patch 11Aug17

Fixes for stable

.github/CONTRIBUTING.md

@@ -0,0 +1,112 @@
+# Contributing to LAMMPS via GitHub
+
+Thank your for considering to contribute to the LAMMPS software project.
+
+The following is a set of guidelines as well as explanations of policies and workflows for contributing to the LAMMPS molecular dynamics software project. These guidelines focus on submitting issues or pull requests on the LAMMPS GitHub project.
+
+Thus please also have a look at:
+* [The Section on submitting new features for inclusion in LAMMPS of the Manual](http://lammps.sandia.gov/doc/Section_modify.html#mod-15)
+* [The LAMMPS GitHub Tutorial in the Manual](http://lammps.sandia.gov/doc/tutorial_github.html)
+
+## Table of Contents
+
+[I don't want to read this whole thing, I just have a question!](#i-dont-want-to-read-this-whole-thing-i-just-have-a-question)
+
+[How Can I Contribute?](#how-can-i-contribute)
+* [Discussing How To Use LAMMPS](#discussing-how-to-use-lammps)
+* [Reporting Bugs](#reporting-bugs)
+* [Suggesting Enhancements](#suggesting-enhancements)
+* [Contributing Code](#contributing-code)
+
+[GitHub Workflows](#github-workflows)
+* [Issues](#issues)
+* [Pull Requests](#pull-requests)
+
+__
+
+## I don't want to read this whole thing I just have a question!
+
+> **Note:** Please do not file an issue to ask a general question about LAMMPS, its features, how to use specific commands, or how perform simulations or analysis in LAMMPS. Instead post your question to the ['lammps-users' mailing list](http://lammps.sandia.gov/mail.html). You do not need to be subscribed to post to the list (but a mailing list subscription avoids having your post delayed until it is approved by a mailing list moderator). Most posts to the mailing list receive a response within less than 24 hours. Before posting to the mailing list, please read the [mailing list guidelines](http://lammps.sandia.gov/guidelines.html). Following those guidelines will help greatly to get a helpful response. Always mention which LAMMPS version you are using.
+
+## How Can I Contribute?
+
+There are several ways how you can actively contribute to the LAMMPS project: you can discuss compiling and using LAMMPS, and solving LAMMPS related problems with other LAMMPS users on the lammps-users mailing list, you can report bugs or suggest enhancements by creating issues on GitHub (or posting them to the lammps-users mailing list), and you can contribute by submitting pull requests on GitHub or e-mail your code
+to one of the [LAMMPS core developers](http://lammps.sandia.gov/authors.html). As you may see from the aforementioned developer page, the LAMMPS software package includes the efforts of a very large number of contributors beyond the principal authors and maintainers.
+
+### Discussing How To Use LAMMPS
+
+The LAMMPS mailing list is hosted at SourceForge. The mailing list began in 2005, and now includes tens of thousands of messages in thousands of threads. LAMMPS developers try to respond to posted questions in a timely manner, but there are no guarantees. Please consider that people live in different timezone and may not have time to answer e-mails outside of their work hours.
+You can post to list by sending your email to lammps-users at lists.sourceforge.net (no subscription required), but before posting, please read the [mailing list guidelines](http://lammps.sandia.gov/guidelines.html) to maximize your chances to receive a helpful response.
+
+Anyone can browse/search previous questions/answers in the archives. You do not have to subscribe to the list to post questions, receive answers (to your questions), or browse/search the archives. You **do** need to subscribe to the list if you want emails for **all** the posts (as individual messages or in digest form), or to answer questions yourself. Feel free to sign up and help us out! Answering questions from fellow LAMMPS users is a great way to pay back the community for providing you a useful tool for free, and to pass on the advice you have received yourself to others. It improves your karma and helps you understand your own research better.
+
+If you post a message and you are a subscriber, your message will appear immediately. If you are not a subscriber, your message will be moderated, which typically takes one business day. Either way, when someone replies the reply will usually be sent to both, your personal email address and the mailing list. When replying to people, that responded to your post to the list, please always included the mailing list in your replies (i.e. use "Reply All" and **not** "Reply"). Responses will appear on the list in a few minutes, but it can take a few hours for postings and replies to show up in the SourceForge archive. Sending replies also to the mailing list is important, so that responses are archived and people with a similar issue can search for possible solutions in the mailing list archive.
+
+### Reporting Bugs
+
+While developers writing code for LAMMPS are careful to test their code, LAMMPS is such a large and complex software, that it is impossible to test for all combinations of features under all normal and not so normal circumstances. Thus bugs do happen, and if you suspect, that you have encountered one, please try to document it and report it as an [Issue](https://github.com/lammps/lammps/issues) on the LAMMPS GitHub project web page. However, before reporting a bug, you need to check whether this is something that may have already been corrected. The [Latest Features and Bug Fixes in LAMMPS](http://lammps.sandia.gov/bug.html) web page lists all significant changes to LAMMPS over the years. It also tells you what the current latest development version of LAMMPS is, and you should test whether your issue still applies to that version.
+
+When you click on the green "New Issue" button, you will be provided with a text field, where you can enter your message. That text field with contain a template with several headlines and some descriptions. Keep the headlines that are relevant to your reported potential bug and replace the descriptions with the information as suggested by the descriptions.
+You can also attach small text files (please add the file name extension `.txt` or it will be rejected), images, or small compressed text files (using gzip, do not use RAR or 7-ZIP or similar tools that are uncommon outside of Windows machines). In many cases, bugs are best illustrated by providing a small input deck (do **not** attach your entire production input, but remove everything that is not required to reproduce the issue, and scale down your system size, that the resulting calculation runs fast and can be run on small desktop quickly).
+
+To be able to submit an issue on GitHub, you have to register for an account (for GitHub in general). If you do not want to do that, or have other reservations against submitting an issue there, you can - as an alternative and in decreasing preference - either send an e-mail to the lammps-users mailing list, the original authors of the feature that you suspect to be affected, or one or more of the core LAMMPS developers.
+
+### Suggesting Enhancements
+
+The LAMMPS developers welcome suggestions for enhancements or new features. These should be submitted using the [GitHub Issue Tracker](https://github.com/lammps/lammps/issues) of the LAMMPS project. This is particularly recommended, when you plan to implement the feature or enhancement yourself, as this allows to coordinate in case there are other similar or conflicting ongoing developments.
+The LAMMPS developers will review your submission and consider implementing it. Whether this will actually happen depends on many factors: how difficult it would be, how much effort it would take, how many users would benefit from it, how well the individual developer would understand the underlying physics of the feature, and whether this is a feature that would fit into a software like LAMMPS, or would be better implemented as a separate tool. Because of these factors, it matters how well the suggested enhancement is formulated and the overall benefit is argued convincingly.
+
+To be able to submit an issue on GitHub, you have to register for an account (for GitHub in general). If you do not want to do that, or have other reservations against submitting an issue there, you can - as an alternative - send an e-mail to the lammps-users mailing list.
+
+### Contributing Code
+
+We encourage users to submit new features or modifications for LAMMPS to the core developers so they can be added to the LAMMPS distribution. The preferred way to manage and coordinate this is by submitting a pull request at the LAMMPS project on GitHub. For any larger modifications or programming project, you are encouraged to contact the LAMMPS developers ahead of time, in order to discuss implementation strategies and coding guidelines, that will make it easier to integrate your contribution and result in less work for everybody involved. You are also encouraged to search through the list of open issues on GitHub and submit a new issue for a planned feature, so you would not duplicate the work of others (and possibly get scooped by them) or have your work duplicated by others.
+
+How quickly your contribution will be integrated depends largely on how much effort it will cause to integrate and test it, how much it requires changes to the core code base, and of how much interest it is to the larger LAMMPS community. Please see below for a checklist of typical requirements. Once you have prepared everything, see [this tutorial](http://lammps.sandia.gov/doc/tutorial_github.html)
+ for instructions on how to submit your changes or new files through a GitHub pull request
+
+Here is a checklist of steps you need to follow to submit a single file or user package for our consideration. Following these steps will save both you and us time. See existing files in packages in the source directory for examples. If you are uncertain, please ask on the lammps-users mailing list.
+
+* All source files you provide must compile with the most current version of LAMMPS with multiple configurations. In particular you need to test compiling LAMMPS from scratch with `-DLAMMPS_BIGBIG` set in addition to the default `-DLAMMPS_SMALLBIG` setting. Your code will need to work correctly in serial and in parallel using MPI.
+* For consistency with the rest of LAMMPS and especially, if you want your contribution(s) to be added to main LAMMPS code or one of its standard packages, it needs to be written in a style compatible with other LAMMPS source files. This means: 2-character indentation per level, no tabs, no lines over 80 characters. I/O is done via the C-style stdio library, class header files should not import any system headers outside <stdio.h>, STL containers should be avoided in headers, and forward declarations used where possible or needed. All added code should be placed into the LAMMPS_NS namespace or a sub-namespace; global or static variables should be avoided, as they conflict with the modular nature of LAMMPS and the C++ class structure. Header files must not import namespaces with using. This all is so the developers can more easily understand, integrate, and maintain your contribution and reduce conflicts with other parts of LAMMPS. This basically means that the code accesses data structures, performs its operations, and is formatted similar to other LAMMPS source files, including the use of the error class for error and warning messages.
+* If you want your contribution to be added as a user-contributed feature, and it is a single file (actually a `<name>.cpp` and `<name>.h` file) it can be rapidly added to the USER-MISC directory. Include the one-line entry to add to the USER-MISC/README file in that directory, along with the 2 source files. You can do this multiple times if you wish to contribute several individual features.
