated styles explicitly in your input script
by including their suffix, or you can use the "-suffix command-line
switch"_Section_start.html#start_7 when you invoke LAMMPS, or you can
use the "suffix"_suffix.html command in your input script.
See "Section_accelerate"_Section_accelerate.html of the manual for
more instructions on how to use the accelerated styles effectively.
:line
[Restrictions:]
The fix species currently only works with

View File

@ -87,7 +87,7 @@ end of each run. A positive value N means that the diagnostics are reported once
per N time-steps.
The diagnostics report the average # of integrator steps and RHS function evaluations
and run-time per ODE as well as the the average/RMS/min/max per process. If the
and run-time per ODE as well as the average/RMS/min/max per process. If the
reporting frequency is 1, the RMS/min/max per ODE are also reported. The per ODE
statistics can be used to adjust the tolerance and min/max step parameters. The
statistics per MPI process can be useful to examine any load imbalance caused by the

View File

@ -28,7 +28,7 @@ fix 1 all smd/adjust_dt 0.1 :pre
The fix calculates a new stable time increment for use with the SMD time integrators.
The stable time increment is based on multiple conditions. For the SPH pair styles, a
CFL criterion (Courant, Friedrichs & Lewy, 1928) is evaluated, which determines the the speed of
CFL criterion (Courant, Friedrichs & Lewy, 1928) is evaluated, which determines the speed of
sound cannot propagate further than a typical spacing between particles within a single time step to ensure
no information is lost. For the contact pair styles, a linear analysis of the pair potential determines a
stable maximum time step.

View File

@ -101,7 +101,7 @@ particles move in the normal way via a time integration "fix"_fix.html
with a short timestep dt. SRD particles advect with a large timestep
dt_SRD >= dt.
If the {lamda} keyword is not specified, the the SRD temperature
If the {lamda} keyword is not specified, the SRD temperature
{Tsrd} is used in the above formula to compute lamda. If the {lamda}
keyword is specified, then the {Tsrd} setting is ignored and the above
equation is used to compute the SRD temperature.

View File

@ -107,7 +107,7 @@ specified as parameters to the fix. The other quantities are derived.
The form of the heat diffusion equation used here is almost the same
as that in equation 6 of "(Duffy)"_#Duffy, with the exception that the
electronic density is explicitly reprensented, rather than being part
of the the specific heat parameter.
of the specific heat parameter.
Currently, fix ttm assumes that none of the user-supplied parameters
will vary with temperature. Note that "(Duffy)"_#Duffy used a tanh()

View File

@ -48,6 +48,7 @@ Fixes :h1
fix_gld
fix_gle
fix_gravity
fix_grem
fix_halt
fix_heat
fix_imd

View File

@ -77,7 +77,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This improper style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -81,7 +81,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This improper style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -55,7 +55,7 @@ types.
[Restrictions:]
This improper style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other improper styles, the hybrid improper style does not store

View File

@ -27,7 +27,7 @@ between quadruplets of atoms, which remain in force for the duration
of the simulation. The list of improper quadruplets is read in by a
"read_data"_read_data.html or "read_restart"_read_restart.html command
from a data or restart file. Note that the ordering of the 4 atoms in
an improper quadruplet determines the the definition of the improper
an improper quadruplet determines the definition of the improper
angle used in the formula for each style. See the doc pages of
individual styles for details.

View File

@ -74,7 +74,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This improper style can only be used if LAMMPS was built with the
MOLECULE package (which it is by default). See the "Making
MOLECULE package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -14,7 +14,7 @@ info args :pre
args = one or more of the following keywords: {out}, {all}, {system}, {communication}, {computes}, {dumps}, {fixes}, {groups}, {regions}, {variables}, {styles}, {time}, or {configuration}
{out} values = {screen}, {log}, {append} filename, {overwrite} filename
{styles} values = {all}, {angle}, {atom}, {bond}, {compute}, {command}, {dump}, {dihedral}, {fix}, {improper}, {integrate}, {kspace}, {minimize}, {region} :ul
{styles} values = {all}, {angle}, {atom}, {bond}, {compute}, {command}, {dump}, {dihedral}, {fix}, {improper}, {integrate}, {kspace}, {minimize}, {pair}, {region} :ul
[Examples:]
@ -70,8 +70,9 @@ The {variables} category prints a list of all currently defined
variables, their names, styles, definition and last computed value, if
available.
The {styles} category prints the list of styles available in LAMMPS. It
supports one of the following options to control what is printed out:
The {styles} category prints the list of styles available in the
current LAMMPS binary. It supports one of the following options
to control which category of styles is printed out:
all
angle
@ -86,6 +87,7 @@ improper
integrate
kspace
minimize
pair
region :ul
The {time} category prints the accumulated CPU and wall time for the