+* If you want your contribution to be added as a user-contribution and it is several related features, it is probably best to make it a user package directory with a name like USER-FOO. In addition to your new files, the directory should contain a README text file. The README should contain your name and contact information and a brief description of what your new package does. If your files depend on other LAMMPS style files also being installed (e.g. because your file is a derived class from the other LAMMPS class), then an Install.sh file is also needed to check for those dependencies. See other README and Install.sh files in other USER directories as examples. Send us a tarball of this USER-FOO directory.
+* Your new source files need to have the LAMMPS copyright, GPL notice, and your name and email address at the top, like other user-contributed LAMMPS source files. They need to create a class that is inside the LAMMPS namespace. If the file is for one of the USER packages, including USER-MISC, then we are not as picky about the coding style (see above). I.e. the files do not need to be in the same stylistic format and syntax as other LAMMPS files, though that would be nice for developers as well as users who try to read your code.
+* You **must** also create or extend a documentation file for each new command or style you are adding to LAMMPS. For simplicity and convenience, the documentation of groups of closely related commands or styles may be combined into a single file. This will be one file for a single-file feature. For a package, it might be several files. These are simple text files with a specific markup language, that are then auto-converted to HTML and PDF. The tools for this conversion are included in the source distribution, and the translation can be as simple as doing "make html pdf" in the doc folder. Thus the documentation source files must be in the same format and style as other `<name>.txt` files in the lammps/doc/src directory for similar commands and styles; use one or more of them as a starting point. A description of the markup can also be found in `lammps/doc/utils/txt2html/README.html` As appropriate, the text files can include links to equations (see doc/Eqs/*.tex for examples, we auto-create the associated JPG files), or figures (see doc/JPG for examples), or even additional PDF files with further details (see doc/PDF for examples). The doc page should also include literature citations as appropriate; see the bottom of doc/fix_nh.txt for examples and the earlier part of the same file for how to format the cite itself. The "Restrictions" section of the doc page should indicate that your command is only available if LAMMPS is built with the appropriate USER-MISC or USER-FOO package. See other user package doc files for examples of how to do this. The prerequisite for building the HTML format files are Python 3.x and virtualenv, the requirement for generating the PDF format manual is the htmldoc software. Please run at least "make html" and carefully inspect and proofread the resulting HTML format doc page before submitting your code.
+* For a new package (or even a single command) you should include one or more example scripts demonstrating its use. These should run in no more than a couple minutes, even on a single processor, and not require large data files as input. See directories under examples/USER for examples of input scripts other users provided for their packages. These example inputs are also required for validating memory accesses and testing for memory leaks with valgrind
+* If there is a paper of yours describing your feature (either the algorithm/science behind the feature itself, or its initial usage, or its implementation in LAMMPS), you can add the citation to the *.cpp source file. See src/USER-EFF/atom_vec_electron.cpp for an example. A LaTeX citation is stored in a variable at the top of the file and a single line of code that references the variable is added to the constructor of the class. Whenever a user invokes your feature from their input script, this will cause LAMMPS to output the citation to a log.cite file and prompt the user to examine the file. Note that you should only use this for a paper you or your group authored. E.g. adding a cite in the code for a paper by Nose and Hoover if you write a fix that implements their integrator is not the intended usage. That kind of citation should just be in the doc page you provide.
+
+Finally, as a general rule-of-thumb, the more clear and self-explanatory you make your documentation and README files, and the easier you make it for people to get started, e.g. by providing example scripts, the more likely it is that users will try out your new feature.
+
+If the new features/files are broadly useful we may add them as core files to LAMMPS or as part of a standard package. Else we will add them as a user-contributed file or package. Examples of user packages are in src sub-directories that start with USER. The USER-MISC package is simply a collection of (mostly) unrelated single files, which is the simplest way to have your contribution quickly added to the LAMMPS distribution. You can see a list of the both standard and user packages by typing "make package" in the LAMMPS src directory.
+
+Note that by providing us files to release, you are agreeing to make them open-source, i.e. we can release them under the terms of the GPL, used as a license for the rest of LAMMPS. See Section 1.4 for details.
+
+With user packages and files, all we are really providing (aside from the fame and fortune that accompanies having your name in the source code and on the Authors page of the LAMMPS WWW site), is a means for you to distribute your work to the LAMMPS user community, and a mechanism for others to easily try out your new feature. This may help you find bugs or make contact with new collaborators. Note that you are also implicitly agreeing to support your code which means answer questions, fix bugs, and maintain it if LAMMPS changes in some way that breaks it (an unusual event).
+
+To be able to submit an issue on GitHub, you have to register for an account (for GitHub in general). If you do not want to do that, or have other reservations or difficulties to submit a pull request, you can - as an alternative - contact one or more of the core LAMMPS developers and ask if one of them would be interested in manually merging your code into LAMMPS and send them your source code. Since the effort to merge a pull request is a small fraction of the effort of integrating source code manually (which would usually be done by converting the contribution into a pull request), your chances to have your new code included quickly are the best with a pull request.
+
+If you prefer to submit patches or full files, you should first make certain, that your code works correctly with the latest patch-level version of LAMMPS and contains all bug fixes from it. Then create a gzipped tar file of all changed or added files or a corresponding patch file using 'diff -u' or 'diff -c' and compress it with gzip. Please only use gzip compression, as this works well on all platforms.
+
+## GitHub Workflows
+
+This section briefly summarizes the steps that will happen **after** you have submitted either an issue or a pull request on the LAMMPS GitHub project page. 
+
+### Issues
+
+After submitting an issue, one or more of the LAMMPS developers will review it and categorize it by assigning labels. Confirmed bug reports will be labeled `bug`; if the bug report also contains a suggestion for how to fix it, it will be labeled `bugfix`; if the issue is a feature request, it will be labeled `enhancement`. Other labels may be attached as well, depending on which parts of the LAMMPS code are affected. If the assessment is, that the issue does not warrant any changes, the `wontfix` label will be applied and if the submission is incorrect or something that should not be submitted as an issue, the `invalid` label will be applied. In both of the last two cases, the issue will then be closed without further action.
+
+For feature requests, what happens next is that developers may comment on the viability or relevance of the request, discuss and make suggestions for how to implement it. If a LAMMPS developer or user is planning to implement the feature, the issue will be assigned to that developer. For developers, that are not yet listed as LAMMPS project collaborators, they will receive an invitation to be added to the LAMMPS project as a collaborator so they can get assigned. If the requested feature or enhancement is implemented, it will usually be submitted as a pull request, which will contain a reference to the issue number. And once the pull request is reviewed and accepted for inclusion into LAMMPS, the issue will be closed. For details on how pull requests are processed, please see below.
+
+For bug reports, the next step is that one of the core LAMMPS developers will self-assign to the issue and try to confirm the bug. If confirmed, the `bug` label and potentially other labels are added to classify the issue and its impact to LAMMPS. Before confirming, further questions may be asked or requests for providing additional input files or details about the steps required to reproduce the issue. Any bugfix is likely to be submitted as a pull request (more about that below) and since most bugs require only local changes, the bugfix may be included in a pull request specifically set up to collect such local bugfixes or small enhancements. Once the bugfix is included in the master branch, the issue will be closed.
+
+### Pull Requests
+
+For submitting pull requests, there is a [detailed tutorial](http://lammps.sandia.gov/doc/tutorial_github.html) in the LAMMPS manual. Thus only a brief breakdown of the steps is presented here.
+Immediately after the submission, the LAMMPS continuing integration server at ci.lammps.org will download your submitted branch and perform a simple compilation test, i.e. will test whether your submitted code can be compiled under various conditions. It will also do a check on whether your included documentation translates cleanly. Whether these tests are successful or fail will be recorded. If a test fails, please inspect the corresponding output on the CI server and take the necessary steps, if needed, so that the code can compile cleanly again. The test will be re-run each the pull request is updated with a push to the remote branch on GitHub.
+Next a LAMMPS core developer will self-assign and do an overall technical assessment of the submission. If you are not yet registered as a LAMMPS collaborator, you will receive an invitation for that.
+You may also receive comments and suggestions on the overall submission or specific details. If permitted, additional changes may be pushed into your pull request branch or a pull request may be filed in your LAMMPS fork on GitHub to include those changes.
+The LAMMPS developer may then decide to assign the pull request to another developer (e.g. when that developer is more knowledgeable about the submitted feature or enhancement or has written the modified code). It may also happen, that additional developers are requested to provide a review and approve the changes. For submissions, that may change the general behavior of LAMMPS, or where a possibility of unwanted side effects exists, additional tests may be requested by the assigned developer.
+If the assigned developer is satisfied and considers the submission ready for inclusion into LAMMPS, the pull request will be assigned to the LAMMPS lead developer, Steve Plimpton (@sjplimp), who will then have the final decision on whether the submission will be included, additional changes are required or it will be ultimately rejected. After the pull request is merged, you may delete the pull request branch in your personal LAMMPS fork.
+Since the learning curve for git is quite steep for efficiently managing remote repositories, local and remote branches, pull requests and more, do not hesitate to ask questions, if you are not sure about how to do certain steps that are asked of you. Even if the changes asked of you do not make sense to you, they may be important for the LAMMPS developers. Please also note, that these all are guidelines and not set in stone.
+

.github/ISSUE_TEMPLATE.md

@@ -0,0 +1,31 @@
+## Summary
+
+_Please provide a brief description of the issue_
+
+## Type of Issue
+
+_Is this a 'Bug Report' or a 'Suggestion for an Enhancement'?_
+
+## Detailed Description (Enhancement Suggestion)
+
+_Explain how you would like to see LAMMPS enhanced, what feature(s) you are looking for, provide references to relevant background information, and whether you are willing to implement the enhancement yourself or would like to participate in the implementation_
+
+## LAMMPS Version (Bug Report)
+
+_Please specify which LAMMPS version this issue was detected with. If this is not the latest development version, please stop and test that version, too, and report it here if the bug persists_
+
+## Expected Behavior (Bug Report)
+
+_Describe the expected behavior. Quote from the LAMMPS manual where needed or explain why the expected behavior is meaningful, especially when it differs from the manual_
+
+## Actual Behavior (Bug Report)
+
+_Describe the actual behavior, how it differs from the expected behavior, and how this can be observed. Try to be specific and do **not* use vague terms like "doesn't work" or "wrong result". Do not assume that the person reading this has any experience with or knowledge of your specific research._
+
+## Steps to Reproduce (Bug Report)
+
+_Describe the steps required to quickly reproduce the issue. You can attach (small) files to the section below or add URLs where to download an archive with all necessary files. Please try to create input that are as small as possible and run as fast as possible. NOTE: the less effort and time it takes to reproduce your issue, the more likely, that somebody will look into it._
+
+## Further Information, Files, and Links
+
+_Put any additional information here, attach relevant text or image files and URLs to external sites, e.g. relevant publications_

.github/PULL_REQUEST_TEMPLATE.md

@@ -0,0 +1,29 @@
+## Purpose
+
+_Briefly describe the new feature(s), enhancement(s), or bugfix(es) included in this pull request. If this addresses an open GitHub Issue, mention the issue number, e.g. with `fixes #221` or `closes #135`, so that issue will be automatically closed when the pull request is merged_
+
+## Author(s)
+
+_Please state name and affiliation of the author or authors that should be credited with the changes in this pull request_
+
+## Backward Compatibility
+
+_Please state whether any changes in the pull request break backward compatibility for inputs, and - if yes - explain what has been changed and why_
+
+## Implementation Notes
+
+_Provide any relevant details about how the changes are implemented, how correctness was verified, how other features - if any - in LAMMPS are affected_
+
+## Post Submission Checklist
+
+_Please check the fields below as they are completed_
+- [ ] The feature or features in this pull request is complete
+- [ ] Suitable new documentation files and/or updates to the existing docs are included
+- [ ] One or more example input decks are included
+- [ ] The source code follows the LAMMPS formatting guidelines
+
+## Further Information, Files, and Links
+
+_Put any additional information here, attach relevant text or image files, and URLs to external sites (e.g. DOIs or webpages)_
+
+

LICENSE

@@ -3,7 +3,7 @@ GNU GENERAL PUBLIC LICENSE
 Version 2, June 1991 
 
 Copyright (C) 1989, 1991 Free Software Foundation, Inc.  
-59 Temple Place - Suite 330, Boston, MA  02111-1307, USA
+51 Franklin Street, Fifth Floor, Boston, MA  02110-1301, USA
 
 Everyone is permitted to copy and distribute verbatim copies of this
 license document, but changing it is not allowed.

bench/FERMI/README

@@ -1,55 +1,21 @@
 These are input scripts used to run versions of several of the
-benchmarks in the top-level bench directory using the GPU and
-USER-CUDA accelerator packages.  The results of running these scripts
-on two different machines (a desktop with 2 Tesla GPUs and the ORNL
-Titan supercomputer) are shown on the "GPU (Fermi)" section of the
-Benchmark page of the LAMMPS WWW site: lammps.sandia.gov/bench.
+benchmarks in the top-level bench directory using the GPU accelerator
+package.  The results of running these scripts on two different machines
+(a desktop with 2 Tesla GPUs and the ORNL Titan supercomputer) are shown
+on the "GPU (Fermi)" section of the Benchmark page of the LAMMPS WWW
+site: lammps.sandia.gov/bench.
 
 Examples are shown below of how to run these scripts.  This assumes
-you have built 3 executables with both the GPU and USER-CUDA packages
+you have built 3 executables with the GPU package
 installed, e.g.
 
 lmp_linux_single
 lmp_linux_mixed
 lmp_linux_double
 
-The precision (single, mixed, double) refers to the GPU and USER-CUDA
-pacakge precision.  See the README files in the lib/gpu and lib/cuda
-directories for instructions on how to build the packages with
-different precisions.  The GPU and USER-CUDA sub-sections of the
-doc/Section_accelerate.html file also describes this process.
-
-Make.py -d ~/lammps -j 16 -p #all orig -m linux -o cpu -a exe
-Make.py -d ~/lammps -j 16 -p #all opt orig -m linux -o opt -a exe
-Make.py -d ~/lammps -j 16 -p #all omp orig -m linux -o omp -a exe
-Make.py -d ~/lammps -j 16 -p #all gpu orig -m linux \
-        -gpu mode=double arch=20 -o gpu_double -a libs exe
-Make.py -d ~/lammps -j 16 -p #all gpu orig -m linux \
-        -gpu mode=mixed arch=20 -o gpu_mixed -a libs exe
-Make.py -d ~/lammps -j 16 -p #all gpu orig -m linux \
-        -gpu mode=single arch=20 -o gpu_single -a libs exe
-Make.py -d ~/lammps -j 16 -p #all cuda orig -m linux \
-        -cuda mode=double arch=20 -o cuda_double -a libs exe
-Make.py -d ~/lammps -j 16 -p #all cuda orig -m linux \
-        -cuda mode=mixed arch=20 -o cuda_mixed -a libs exe
-Make.py -d ~/lammps -j 16 -p #all cuda orig -m linux \
-        -cuda mode=single arch=20 -o cuda_single -a libs exe
-Make.py -d ~/lammps -j 16 -p #all intel orig -m linux -o intel_cpu -a exe
-Make.py -d ~/lammps -j 16 -p #all kokkos orig -m linux -o kokkos_omp -a exe
-Make.py -d ~/lammps -j 16 -p #all kokkos orig -kokkos cuda arch=20 \
-        -m cuda -o kokkos_cuda -a exe
-
-Make.py -d ~/lammps -j 16 -p #all opt omp gpu cuda intel kokkos orig \
-        -gpu mode=double arch=20 -cuda mode=double arch=20 -m linux \
-        -o all -a libs exe
-
-Make.py -d ~/lammps -j 16 -p #all opt omp gpu cuda intel kokkos orig \
-        -kokkos cuda arch=20 -gpu mode=double arch=20 \
-        -cuda mode=double arch=20 -m cuda -o all_cuda -a libs exe
-
 ------------------------------------------------------------------------
 
-To run on just CPUs (without using the GPU or USER-CUDA styles),
+To run on just CPUs (without using the GPU styles),
 do something like the following:
 
 mpirun -np 1 lmp_linux_double -v x 8 -v y 8 -v z 8 -v t 100 < in.lj
@@ -81,23 +47,5 @@ node via a "-ppn" setting.
 