View File

@ -59,6 +59,7 @@ dump_h5md.html
dump_image.html
dump_modify.html
dump_molfile.html
dump_nc.html
echo.html
fix.html
fix_modify.html
@ -152,6 +153,7 @@ fix_colvars.html
fix_controller.html
fix_deform.html
fix_deposit.html
fix_dpd_energy.html
fix_drag.html
fix_drude.html
fix_drude_transform.html
@ -170,6 +172,7 @@ fix_gcmc.html
fix_gld.html
fix_gle.html
fix_gravity.html
fix_grem.html
fix_halt.html
fix_heat.html
fix_imd.html
@ -272,6 +275,7 @@ fix_viscosity.html
fix_viscous.html
fix_wall.html
fix_wall_gran.html
fix_wall_gran_region.html
fix_wall_piston.html
fix_wall_reflect.html
fix_wall_region.html
@ -390,6 +394,7 @@ compute_voronoi_atom.html
compute_xrd.html
pair_adp.html
pair_agni.html
pair_airebo.html
pair_awpmd.html
pair_beck.html
@ -622,3 +627,4 @@ USER/atc/man_unfix_flux.html
USER/atc/man_unfix_nodes.html
USER/atc/man_write_atom_weights.html
USER/atc/man_write_restart.html

View File

@ -284,7 +284,7 @@ ID2 x2 y2 z2
...
IDN xN yN zN :pre
The fields are the the atom ID, followed by the x,y,z coordinates.
The fields are the atom ID, followed by the x,y,z coordinates.
The lines can be listed in any order. Additional trailing information
on the line is OK, such as a comment.

View File

@ -44,7 +44,7 @@ one value from their respective list of values. A {file}-style
variable reads the next line from its associated file. An
{atomfile}-style variable reads the next set of lines (one per atom)
from its associated file. {String-} or {atom}- or {equal}- or
{world}-style variables cannot be used with the the next command,
{world}-style variables cannot be used with the next command,
since they only store a single value.
When any of the variables in the next command has no more values, a

View File

@ -168,7 +168,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
This pair style is part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default).
if LAMMPS was built with that package.
[Related commands:]