 ------------------------------------------------------------------------
 
-To run with the USER-CUDA package, do something like the following:
-
-mpirun -np 1 lmp_linux_single -c on -sf cuda -v x 16 -v y 16 -v z 16 -v t 100 < in.lj
-mpirun -np 2 lmp_linux_double -c on -sf cuda -pk cuda 2 -v x 32 -v y 64 -v z 64 -v t 100 < in.eam
-
-The "xyz" settings determine the problem size.  The "t" setting
-determines the number of timesteps.  The "np" setting determines how
-many MPI tasks (per node) the problem will run on.  The numeric
-argument to the "-pk" setting is the number of GPUs (per node); 1 GPU
-is the default.  Note that the number of MPI tasks must equal the
-number of GPUs (both per node) with the USER-CUDA package.
-
-These mpirun commands run on a single node.  To run on multiple nodes,
-scale up the "-np" setting, and control the number of MPI tasks per
-node via a "-ppn" setting.
-
-------------------------------------------------------------------------
-
 If the script has "titan" in its name, it was run on the Titan
 supercomputer at ORNL.

bench/README

@@ -71,49 +71,33 @@ integration
 
 ----------------------------------------------------------------------
 
-Here is a src/Make.py command which will perform a parallel build of a
-LAMMPS executable "lmp_mpi" with all the packages needed by all the
-examples.  This assumes you have an MPI installed on your machine so
-that "mpicxx" can be used as the wrapper compiler.  It also assumes
-you have an Intel compiler to use as the base compiler.  You can leave
-off the "-cc mpi wrap=icc" switch if that is not the case.  You can
-also leave off the "-fft fftw3" switch if you do not have the FFTW
-(v3) installed as an FFT package, in which case the default KISS FFT
-library will be used.
-
-cd src
-Make.py -j 16 -p none molecule manybody kspace granular rigid orig \
-  -cc mpi wrap=icc -fft fftw3 -a file mpi
-
-----------------------------------------------------------------------
-
 Here is how to run each problem, assuming the LAMMPS executable is
 named lmp_mpi, and you are using the mpirun command to launch parallel
 runs:
 
 Serial (one processor runs):
 
-lmp_mpi < in.lj
-lmp_mpi < in.chain
-lmp_mpi < in.eam
-lmp_mpi < in.chute
-lmp_mpi < in.rhodo
+lmp_mpi -in in.lj
+lmp_mpi -in in.chain
+lmp_mpi -in in.eam
+lmp_mpi -in in.chute
+lmp_mpi -in in.rhodo
 
 Parallel fixed-size runs (on 8 procs in this case):
 
-mpirun -np 8 lmp_mpi < in.lj
-mpirun -np 8 lmp_mpi < in.chain
-mpirun -np 8 lmp_mpi < in.eam
-mpirun -np 8 lmp_mpi < in.chute
-mpirun -np 8 lmp_mpi < in.rhodo
+mpirun -np 8 lmp_mpi -in in.lj
+mpirun -np 8 lmp_mpi -in in.chain
+mpirun -np 8 lmp_mpi -in in.eam
+mpirun -np 8 lmp_mpi -in in.chute
+mpirun -np 8 lmp_mpi -in in.rhodo
 
 Parallel scaled-size runs (on 16 procs in this case):
 
-mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 < in.lj
-mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 < in.chain.scaled
-mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 < in.eam
-mpirun -np 16 lmp_mpi -var x 4 -var y 4 < in.chute.scaled
-mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 < in.rhodo.scaled
+mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 -in in.lj
+mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 -in in.chain.scaled
+mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 -in in.eam
+mpirun -np 16 lmp_mpi -var x 4 -var y 4 -in in.chute.scaled
+mpirun -np 16 lmp_mpi -var x 2 -var y 2 -var z 4 -in in.rhodo.scaled
 
 For each of the scaled-size runs you must set 3 variables as -var
 command line switches.  The variables x,y,z are used in the input

doc/.gitignore

@@ -1 +1,6 @@
 /html
+/spelling
+/LAMMPS.epub
+/LAMMPS.mobi
+/Manual.pdf
+/Developer.pdf

doc/Makefile

@@ -6,21 +6,24 @@ BUILDDIR      = /tmp/lammps-docs-$(SHA1)
 RSTDIR        = $(BUILDDIR)/rst
 VENV          = $(BUILDDIR)/docenv
 TXT2RST       = $(VENV)/bin/txt2rst
+ANCHORCHECK   = $(VENV)/bin/doc_anchor_check
 
 PYTHON        = $(shell which python3)
+HAS_PYTHON3    = NO
+HAS_VIRTUALENV = NO
 
-ifeq ($(shell which python3 >/dev/null 2>&1; echo $$?), 1)
-$(error Python3 was not found! Please check README.md for further instructions)
+ifeq ($(shell which python3 >/dev/null 2>&1; echo $$?), 0)
+HAS_PYTHON3 = YES
 endif
 
-ifeq ($(shell which virtualenv >/dev/null 2>&1; echo $$?), 1)
-$(error virtualenv was not found! Please check README.md for further instructions)
+ifeq ($(shell which virtualenv >/dev/null 2>&1; echo $$?), 0)
+HAS_VIRTUALENV = YES
 endif
 
 SOURCES=$(wildcard src/*.txt)
 OBJECTS=$(SOURCES:src/%.txt=$(RSTDIR)/%.rst)
 
-.PHONY: help clean-all clean html pdf old venv
+.PHONY: help clean-all clean epub html pdf old venv spelling anchor_check
 
 # ------------------------------------------
 
@@ -30,9 +33,11 @@ help:
 	@echo "  pdf        create Manual.pdf and Developer.pdf in this dir"
 	@echo "  old        create old-style HTML doc pages in old dir"
 	@echo "  fetch      fetch HTML and PDF files from LAMMPS web site"
+	@echo "  epub       create ePUB format manual for e-book readers"
 	@echo "  clean      remove all intermediate RST files"
 	@echo "  clean-all  reset the entire build environment"
 	@echo "  txt2html   build txt2html tool"
+	@echo "  anchor_check  scan for duplicate anchor labels"
 
 # ------------------------------------------
 
@@ -40,13 +45,20 @@ clean-all:
 	rm -rf $(BUILDDIR)/* utils/txt2html/txt2html.exe
 
 clean:
-	rm -rf $(RSTDIR)
+	rm -rf $(RSTDIR) html
+	rm -rf spelling
 
-html: $(OBJECTS)
+clean-spelling:
+	rm -rf spelling
+
+html: $(OBJECTS) $(ANCHORCHECK)
 	@(\
 		. $(VENV)/bin/activate ;\
 		cp -r src/* $(RSTDIR)/ ;\
 		sphinx-build -j 8 -b html -c utils/sphinx-config -d $(BUILDDIR)/doctrees $(RSTDIR) html ;\
+		echo "############################################" ;\
+		doc_anchor_check src/*.txt ;\
+		echo "############################################" ;\
 		deactivate ;\
 	)
 	-rm html/searchindex.js
@@ -61,8 +73,34 @@ html: $(OBJECTS)
 	@rm -rf html/USER/*/*.[sg]*
 	@echo "Build finished. The HTML pages are in doc/html."
 
+spelling: $(OBJECTS) utils/sphinx-config/false_positives.txt
+	@(\
+		. $(VENV)/bin/activate ;\
+		pip install sphinxcontrib-spelling ;\
+		cp -r src/* $(RSTDIR)/ ;\
+        cp utils/sphinx-config/false_positives.txt $(RSTDIR)/ ;\
+		sphinx-build -b spelling -c utils/sphinx-config -d $(BUILDDIR)/doctrees $(RSTDIR) spelling ;\
+		deactivate ;\
+	)
+	@echo "Spell check finished."
+
+epub: $(OBJECTS)
+	@mkdir -p epub
+	@rm -f LAMMPS.epub
+	@cp src/JPG/lammps-logo.png epub/
+	@(\
+		. $(VENV)/bin/activate ;\
+		cp -r src/* $(RSTDIR)/ ;\
+		sphinx-build -j 8 -b epub -c utils/sphinx-config -d $(BUILDDIR)/doctrees $(RSTDIR) epub ;\
+		deactivate ;\
+	)
+	@mv  epub/LAMMPS.epub .
+	@rm -rf epub
+	@echo "Build finished. The ePUB manual file is created."
+
 pdf: utils/txt2html/txt2html.exe
 	@(\
+		set -e; \
 		cd src; \
 		../utils/txt2html/txt2html.exe -b *.txt; \
 		htmldoc --batch lammps.book;          \
@@ -95,6 +133,13 @@ fetch:
 
 txt2html: utils/txt2html/txt2html.exe
 
+anchor_check : $(ANCHORCHECK)
+	@(\
+		. $(VENV)/bin/activate ;\
+		doc_anchor_check src/*.txt ;\
+		deactivate ;\
+	)
+
 # ------------------------------------------
 
 utils/txt2html/txt2html.exe: utils/txt2html/txt2html.cpp
@@ -109,15 +154,17 @@ $(RSTDIR)/%.rst : src/%.txt $(TXT2RST)
 	)
 