128
doc/src/pair_agni.txt Normal file
View File

@ -0,0 +1,128 @@
"LAMMPS WWW Site"_lws - "LAMMPS Documentation"_ld - "LAMMPS Commands"_lc :c
:link(lws,http://lammps.sandia.gov)
:link(ld,Manual.html)
:link(lc,Section_commands.html#comm)
:line
pair_style agni command :h3
pair_style agni/omp command :h3
[Syntax:]
pair_style agni :pre
[Examples:]
pair_style agni
pair_coeff * * Al.agni Al
[Description:]
Style {agni} style computes the manybody vectorial force components for
an atom as
:c,image(Eqs/pair_agni.jpg)
{u} labels the individual components, i.e. x, y or z, and {V} is the
corresponding atomic fingerprint. {d} is the Euclidean distance between
any two atomic fingerprints. A total of N_t reference atomic
environments are considered to construct the force field file. {alpha_t}
and {l} are the weight coefficients and length scale parameter of the
non-linear regression model.
The method implements the recently proposed machine learning access to
atomic forces as discussed extensively in the following publications -
"(Botu1)"_#Botu2015adaptive and "(Botu2)"_#Botu2015learning. The premise
of the method is to map the atomic enviornment numerically into a
fingerprint, and use machine learning methods to create a mapping to the
vectorial atomic forces.
Only a single pair_coeff command is used with the {agni} style which
specifies an AGNI potential file containing the parameters of the
force field for the needed elements. These are mapped to LAMMPS atom
types by specifying N additional arguments after the filename in the
pair_coeff command, where N is the number of LAMMPS atom types:
filename
N element names = mapping of AGNI elements to atom types :ul
See the "pair_coeff"_pair_coeff.html doc page for alternate ways
to specify the path for the force field file.
An AGNI force field is fully specified by the filename which contains the
parameters of the force field, i.e., the reference training environments
used to construct the machine learning force field. Example force field
and input files are provided in the examples/USER/misc/agni directory.
:line
Styles with {omp} suffix is functionally the same as the corresponding
style without the suffix. They have been optimized to run faster, depending
on your available hardware, as discussed in "Section 5"_Section_accelerate.html
of the manual. The accelerated style takes the same arguments and
should produce the same results, except for round-off and precision
issues.
The accelerated style is part of the USER-OMP. They are only enabled if
LAMMPS was built with those packages. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info.
You can specify the accelerated style explicitly in your input script
by including their suffix, or you can use the "-suffix command-line
switch"_Section_start.html#start_7 when you invoke LAMMPS, or you can
use the "suffix"_suffix.html command in your input script.
See "Section 5"_Section_accelerate.html of the manual for
more instructions on how to use the accelerated styles effectively.
:line
[Mixing, shift, table, tail correction, restart, rRESPA info]:
This pair style does not support the "pair_modify"_pair_modify.html
shift, table, and tail options.
This pair style does not write its information to "binary restart
files"_restart.html, since it is stored in potential files. Thus, you
need to re-specify the pair_style and pair_coeff commands in an input
script that reads a restart file.
This pair style can only be used via the {pair} keyword of the
"run_style respa"_run_style.html command. It does not support the
{inner}, {middle}, {outer} keywords.
:line
[Restrictions:]
Currently, only elemental systems are implemented. Also, the method only
provides access to the forces and not energies or stresses. However, one
can access the energy via thermodynamic integration of the forces as
discussed in "(Botu3)"_#Botu2016construct. This pair style is part
of the USER-MISC package. It is only enabled if LAMMPS was built with
that package. See the "Making LAMMPS"_Section_start.html#start_3 section
for more info.
The AGNI force field files provided with LAMMPS (see the
potentials directory) are parameterized for metal "units"_units.html.
You can use the AGNI potential with any LAMMPS units, but you would need
to create your own AGNI potential file with coefficients listed in the
appropriate units if your simulation doesn't use "metal" units.
[Related commands:]
"pair_coeff"_pair_coeff.html
[Default:] none
:line
:link(Botu2015adaptive)
[(Botu1)] V. Botu and R. Ramprasad, Int. J. Quant. Chem., 115(16), 1074 (2015).
:link(Botu2015learning)
[(Botu2)] V. Botu and R. Ramprasad, Phys. Rev. B, 92(9), 094306 (2015).
:link(Botu2016construct)
[(Botu3)] V. Botu, R. Batra, J. Chapman and R. Ramprasad, https://arxiv.org/abs/1610.02098 (2016).

View File

@ -203,9 +203,8 @@ These pair styles can only be used via the {pair} keyword of the
[Restrictions:]
These pair styles are part of the MANYBODY package. They are only
enabled if LAMMPS was built with that package (which it is by
default). See the "Making LAMMPS"_Section_start.html#start_3 section
for more info.
enabled if LAMMPS was built with that package. See the
"Making LAMMPS"_Section_start.html#start_3 section for more info.
These pair potentials require the "newton"_newton.html setting to be
"on" for pair interactions.

View File

@ -382,7 +382,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
These pair styles are part of the MANYBODY package. They are only
enabled if LAMMPS was built with that package (which it is by default).
enabled if LAMMPS was built with that package.
See the "Making LAMMPS"_Section_start.html#start_3 section for more
info.