 $(VENV):
+	@if [ "$(HAS_PYTHON3)" == "NO" ] ; then echo "Python3 was not found! Please check README.md for further instructions" 1>&2; exit 1; fi
+	@if [ "$(HAS_VIRTUALENV)" == "NO" ] ; then echo "virtualenv was not found! Please check README.md for further instructions" 1>&2; exit 1; fi
 	@( \
 		virtualenv -p $(PYTHON) $(VENV); \
 		. $(VENV)/bin/activate; \
-		pip install Sphinx; \
+		pip install Sphinx==1.5.6; \
 		pip install sphinxcontrib-images; \
 		deactivate;\
 	)
 
-$(TXT2RST): $(VENV)
+$(TXT2RST) $(ANCHORCHECK): $(VENV)
 	@( \
 		. $(VENV)/bin/activate; \
 		(cd utils/converters;\

doc/README

@@ -1,13 +1,14 @@
 LAMMPS Documentation
 
 Depending on how you obtained LAMMPS, this directory has 2 or 3
-sub-directories and optionally 2 PDF files:
+sub-directories and optionally 2 PDF files and an ePUB file:
 
 src             content files for LAMMPS documentation
 html            HTML version of the LAMMPS manual (see html/Manual.html)
 tools           tools and settings for building the documentation
 Manual.pdf      large PDF version of entire manual
 Developer.pdf   small PDF with info about how LAMMPS is structured
+LAMMPS.epub     Manual in ePUB format
 
 If you downloaded LAMMPS as a tarball from the web site, all these
 directories and files should be included.
@@ -49,6 +50,7 @@ make pdf          # generate 2 PDF files (Manual.pdf,Developer.pdf)
 make old          # generate old-style HTML pages in old dir via txt2html
 make fetch        # fetch HTML doc pages and 2 PDF files from web site
                   #   as a tarball and unpack into html dir and 2 PDFs
+make epub         # generate LAMMPS.epub in ePUB format using Sphinx 
 make clean        # remove intermediate RST files created by HTML build
 make clean-all    # remove entire build folder and any cached data
 
@@ -92,5 +94,22 @@ This will install virtualenv from the Python Package Index.
 
 Installing prerequisites for PDF build
 
+[TBA]
 
+----------------
+
+Installing prerequisites for epub build
+
+## ePUB
+
+Same as for HTML. This uses the same tools and configuration
+files as the HTML tree.
+
+For converting the generated ePUB file to a mobi format file
+(for e-book readers like Kindle, that cannot read ePUB), you
+also need to have the 'ebook-convert' tool from the "calibre"
+software installed. http://calibre-ebook.com/
+You first create the ePUB file with 'make epub' and then do:
+
+ebook-convert LAMMPS.epub LAMMPS.mobi
 

doc/src/2001/input_commands.html

@@ -464,7 +464,7 @@ the angletype option can only be assigned to a "fix style" of "shake",
   entirely rigid (e.g. water)
 the angletype option enables an additional check when SHAKE constraints
   are computed: if a cluster is of size 3 and both bonds in
-  the cluster are of a bondtype specified by the 2nd paramter of
+  the cluster are of a bondtype specified by the 2nd parameter of
   angletype, then the cluster is SHAKEn with an additional angle
   constraint that makes it rigid, using the equilibrium angle appropriate
   to the specified angletype
@@ -476,7 +476,7 @@ IMPORTANT NOTE: the angletype option has one additional affect, namely
   since they will not be SHAKEn but neither will the angle force by computed
 for style region, a coeff of INF means + or - infinity (all the way 
   to the boundary)
-an atom can be assigned to multiple constraints, the contraints will be
+an atom can be assigned to multiple constraints, the constraints will be
   applied in the reverse order they are assigned to that atom
   (e.g. each timestep, the last fix assigned to an atom will be applied 
   to it first, then the next-to-last applied second, etc)
@@ -689,7 +689,7 @@ coeffs:  types
          remainder
                no other parameters required
        
-used with "create temp" commmand to initialize velocities of atoms
+used with "create temp" command to initialize velocities of atoms
 by default, the "create temp" command initializes the velocities of all atoms,
   this command limits the initialization to a group of atoms
 this command is only in force for the next "create temp" command, any
@@ -1263,7 +1263,7 @@ when using constraints with the minimizer, fixes are
   applied when atoms move except for the following
 fixes associated with temperature control are not allowed
   (rescale, hoover/drag, langevin)
-the minimizer does not invoke the "fix style shake" contraints on
+the minimizer does not invoke the "fix style shake" constraints on
   bond lengths
 the minimizer does not invoke pressure control or volume control settings
 for good convergence, should specify use of smooth nonbond force fields 
@@ -1566,7 +1566,7 @@ mesh dimensions that are power-of-two are fastest for FFTs, but any sizes
   can be used that are supported by native machine libraries
 this command is optional - if not used, a default
   mesh size will be chosen to satisfy accuracy criterion - if used, the
-  specifed mesh size will override the default
+  specified mesh size will override the default
 </PRE>
 <HR>
 <H3>
@@ -1788,7 +1788,7 @@ if the style is 2, restart information will be written alternately to files
 when the minimizer is invoked this command means create a restart file
   at the end of the minimization with the filename filename.timestep.min
 a restart file stores atom and force-field information in binary form
-allows program to restart from where it left off (see &quot;read restart&quot; commmand)
+allows program to restart from where it left off (see &quot;read restart&quot; command)
 
 Default = 0
 </PRE>

doc/src/99/basics.html

@@ -167,7 +167,7 @@ tool on the small-system data file.</P>
 <P>
 (6) flow</P>
 <P>
-2-d flow of Lennard-Jones atoms in a channel using various contraint 
+2-d flow of Lennard-Jones atoms in a channel using various constraint
 options.</P>
 <P>
 (7) polymer</P>
@@ -201,7 +201,7 @@ The tools directory also has a F77 program called setup_chain.f
 (compile and link with print.c) which can be used to generate random 
 initial polymer configurations for bead-spring models like those used 
 in examples/polymer. It uses an input polymer definition file (see 
-examples/polymer for two sample def files) that specfies how many 
+examples/polymer for two sample def files) that specifies how many
 chains of what length, a random number seed, etc.</P>
 </BODY>
 </HTML>

doc/src/99/crib.html

@@ -40,7 +40,7 @@ Note: this file is somewhat out-of-date for LAMMPS 99.</P>
     <LI>
     maxtype = max # of atom types 
     <LI>
-    maxbond = max # of bonds to compute on one procesor 
+    maxbond = max # of bonds to compute on one processor
     <LI>
     maxangle = max # of angles to compute on one processor 
     <LI>

doc/src/99/input_commands.html

@@ -294,7 +294,7 @@ assign a group of atoms to a particular constraint
 use appropriate number of coeffs for a particular style
 the constraint itself is defined by the "fix style" command
 multiple groups of atoms can be assigned to the same constraint
-an atom can be assigned to multiple constraints, the contraints will be
+an atom can be assigned to multiple constraints, the constraints will be
   applied in the reverse order they are assigned to that atom
   (e.g. each timestep, the last fix assigned to an atom will be applied 
   to it first, then the next-to-last applied second, etc)
@@ -477,7 +477,7 @@ coeffs:  types
          remainder
                no other parameters required
        
-used with "create temp" commmand to initialize velocities of atoms
+used with "create temp" command to initialize velocities of atoms
 by default, the "create temp" command initializes the velocities of all atoms,
   this command limits the initialization to a group of atoms
 this command is only in force for the next "create temp" command, any
@@ -1124,7 +1124,7 @@ mesh dimensions that are power-of-two are fastest for FFTs, but any size
   can be used that are supported by native machine libraries
 this command is optional - if not used, a default
   mesh size will be chosen to satisfy accuracy criterion - if used, the
-  specifed mesh size will override the default
+  specified mesh size will override the default
 
 Default = none
 </PRE>
@@ -1343,7 +1343,7 @@ value of 0 means never create one
 program will toggle between 2 filenames as the run progresses
   so always have at least one good file even if the program dies in mid-write
 restart file stores atom positions and velocities in binary form
-allows program to restart from where it left off (see &quot;read restart&quot; commmand)
+allows program to restart from where it left off (see &quot;read restart&quot; command)
 