View File

@ -19,6 +19,8 @@ pair_style born/coul/msm/omp command :h3
pair_style born/coul/wolf command :h3
pair_style born/coul/wolf/gpu command :h3
pair_style born/coul/wolf/omp command :h3
pair_style born/coul/dsf command :h3
pair_style born/coul/dsf/cs command :h3
[Syntax:]
@ -37,7 +39,11 @@ args = list of arguments for a particular style :ul
{born/coul/wolf} args = alpha cutoff (cutoff2)
alpha = damping parameter (inverse distance units)
cutoff = global cutoff for non-Coulombic (and Coulombic if only 1 arg) (distance units)
cutoff2 = global cutoff for Coulombic (optional) (distance units) :pre
cutoff2 = global cutoff for Coulombic (optional) (distance units)
{born/coul/dsf} or {born/coul/dsf/cs} args = alpha cutoff (cutoff2)
alpha = damping parameter (inverse distance units)
cutoff = global cutoff for non-Coulombic (and Coulombic if only 1 arg) (distance units)
cutoff2 = global cutoff for Coulombic (distance units) :pre
[Examples:]
@ -62,6 +68,10 @@ pair_style born/coul/wolf 0.25 10.0 9.0
pair_coeff * * 6.08 0.317 2.340 24.18 11.51
pair_coeff 1 1 6.08 0.317 2.340 24.18 11.51 :pre
pair_style born/coul/dsf 0.1 10.0 12.0
pair_coeff * * 0.0 1.00 0.00 0.00 0.00
pair_coeff 1 1 480.0 0.25 0.00 1.05 0.50 :pre
[Description:]
The {born} style computes the Born-Mayer-Huggins or Tosi/Fumi
@ -90,10 +100,14 @@ term.
The {born/coul/wolf} style adds a Coulombic term as described for the
Wolf potential in the "coul/wolf"_pair_coul.html pair style.
The {born/coul/dsf} style computes the Coulomb contribution with the
damped shifted force model as in the "coul/dsf"_pair_coul.html style.
Style {born/coul/long/cs} is identical to {born/coul/long} except that
a term is added for the "core/shell model"_Section_howto.html#howto_25
to allow charges on core and shell particles to be separated by r =
0.0.
0.0. The same correction is introduced for {born/coul/dsf/cs} style
which is identical to {born/coul/dsf}.
Note that these potentials are related to the "Buckingham
potential"_pair_buck.html.
@ -116,9 +130,10 @@ The second coefficient, rho, must be greater than zero.
The last coefficient is optional. If not specified, the global A,C,D
cutoff specified in the pair_style command is used.
For {born/coul/long} and {born/coul/wolf} no Coulombic cutoff can be
specified for an individual I,J type pair. All type pairs use the
same global Coulombic cutoff specified in the pair_style command.
For {born/coul/long}, {born/coul/wolf} and {born/coul/dsf} no
Coulombic cutoff can be specified for an individual I,J type pair.
All type pairs use the same global Coulombic cutoff specified in the
pair_style command.
:line
@ -174,9 +189,8 @@ respa"_run_style.html command. They do not support the {inner},
[Restrictions:]
The {born/coul/long} style is part of the KSPACE package. It is only
enabled if LAMMPS was built with that package (which it is by
default). See the "Making LAMMPS"_Section_start.html#start_3 section
for more info.
enabled if LAMMPS was built with that package. See the
"Making LAMMPS"_Section_start.html#start_3 section for more info.
[Related commands:]

View File

@ -186,9 +186,8 @@ respa"_run_style.html command. They do not support the {inner},
The {buck/coul/long} style is part of the KSPACE package. The
{buck/coul/long/cs} style is part of the CORESHELL package. They are
only enabled if LAMMPS was built with that package (which it is by
default). See the "Making LAMMPS"_Section_start.html#start_3 section
for more info.
only enabled if LAMMPS was built with that package. See the
"Making LAMMPS"_Section_start.html#start_3 section for more info.
[Related commands:]

View File

@ -156,7 +156,7 @@ These pair styles can only be used via the {pair} keyword of the
[Restrictions:]
These pair styles are part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default). See
if LAMMPS was built with that package. See
the "Making LAMMPS"_Section_start.html#start_3 section for more info.
These pair styles requires the "newton"_newton.html setting to be "on"

View File

@ -313,9 +313,8 @@ This pair style can only be used via the {pair} keyword of the
The {coul/long}, {coul/msm} and {tip4p/long} styles are part of the
KSPACE package. The {coul/long/cs} style is part of the CORESHELL
package. They are only enabled if LAMMPS was built with that package
(which it is by default). See the "Making
LAMMPS"_Section_start.html#start_3 section for more info.
package. They are only enabled if LAMMPS was built with that package.
See the "Making LAMMPS"_Section_start.html#start_3 section for more info.
[Related commands:]

View File

@ -8,19 +8,24 @@
pair_style born/coul/long/cs command :h3
pair_style buck/coul/long/cs command :h3
pair_style born/coul/dsf/cs command :h3
[Syntax:]
pair_style style args :pre
style = {born/coul/long/cs} or {buck/coul/long/cs}
style = {born/coul/long/cs} or {buck/coul/long/cs} or {born/coul/dsf/cs}
args = list of arguments for a particular style :ul
{born/coul/long/cs} args = cutoff (cutoff2)
cutoff = global cutoff for non-Coulombic (and Coulombic if only 1 arg) (distance units)
cutoff2 = global cutoff for Coulombic (optional) (distance units)
{buck/coul/long/cs} args = cutoff (cutoff2)
cutoff = global cutoff for Buckingham (and Coulombic if only 1 arg) (distance units)
cutoff2 = global cutoff for Coulombic (optional) (distance units) :pre
cutoff2 = global cutoff for Coulombic (optional) (distance units)
{born/coul/dsf/cs} args = alpha cutoff (cutoff2)
alpha = damping parameter (inverse distance units)
cutoff = global cutoff for non-Coulombic (and Coulombic if only 1 arg) (distance units)
cutoff2 = global cutoff for Coulombic (distance units) :pre
[Examples:]
@ -32,6 +37,10 @@ pair_style buck/coul/long/cs 10.0 8.0
pair_coeff * * 100.0 1.5 200.0
pair_coeff 1 1 100.0 1.5 200.0 9.0 :pre
pair_style born/coul/dsf/cs 0.1 10.0 12.0
pair_coeff * * 0.0 1.00 0.00 0.00 0.00
pair_coeff 1 1 480.0 0.25 0.00 1.05 0.50 :pre
[Description:]
These pair styles are designed to be used with the adiabatic
@ -39,7 +48,7 @@ core/shell model of "(Mitchell and Finchham)"_#MitchellFinchham. See
"Section 6.25"_Section_howto.html#howto_25 of the manual for an
overview of the model as implemented in LAMMPS.
These pair styles are identical to the "pair_style
The styles with a {coul/long} term are identical to the "pair_style
born/coul/long"_pair_born.html and "pair_style
buck/coul/long"_pair_buck.html styles, except they correctly treat the
special case where the distance between two charged core and shell
@ -63,6 +72,14 @@ where C is an energy-conversion constant, Qi and Qj are the charges on
the core and shell, epsilon is the dielectric constant and r_min is the
minimal distance.
The pair style {born/coul/dsf/cs} is identical to the
"pair_style born/coul/dsf"_pair_born.html style, which uses the
the damped shifted force model as in "coul/dsf"_pair_coul.html
to compute the Coulomb contribution. This approach does not require
a long-range solver, thus the only correction is the addition of a
minimal distance to avoid the possible r = 0.0 case for a
core/shell pair.
[Restrictions:]
These pair styles are part of the CORESHELL package. They are only

View File

@ -412,9 +412,8 @@ The eam pair styles can only be used via the {pair} keyword of the
[Restrictions:]
All of these styles except the {eam/cd} style are part of the MANYBODY
package. They are only enabled if LAMMPS was built with that package
(which it is by default). See the "Making
LAMMPS"_Section_start.html#start_3 section for more info.
package. They are only enabled if LAMMPS was built with that package.
See the "Making LAMMPS"_Section_start.html#start_3 section for more info.
The {eam/cd} style is part of the USER-MISC package and also requires
the MANYBODY package. It is only enabled if LAMMPS was built with

View File

@ -159,7 +159,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This style is part of the MANYBODY package. It is only enabled if
LAMMPS was built with that package (which it is by default).
LAMMPS was built with that package.
[Related commands:]

View File

@ -72,7 +72,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
This pair styles is part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default). See
if LAMMPS was built with that package. See
the "Making LAMMPS"_Section_start.html#start_3 section for more info.
This pair potential requires the "newton"_newton.html setting to be

View File

@ -113,7 +113,7 @@ more instructions on how to use the accelerated styles effectively.
[Restrictions:]
This pair style can only be used if LAMMPS was built with the MANYBODY
package (which it is by default). See the "Making
package. See the "Making
LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]

View File

@ -191,7 +191,7 @@ input script. If using read_data, atomic masses must be defined in the
atomic structure data file.
This pair style is part of the MANYBODY package. It is only enabled if
LAMMPS was built with that package (which it is by default). See the
LAMMPS was built with that package. See the
"Making LAMMPS"_Section_start.html#start_3 section for more info.
This pair potential requires the "newtion"_newton.html setting to be

View File

@ -15,7 +15,7 @@ pair_style snap :pre
[Examples:]
pair_style snap
pair_coeff * * snap InP.snapcoeff In P InP.snapparam In In P P :pre
pair_coeff * * InP.snapcoeff In P InP.snapparam In In P P :pre
[Description:]
@ -27,9 +27,9 @@ it uses bispectrum components
to characterize the local neighborhood of each atom
in a very general way. The mathematical definition of the
bispectrum calculation used by SNAP is identical
to that used of "compute sna/atom"_compute_sna_atom.html.
to that used by "compute sna/atom"_compute_sna_atom.html.
In SNAP, the total energy is decomposed into a sum over
atom energies. The energy of atom {i} is
atom energies. The energy of atom {i } is
expressed as a weighted sum over bispectrum components.
:c,image(Eqs/pair_snap.jpg)
@ -183,8 +183,7 @@ LAMMPS"_Section_start.html#start_3 section for more info.
:line
:link(Thompson2014)
[(Thompson)] Thompson, Swiler, Trott, Foiles, Tucker, under review, preprint
available at "arXiv:1409.3880"_http://arxiv.org/abs/1409.3880
[(Thompson)] Thompson, Swiler, Trott, Foiles, Tucker, J Comp Phys, 285, 316 (2015).
:link(Bartok2010)
[(Bartok2010)] Bartok, Payne, Risi, Csanyi, Phys Rev Lett, 104, 136403 (2010).