 Default = 0
 </PRE>

doc/src/Eqs/bond_oxdna_fene.tex

@@ -0,0 +1,10 @@
+\documentclass[12pt]{article}
+\pagestyle{empty}
+
+\begin{document}
+
+$$ 
+  E = - \frac{\epsilon}{2} \ln \left[ 1 - \left(\frac{r-r0}{\Delta}\right)^2\right]
+$$
+
+\end{document}

doc/src/Eqs/cnp_cutoff.tex

@@ -0,0 +1,14 @@
+\documentclass[12pt,article]{article}
+
+\usepackage{indentfirst}
+\usepackage{amsmath}
+
+\begin{document}
+
+\begin{eqnarray*}
+  r_{c}^{fcc} & = & \frac{1}{2} \left(\frac{\sqrt{2}}{2} + 1\right) \mathrm{a} \simeq 0.8536 \:\mathrm{a} \\
+  r_{c}^{bcc} & = & \frac{1}{2}(\sqrt{2} + 1) \mathrm{a} \simeq 1.207 \:\mathrm{a} \\
+  r_{c}^{hcp} & = & \frac{1}{2}\left(1+\sqrt{\frac{4+2x^{2}}{3}}\right) \mathrm{a}
+\end{eqnarray*}
+
+\end{document}

doc/src/Eqs/cnp_cutoff2.tex

@@ -0,0 +1,12 @@
+\documentclass[12pt,article]{article}
+
+\usepackage{indentfirst}
+\usepackage{amsmath}
+
+\begin{document}
+
+$$
+  Rc + Rs > 2*{\rm cutoff}
+$$
+
+\end{document}

doc/src/Eqs/cnp_eq.tex

@@ -0,0 +1,9 @@
+\documentclass[12pt]{article}
+
+\begin{document}
+
+$$
+   Q_{i} = \frac{1}{n_i}\sum_{j = 1}^{n_i} | \sum_{k = 1}^{n_{ij}}  \vec{R}_{ik} + \vec{R}_{jk} |^2
+$$
+
+\end{document}

doc/src/Eqs/fix_gcmc1.tex

@@ -0,0 +1,9 @@
+\documentclass[12pt]{article}
+
+\begin{document}
+
+\begin{eqnarray*}
+\mu &=&\mu^{id} + \mu^{ex}
+\end{eqnarray*}
+
+\end{document}

doc/src/Eqs/fix_gcmc2.tex

@@ -0,0 +1,10 @@
+\documentclass[12pt]{article}
+
+\begin{document}
+
+\begin{eqnarray*}
+\mu^{id} &=& k T \ln{\rho \Lambda^3} \\
+&=& k T \ln{\frac{\phi P \Lambda^3}{k T}} 
+\end{eqnarray*}
+
+\end{document}

doc/src/Eqs/fix_gcmc3.tex

@@ -0,0 +1,9 @@
+\documentclass[12pt]{article}
+
+\begin{document}
+
+\begin{eqnarray*}
+\Lambda &=& \sqrt{ \frac{h^2}{2 \pi m k T}}
+\end{eqnarray*}
+
+\end{document}

doc/src/Eqs/fix_grem.tex

@@ -0,0 +1,9 @@
+\documentclass[12pt]{article}
+
+\begin{document}
+
+$$
+  T_{eff} = \lambda + \eta (H - H_0)
+$$
+
+\end{document}

doc/src/Eqs/fix_wall_ees.tex

@@ -0,0 +1,10 @@
+\documentclass[12pt]{article}
+
+\begin{document}
+
+$$ 
+E = \epsilon \left[ \frac{2  \sigma_{LJ}^{12} \left(7 r^5+14 r^3 \sigma_{n}^2+3 r \sigma_{n}^4\right) }{945 \left(r^2-\sigma_{n}^2\right)^7} -\frac{ \sigma_{LJ}^6 \left(2 r \sigma_{n}^3+\sigma_{n}^2 \left(r^2-\sigma_{n}^2\right)\log{ \left[\frac{r-\sigma_{n}}{r+\sigma_{n}}\right]}\right) }{12 \sigma_{n}^5 \left(r^2-\sigma_{n}^2\right)} \right]\qquad \sigma_n < r < r_c
+$$
+
+
+\end{document}

doc/src/Eqs/pair_dpd_conservative.tex

@@ -1,9 +0,0 @@
-\documentclass[12pt]{article}
-\pagestyle{empty}
-\begin{document}
-
-$$
-F^C = A \omega_{ij} \qquad \qquad r_{ij} < r_c
-$$
-
-\end{document}

doc/src/Eqs/pair_dpd_energy.tex

@@ -0,0 +1,12 @@
+\documentclass[12pt]{article}
+\pagestyle{empty}
+\begin{document}
+
+\begin{eqnarray*}
+  du_{i}^{cond} & = & \kappa_{ij}(\frac{1}{\theta_{i}}-\frac{1}{\theta_{j}})\omega_{ij}^{2} + \alpha_{ij}\omega_{ij}\zeta_{ij}^{q}(\Delta{t})^{-1/2} \\
+  du_{i}^{mech} & = & -\frac{1}{2}\gamma_{ij}\omega_{ij}^{2}(\frac{\vec{r_{ij}}}{r_{ij}}\bullet\vec{v_{ij}})^{2} - 
+  \frac{\sigma^{2}_{ij}}{4}(\frac{1}{m_{i}}+\frac{1}{m_{j}})\omega_{ij}^{2} - 
+  \frac{1}{2}\sigma_{ij}\omega_{ij}(\frac{\vec{r_{ij}}}{r_{ij}}\bullet\vec{v_{ij}})\zeta_{ij}(\Delta{t})^{-1/2} \\
+\end{eqnarray*}                           
+
+\end{document}

doc/src/Eqs/pair_dpd_energy_terms.tex

@@ -0,0 +1,11 @@
+\documentclass[12pt]{article}
+\pagestyle{empty}
+\begin{document}
+
+\begin{eqnarray*}
+  \alpha_{ij}^{2} & = & 2k_{B}\kappa_{ij} \\
+  \sigma^{2}_{ij} & = & 2\gamma_{ij}k_{B}\Theta_{ij} \\
+  \Theta_{ij}^{-1} & = & \frac{1}{2}(\frac{1}{\theta_{i}}+\frac{1}{\theta_{j}}) \\
+\end{eqnarray*}                           
+
+\end{document}

doc/src/Eqs/pair_kolmogorov_crespi_z.tex

@@ -0,0 +1,13 @@
+\documentclass[12pt]{article}
+\thispagestyle{empty}
+
+\begin{document}
+
+\begin{eqnarray*}
+  E & = & \frac{1}{2} \sum_i \sum_{j \neq i} V_{ij} \\
+  V_{ij} & = & e^{-\lambda(r_{ij} -z_0}) \left[ C + f(\rho_{ij}) + f(\rho_{ji}) \right] - A \left( \frac{r_{ij}}{z_0}\right)^{-6} + A \left( \frac{\textrm{cutoff}}{z_0}\right)^{-6} \\
+  \rho_{ij}^2 = \rho_{ji}^2 & = &  x_{ij}^2 + y_{ij}^2 ~\hspace{2cm} (\mathbf{n_i}\equiv\hat \mathbf{z})\\
+  f(\rho) & = &  e^{-(\rho/\delta)^2} \sum_{n=0}^2 C_{2n} \left( \rho/\delta \right) ^{2n}
+\end{eqnarray*}
+
+\end{document}

doc/src/Eqs/pair_lj_sf.tex

@@ -1,11 +0,0 @@
-\documentclass[12pt]{article}
-
-\begin{document}
-
-\begin{eqnarray*}
- F & = & F_{\mathrm{LJ}}(r) - F_{\mathrm{LJ}}(r_{\mathrm{c}}) \qquad r < r_{\mathrm{c}} \\
- E & = & E_{\mathrm{LJ}}(r) - E_{\mathrm{LJ}}(r_{\mathrm{c}}) + (r - r_{\mathrm{c}}) F_{\mathrm{LJ}}(r_{\mathrm{c}}) \qquad r < r_{\mathrm{c}} \\
- \mathrm{with} \qquad E_{\mathrm{LJ}}(r) & = & 4 \epsilon \left[ \left(\frac{\sigma}{r}\right)^{12} - \left(\frac{\sigma}{r}\right)^6 \right] \qquad \mathrm{and} \qquad F_{\mathrm{LJ}}(r) = - E^\prime_{\mathrm{LJ}}(r)
-\end{eqnarray*}                           
-
-\end{document}

doc/src/Eqs/pair_meam_spline.tex

@@ -1,13 +1,14 @@
 \documentclass[12pt]{article}
+\usepackage{amsmath}
 
 \begin{document}
 
 $$
-   E=\sum_{ij}\phi(r_{ij})+\sum_{i}U(\rho_{i}),
+   E=\sum_{i<j}\phi(r_{ij})+\sum_{i}U(n_{i}),
 $$
 
 $$
-   \rho_{i}=\sum_{j}\rho(r_{ij})+\sum_{jk}f(r_{ij})f(r_{ik})g[\cos(\theta_{jik})]
+   n_{i}=\sum_{j}\rho(r_{ij})+\sum_{\substack{j<k,\\j,k\neq i}}f(r_{ij})f(r_{ik})g[\cos(\theta_{jik})]
 $$
 
 \end{document}

doc/src/Eqs/pair_meam_spline_multicomponent.tex

@@ -0,0 +1,14 @@
+\documentclass[12pt]{article}
+\usepackage{amsmath}
+
+\begin{document}
+
+$$
+   E=\sum_{i<j}\phi_{ij}(r_{ij})+\sum_{i}U_i(n_{i}),
+$$
+
+$$
+   n_{i}=\sum_{j\ne i}\rho_j(r_{ij})+\sum_{\substack{j<k,\\j,k\neq i}}f_{j}(r_{ij})f_{k}(r_{ik})g_{jk}[\cos(\theta_{jik})]
+$$
+
+\end{document}

doc/src/Eqs/pair_momb.tex

@@ -0,0 +1,13 @@
+\documentclass[12pt,fleqn]{article}
+\usepackage{amsmath}
+\thispagestyle{empty}
+
+\begin{document}
+
+\setlength{\jot}{2ex}
+\begin{gather*}
+  E = D_0 [\exp^{-2 \alpha (r-r_0)} - 2\exp^{-\alpha (r-r_0)}] - s_6 \frac{C_6}{r^6} f_{damp}(r,R_r) \\
+  f_{damp}(r,R_r) = \frac{1}{1 + \exp^{-d(r/R_r - 1)}}
+\end{gather*}
+
+\end{document}

doc/src/Eqs/pair_tersoff_mod_c.tex

@@ -0,0 +1,10 @@
+\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}

doc/src/Eqs/pressure.tex

@@ -3,7 +3,7 @@
 \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}

doc/src/Eqs/pressure_tensor.tex

@@ -4,7 +4,7 @@
 
 $$
    P_{IJ} = \frac{\sum_{k}^{N} m_k v_{k_I} v_{k_J}}{V} + 
-   \frac{\sum_{k}^{N} r_{k_I} f_{k_J}}{V}
+   \frac{\sum_{k}^{N'} r_{k_I} f_{k_J}}{V}
 $$
 
 \end{document}

doc/src/Manual.txt

@@ -1,7 +1,7 @@
 <!-- HTML_ONLY -->
 <HEAD>
 <TITLE>LAMMPS Users Manual</TITLE>
-<META NAME="docnumber" CONTENT="11 Oct 2016 version">
+<META NAME="docnumber" CONTENT="11 Aug 2017 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
-11 Oct 2016 version :c,h4
+11 Aug 2017 version :c,h4
 
 Version info: :h4
 
@@ -39,7 +39,7 @@ directory name created when you unpack a tarball, and at the top of
 the first page of the manual (this page).
 
 If you browse the HTML doc pages on the LAMMPS WWW site, they always
-describe the most current version of LAMMPS. :ulb,l
+describe the most current [development] version of LAMMPS. :ulb,l
 
 If you browse the HTML doc pages included in your tarball, they
 describe the version you have. :l
@@ -67,7 +67,7 @@ Labs and Temple University:
 
 "Steve Plimpton"_sjp, sjplimp at sandia.gov :ulb,l
 Aidan Thompson, athomps at sandia.gov :l
-Stan Moore, stamoore at sandia.gov :l
+Stan Moore, stamoor at sandia.gov :l
 "Axel Kohlmeyer"_ako, akohlmey at gmail.com :l
 :ule
 
@@ -158,12 +158,11 @@ END_RST -->
   2.1 "What's in the LAMMPS distribution"_start_1 :ulb,b
   2.2 "Making LAMMPS"_start_2 :b
   2.3 "Making LAMMPS with optional packages"_start_3 :b
-  2.4 "Building LAMMPS via the Make.py script"_start_4 :b
-  2.5 "Building LAMMPS as a library"_start_5 :b
-  2.6 "Running LAMMPS"_start_6 :b
-  2.7 "Command-line options"_start_7 :b
-  2.8 "Screen output"_start_8 :b
-  2.9 "Tips for users of previous versions"_start_9 :ule,b
+  2.4 "Building LAMMPS as a library"_start_4 :b
+  2.5 "Running LAMMPS"_start_5 :b
+  2.6 "Command-line options"_start_6 :b
+  2.7 "Screen output"_start_7 :b
+  2.8 "Tips for users of previous versions"_start_8 :ule,b
 "Commands"_Section_commands.html :l
   3.1 "LAMMPS input script"_cmd_1 :ulb,b
   3.2 "Parsing rules"_cmd_2 :b
@@ -262,7 +261,6 @@ END_RST -->
 :link(start_6,Section_start.html#start_6)
 :link(start_7,Section_start.html#start_7)
 :link(start_8,Section_start.html#start_8)
-:link(start_9,Section_start.html#start_9)
 
 :link(cmd_1,Section_commands.html#cmd_1)
 :link(cmd_2,Section_commands.html#cmd_2)

doc/src/Section_accelerate.txt

@@ -56,7 +56,7 @@ timings; you can simply extrapolate from short runs.
 
 For the set of runs, look at the timing data printed to the screen and
 log file at the end of each LAMMPS run.  "This
-section"_Section_start.html#start_8 of the manual has an overview.
+section"_Section_start.html#start_7 of the manual has an overview.
 
 Running on one (or a few processors) should give a good estimate of
 the serial performance and what portions of the timestep are taking
@@ -226,16 +226,16 @@ re-build LAMMPS |
   make machine |
 prepare and test a regular LAMMPS simulation |
   lmp_machine -in in.script; mpirun -np 32 lmp_machine -in in.script |
-enable specific accelerator support via '-k on' "command-line switch"_Section_start.html#start_7, |
+enable specific accelerator support via '-k on' "command-line switch"_Section_start.html#start_6, |
   only needed for KOKKOS package |
-set any needed options for the package via "-pk" "command-line switch"_Section_start.html#start_7 or "package"_package.html command, |
+set any needed options for the package via "-pk" "command-line switch"_Section_start.html#start_6 or "package"_package.html command, |
   only if defaults need to be changed |
-use accelerated styles in your input via "-sf" "command-line switch"_Section_start.html#start_7 or "suffix"_suffix.html command | lmp_machine -in in.script -sf gpu
+use accelerated styles in your input via "-sf" "command-line switch"_Section_start.html#start_6 or "suffix"_suffix.html command | lmp_machine -in in.script -sf gpu
 :tb(c=2,s=|)
 
-Note that the first 4 steps can be done as a single command, using the
-src/Make.py tool.  This tool is discussed in "Section
-2.4"_Section_start.html#start_4 of the manual, and its use is
+Note that the first 4 steps can be done as a single command with
+suitable make command invocations. This is discussed in "Section
+4"_Section_packages.html of the manual, and its use is
 illustrated in the individual accelerator sections.  Typically these
 steps only need to be done once, to create an executable that uses one
 or more accelerator packages.

doc/src/Section_commands.txt

@@ -106,7 +106,7 @@ the $.  Thus $\{myTemp\} and $x refer to variable names "myTemp" and
 "x".
 
 How the variable is converted to a text string depends on what style
-of variable it is; see the "variable"_variable doc page for details.
+of variable it is; see the "variable"_variable.html doc page for details.
 It can be a variable that stores multiple text strings, and return one
 of them.  The returned text string can be multiple "words" (space
 separated) which will then be interpreted as multiple arguments in the
@@ -281,79 +281,136 @@ the "minimize"_minimize.html command.  A parallel tempering
 
 3.4 Commands listed by category :link(cmd_4),h4
 
-This section lists all LAMMPS commands, grouped by category.  The
-"next section"_#cmd_5 lists the same commands alphabetically.  Note
-that some style options for some commands are part of specific LAMMPS
-packages, which means they cannot be used unless the package was
-included when LAMMPS was built.  Not all packages are included in a
-default LAMMPS build.  These dependencies are listed as Restrictions
-in the command's documentation.
+This section lists core LAMMPS commands, grouped by category.
+The "next section"_#cmd_5 lists all commands alphabetically.  The
+next section also includes (long) lists of style options for entries
+that appear in the following categories as a single command (fix,
+compute, pair, etc).  Commands that are added by user packages are not
+included in the categories here, but they are in the next section.
 