View File

@ -99,7 +99,7 @@ The optional {exclude} keyword determines if forces are computed
between first neighbor (directly connected) bonds. For a setting of
{no}, first neighbor forces are computed; for {yes} they are not
computed. A setting of {no} cannot be used with the {min} option for
distance calculation because the the minimum distance between directly
distance calculation because the minimum distance between directly
connected bonds is zero.
Pair style {srp} turns off normalization of thermodynamic properties

View File

@ -192,7 +192,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
This pair style is part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default). See
if LAMMPS was built with that package. See
the "Making LAMMPS"_Section_start.html#start_3 section for more info.
This pair style requires the "newton"_newton.html setting to be "on"

View File

@ -222,7 +222,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
This pair style is part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default). See
if LAMMPS was built with that package. See
the "Making LAMMPS"_Section_start.html#start_3 section for more info.
This pair style requires the "newton"_newton.html setting to be "on"

View File

@ -7,32 +7,43 @@
:line
pair_style tersoff/mod command :h3
pair_style tersoff/mod/c command :h3
pair_style tersoff/mod/gpu command :h3
pair_style tersoff/mod/kk command :h3
pair_style tersoff/mod/omp command :h3
pair_style tersoff/mod/c/omp command :h3
[Syntax:]
pair_style tersoff/mod :pre
pair_style tersoff/mod/c :pre
[Examples:]
pair_style tersoff/mod
pair_coeff * * Si.tersoff.mod Si Si :pre
pair_style tersoff/mod/c
pair_coeff * * Si.tersoff.modc Si Si :pre
[Description:]
The {tersoff/mod} style computes a bond-order type interatomic
potential "(Kumagai)"_#Kumagai based on a 3-body Tersoff potential
"(Tersoff_1)"_#Tersoff_1, "(Tersoff_2)"_#Tersoff_2 with modified
cutoff function and angular-dependent term, giving the energy E of a
system of atoms as
The {tersoff/mod} and {tersoff/mod/c} styles computes a bond-order type
interatomic potential "(Kumagai)"_#Kumagai based on a 3-body Tersoff
potential "(Tersoff_1)"_#Tersoff_1, "(Tersoff_2)"_#Tersoff_2 with
modified cutoff function and angular-dependent term, giving the energy
E of a system of atoms as
:c,image(Eqs/pair_tersoff_mod.jpg)
where f_R is a two-body term and f_A includes three-body interactions.
The summations in the formula are over all neighbors J and K of atom I
within a cutoff distance = R + D.
The {tersoff/mod/c} style differs from {tersoff/mod} only in the
formulation of the V_ij term, where it contains an additional c0 term.
:c,image(Eqs/pair_tersoff_mod_c.jpg)
The modified cutoff function f_C proposed by "(Murty)"_#Murty and
having a continuous second-order differential is employed. The
@ -69,10 +80,11 @@ are placeholders for atom types that will be used with other
potentials.
Tersoff/MOD file in the {potentials} directory of the LAMMPS
distribution have a ".tersoff.mod" suffix. Lines that are not blank
or comments (starting with #) define parameters for a triplet of
elements. The parameters in a single entry correspond to coefficients
in the formula above:
distribution have a ".tersoff.mod" suffix. Potential files for the
{tersoff/mod/c} style have the suffix ".tersoff.modc". Lines that are
not blank or comments (starting with #) define parameters for a triplet
of elements. The parameters in a single entry correspond to
coefficients in the formulae above:
element 1 (the center atom in a 3-body interaction)
element 2 (the atom bonded to the center atom)
@ -93,13 +105,15 @@ c1
c2
c3
c4
c5 :ul
c5
c0 (energy units, tersoff/mod/c only):ul
The n, eta, lambda2, B, lambda1, and A parameters are only used for
two-body interactions. The beta, alpha, c1, c2, c3, c4, c5, h
parameters are only used for three-body interactions. The R and D
parameters are used for both two-body and three-body interactions. The
non-annotated parameters are unitless.
parameters are used for both two-body and three-body interactions.
The c0 term applies to {tersoff/mod/c} only. The non-annotated
parameters are unitless.
The Tersoff/MOD potential file must contain entries for all the elements
listed in the pair_coeff command. It can also contain entries for
@ -156,7 +170,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
This pair style is part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default). See
if LAMMPS was built with that package. See
the "Making LAMMPS"_Section_start.html#start_3 section for more info.
This pair style requires the "newton"_newton.html setting to be "on"

View File

@ -232,7 +232,7 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
This pair style is part of the MANYBODY package. It is only enabled
if LAMMPS was built with that package (which it is by default). See
if LAMMPS was built with that package. See
the "Making LAMMPS"_Section_start.html#start_3 section for more info.
This pair style requires the "newton"_newton.html setting to be "on"

View File

@ -8,6 +8,7 @@
pair_style vashishta command :h3
pair_style vashishta/omp command :h3
pair_style vashishta/kk command :h3
pair_style vashishta/table command :h3
pair_style vashishta/table/omp command :h3
@ -212,9 +213,8 @@ This pair style can only be used via the {pair} keyword of the
[Restrictions:]
These pair style are part of the MANYBODY package. They is only
enabled if LAMMPS was built with that package (which it is by
default). See the "Making LAMMPS"_Section_start.html#start_3 section
for more info.
enabled if LAMMPS was built with that package. See the
"Making LAMMPS"_Section_start.html#start_3 section for more info.
These pair styles requires the "newton"_newton.html setting to be "on"
for pair interactions.

View File

@ -6,6 +6,7 @@ Pair Styles :h1
:maxdepth: 1
pair_adp
pair_agni
pair_airebo
pair_awpmd
pair_beck

View File

@ -214,7 +214,7 @@ when a correlated event occurs during the third stage of the loop
listed above, i.e. when only one replica is running dynamics.
When more than one replica detects an event at the end of the same
event check (every {t_event} steps) during the the second stage, then
event check (every {t_event} steps) during the second stage, then
one of them is chosen at random. The number of coincident events is
the number of replicas that detected an event. Normally, this value
should be 1. If it is often greater than 1, then either the number of
@ -241,7 +241,7 @@ time was spent in each stage (dephasing, dynamics, quenching, etc).
Any "dump files"_dump.html defined in the input script, will be
written to during a PRD run at timesteps corresponding to both
uncorrelated and correlated events. This means the the requested dump
uncorrelated and correlated events. This means the requested dump
frequency in the "dump"_dump.html command is ignored. There will be
one dump file (per dump command) created for all partitions.

View File

@ -188,7 +188,7 @@ is assumed to have been previously loaded by another python command.
Note that the Python code that is loaded and run must contain a
function with the specified {func} name. To operate properly when
later invoked, the the function code must match the {input} and
later invoked, the function code must match the {input} and
{return} and {format} keywords specified by the python command.
Otherwise Python will generate an error.

View File

@ -185,7 +185,7 @@ For dump files in {xyz} format, only the {x}, {y}, and {z} fields are
supported. The dump file does not store atom IDs, so these are
assigned consecutively to the atoms as they appear in the dump file,
starting from 1. Thus you should insure that order of atoms is
consistent from snapshot to snapshot in the the XYZ dump file. See
consistent from snapshot to snapshot in the XYZ dump file. See
the "dump_modify sort"_dump_modify.html command if the XYZ dump file
was written by LAMMPS.
@ -195,7 +195,7 @@ velocities, or their respective plugins may not support reading of
velocities. The molfile dump files do not store atom IDs, so these
are assigned consecutively to the atoms as they appear in the dump
file, starting from 1. Thus you should insure that order of atoms are
consistent from snapshot to snapshot in the the molfile dump file.
consistent from snapshot to snapshot in the molfile dump file.
See the "dump_modify sort"_dump_modify.html command if the dump file
was written by LAMMPS.

View File

@ -94,6 +94,13 @@ Of course this is also possible by not using any suffix commands, and
explictly appending or not appending the suffix to the relevant
commands in your input script.
NOTE: The default "run_style"_run_style.html verlet is invoked prior to
reading the input script and is therefore not affected by a suffix command
in the input script. The KOKKOS package requires "run_style verlet/kk",
so when using the KOKKOS package it is necessary to either use the command
line "-sf kk" command or add an explicit "run_style verlet" command to the
input script.
[Restrictions:] none
[Related commands:]

View File

@ -231,7 +231,7 @@ time was spent in each stage (NEB, dynamics, quenching, etc).
Any "dump files"_dump.html defined in the input script will be written
to during a TAD run at timesteps when an event is executed. This
means the the requested dump frequency in the "dump"_dump.html command
means the requested dump frequency in the "dump"_dump.html command
is ignored. There will be one dump file (per dump command) created
for all partitions. The atom coordinates of the dump snapshot are
those of the minimum energy configuration resulting from quenching

109
doc/src/temper_grem.txt Normal file
View File

@ -0,0 +1,109 @@
"LAMMPS WWW Site"_lws - "LAMMPS Documentation"_ld - "LAMMPS Commands"_lc :c
:link(lws,http://lammps.sandia.gov)
:link(ld,Manual.html)
:link(lc,Section_commands.html#comm)
:line
temper/grem command :h3
[Syntax:]
temper/grem N M lambda fix-ID thermostat-ID seed1 seed2 index :pre
N = total # of timesteps to run
M = attempt a tempering swap every this many steps
lambda = initial lambda for this ensemble
fix-ID = ID of fix_grem
thermostat-ID = ID of the thermostat that controls kinetic temperature
seed1 = random # seed used to decide on adjacent temperature to partner with
seed2 = random # seed for Boltzmann factor in Metropolis swap
index = which temperature (0 to N-1) I am simulating (optional) :ul
[Examples:]
temper/grem 100000 1000 ${lambda} fxgREM fxnvt 0 58728
temper/grem 40000 100 ${lambda} fxgREM fxnpt 0 32285 ${walkers} :pre
[Description:]
Run a parallel tempering or replica exchange simulation in LAMMPS
partition mode using multiple generalized replicas (ensembles) of a
system defined by "fix grem"_fix_grem.html, which stands for the
generalized replica exchange method (gREM) originally developed by
"(Kim)"_#Kim. It uses non-Boltzmann ensembles to sample over first
order phase transitions. The is done by defining replicas with an
enthalpy dependent effective temperature
Two or more replicas must be used. See the "temper"_temper.html
command for an explanation of how to run replicas on multiple
partitions of one or more processors.
This command is a modification of the "temper"_temper.html command and
has the same dependencies, restraints, and input variables which are
discussed there in greater detail.
Instead of temperature, this command performs replica exchanges in
lambda as per the generalized ensemble enforced by "fix
grem"_fix_grem.html. The desired lambda is specified by {lambda},
which is typically a variable previously set in the input script, so
that each partition is assigned a different temperature. See the
"variable"_variable.html command for more details. For example:
variable lambda world 400 420 440 460
fix fxnvt all nvt temp 300.0 300.0 100.0
fix fxgREM all grem ${lambda} -0.05 -50000 fxnvt
temper 100000 100 ${lambda} fxgREM fxnvt 3847 58382 :pre
would define 4 lambdas with constant kinetic temperature but unique
generalized temperature, and assign one of them to "fix
grem"_fix_grem.html used by each replica, and to the grem command.
As the gREM simulation runs for {N} timesteps, a swap between adjacent
ensembles will be attempted every {M} timesteps. If {seed1} is 0,
then the swap attempts will alternate between odd and even pairings.
If {seed1} is non-zero then it is used as a seed in a random number
generator to randomly choose an odd or even pairing each time. Each
attempted swap of temperatures is either accepted or rejected based on
a Metropolis criterion, derived for gREM by "(Kim)"_#Kim, which uses
{seed2} in the random number generator.
File management works identical to the "temper"_temper.html command.
Dump files created by this fix contain continuous trajectories and
require post-processing to obtain per-replica information.
The last argument {index} in the grem command is optional and is used
when restarting a run from a set of restart files (one for each
replica) which had previously swapped to new lambda. This is done
using a variable. For example if the log file listed the following for
a simulation with 5 replicas:
500000 2 4 0 1 3 :pre
then a setting of
variable walkers world 2 4 0 1 3 :pre
would be used to restart the run with a grem command like the example
above with ${walkers} as the last argument. This functionality is
identical to "temper"_temper.html.
:line
[Restrictions:]
This command can only be used if LAMMPS was built with the USER-MISC
package. See the "Making LAMMPS"_Section_start.html#start_3 section
for more info on packages.
This command must be used with "fix grem"_fix_grem.html.
[Related commands:]
"fix grem"_fix_grem.html, "temper"_temper.html, "variable"_variable.html
[Default:] none
:link(Kim)
[(Kim)] Kim, Keyes, Straub, J Chem Phys, 132, 224107 (2010).

View File

@ -33,7 +33,7 @@ created by the surrounding particles. Drude oscillators represent
these dipoles by two fixed charges: the core (DC) and the Drude
particle (DP) bound by a harmonic potential. The Drude particle can be
thought of as the electron cloud whose center can be displaced from
the position of the the corresponding nucleus.
the position of the corresponding nucleus.
The sum of the masses of a core-Drude pair should be the mass of the
initial (unsplit) atom, \(m_C + m_D = m\). The sum of their charges

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