 Initialization:
 
-"atom_modify"_atom_modify.html, "atom_style"_atom_style.html,
-"boundary"_boundary.html, "dimension"_dimension.html,
-"newton"_newton.html, "processors"_processors.html, "units"_units.html
+"newton"_newton.html,
+"package"_package.html,
+"processors"_processors.html,
+"suffix"_suffix.html,
+"units"_units.html
 
-Atom definition:
+Setup simulation box:
 
-"create_atoms"_create_atoms.html, "create_box"_create_box.html,
-"lattice"_lattice.html, "read_data"_read_data.html,
-"read_dump"_read_dump.html, "read_restart"_read_restart.html,
-"region"_region.html, "replicate"_replicate.html
+"boundary"_boundary.html,
+"box"_box.html,
+"change_box"_change_box.html,
+"create_box"_create_box.html,
+"dimension"_dimension.html,
+"lattice"_lattice.html,
+"region"_region.html
+
+Setup atoms:
+
+"atom_modify"_atom_modify.html,
+"atom_style"_atom_style.html,
+"balance"_balance.html,
+"create_atoms"_create_atoms.html,
+"create_bonds"_create_bonds.html,
+"delete_atoms"_delete_atoms.html,
+"delete_bonds"_delete_bonds.html,
+"displace_atoms"_displace_atoms.html,
+"group"_group.html,
+"mass"_mass.html,
+"molecule"_molecule.html,
+"read_data"_read_data.html,
+"read_dump"_read_dump.html,
+"read_restart"_read_restart.html,
+"replicate"_replicate.html,
+"set"_set.html,
+"velocity"_velocity.html
 
 Force fields:
 
-"angle_coeff"_angle_coeff.html, "angle_style"_angle_style.html,
-"bond_coeff"_bond_coeff.html, "bond_style"_bond_style.html,
-"dielectric"_dielectric.html, "dihedral_coeff"_dihedral_coeff.html,
+"angle_coeff"_angle_coeff.html,
+"angle_style"_angle_style.html,
+"bond_coeff"_bond_coeff.html,
+"bond_style"_bond_style.html,
+"bond_write"_bond_write.html,
+"dielectric"_dielectric.html,
+"dihedral_coeff"_dihedral_coeff.html,
 "dihedral_style"_dihedral_style.html,
 "improper_coeff"_improper_coeff.html,
 "improper_style"_improper_style.html,
-"kspace_modify"_kspace_modify.html, "kspace_style"_kspace_style.html,
-"pair_coeff"_pair_coeff.html, "pair_modify"_pair_modify.html,
-"pair_style"_pair_style.html, "pair_write"_pair_write.html,
+"kspace_modify"_kspace_modify.html,
+"kspace_style"_kspace_style.html,
+"pair_coeff"_pair_coeff.html,
+"pair_modify"_pair_modify.html,
+"pair_style"_pair_style.html,
+"pair_write"_pair_write.html,
 "special_bonds"_special_bonds.html
 
 Settings:
 
-"comm_style"_comm_style.html, "group"_group.html, "mass"_mass.html,
-"min_modify"_min_modify.html, "min_style"_min_style.html,
-"neigh_modify"_neigh_modify.html, "neighbor"_neighbor.html,
-"reset_timestep"_reset_timestep.html, "run_style"_run_style.html,
-"set"_set.html, "timestep"_timestep.html, "velocity"_velocity.html
+"comm_modify"_comm_modify.html,
+"comm_style"_comm_style.html,
+"info"_info.html,
+"min_modify"_min_modify.html,
+"min_style"_min_style.html,
+"neigh_modify"_neigh_modify.html,
+"neighbor"_neighbor.html,
+"partition"_partition.html,
+"reset_timestep"_reset_timestep.html,
+"run_style"_run_style.html,
+"timer"_timer.html,
+"timestep"_timestep.html
 
-Fixes:
+Operations within timestepping (fixes) and diagnostics (computes):
 
-"fix"_fix.html, "fix_modify"_fix_modify.html, "unfix"_unfix.html
-
-Computes:
-
-"compute"_compute.html, "compute_modify"_compute_modify.html,
-"uncompute"_uncompute.html
+"compute"_compute.html,
+"compute_modify"_compute_modify.html,
+"fix"_fix.html,
+"fix_modify"_fix_modify.html,
+"uncompute"_uncompute.html,
+"unfix"_unfix.html
 
 Output:
 
-"dump"_dump.html, "dump image"_dump_image.html,
-"dump_modify"_dump_modify.html, "dump movie"_dump_image.html,
-"restart"_restart.html, "thermo"_thermo.html,
-"thermo_modify"_thermo_modify.html, "thermo_style"_thermo_style.html,
-"undump"_undump.html, "write_data"_write_data.html,
-"write_dump"_write_dump.html, "write_restart"_write_restart.html
+"dump image"_dump_image.html,
+"dump movie"_dump_image.html,
+"dump"_dump.html,
+"dump_modify"_dump_modify.html,
+"restart"_restart.html,
+"thermo"_thermo.html,
+"thermo_modify"_thermo_modify.html,
+"thermo_style"_thermo_style.html,
+"undump"_undump.html,
+"write_coeff"_write_coeff.html,
+"write_data"_write_data.html,
+"write_dump"_write_dump.html,
+"write_restart"_write_restart.html
 
 Actions:
 
-"delete_atoms"_delete_atoms.html, "delete_bonds"_delete_bonds.html,
-"displace_atoms"_displace_atoms.html, "change_box"_change_box.html,
-"minimize"_minimize.html, "neb"_neb.html "prd"_prd.html,
-"rerun"_rerun.html, "run"_run.html, "temper"_temper.html
+"minimize"_minimize.html,
+"neb"_neb.html,
+"prd"_prd.html,
+"rerun"_rerun.html,
+"run"_run.html,
+"tad"_tad.html,
+"temper"_temper.html
 
-Miscellaneous:
+Input script control:
 
-"clear"_clear.html, "echo"_echo.html, "if"_if.html,
-"include"_include.html, "jump"_jump.html, "label"_label.html,
-"log"_log.html, "next"_next.html, "print"_print.html,
-"shell"_shell.html, "variable"_variable.html
+"clear"_clear.html,
+"echo"_echo.html,
+"if"_if.html,
+"include"_include.html,
+"jump"_jump.html,
+"label"_label.html,
+"log"_log.html,
+"next"_next.html,
+"print"_print.html,
+"python"_python.html,
+"quit"_quit.html,
+"shell"_shell.html,
+"variable"_variable.html
 
 :line
 
@@ -470,9 +527,12 @@ These are additional commands in USER packages, which can be used if
 "LAMMPS is built with the appropriate
 package"_Section_start.html#start_3.
 
-"dump custom/vtk"_dump_custom_vtk.html,
+"dump netcdf"_dump_netcdf.html,
+"dump netcdf/mpiio"_dump_netcdf.html,
+"dump vtk"_dump_vtk.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
 
@@ -516,12 +576,14 @@ USER-INTEL, k = KOKKOS, o = USER-OMP, t = OPT.
 "gcmc"_fix_gcmc.html,
 "gld"_fix_gld.html,
 "gravity (o)"_fix_gravity.html,
+"halt"_fix_halt.html,
 "heat"_fix_heat.html,
 "indent"_fix_indent.html,
 "langevin (k)"_fix_langevin.html,
 "lineforce"_fix_lineforce.html,
-"momentum"_fix_momentum.html,
+"momentum (k)"_fix_momentum.html,
 "move"_fix_move.html,
+"mscg"_fix_mscg.html,
 "msst"_fix_msst.html,
 "neb"_fix_neb.html,
 "nph (ko)"_fix_nh.html,
@@ -556,6 +618,7 @@ USER-INTEL, k = KOKKOS, o = USER-OMP, t = OPT.
 "press/berendsen"_fix_press_berendsen.html,
 "print"_fix_print.html,
 "property/atom"_fix_property_atom.html,
+"python"_fix_python.html,
 "qeq/comb (o)"_fix_qeq_comb.html,
 "qeq/dynamic"_fix_qeq.html,
 "qeq/fire"_fix_qeq.html,
@@ -572,10 +635,10 @@ USER-INTEL, k = KOKKOS, o = USER-OMP, t = OPT.
 "rigid/nve (o)"_fix_rigid.html,
 "rigid/nvt (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,
-"rigid/small/nvt"_fix_rigid.html,
+"rigid/small/nph (o)"_fix_rigid.html,
+"rigid/small/npt (o)"_fix_rigid.html,
+"rigid/small/nve (o)"_fix_rigid.html,
+"rigid/small/nvt (o)"_fix_rigid.html,
 "setforce (k)"_fix_setforce.html,
 "shake"_fix_shake.html,
 "spring"_fix_spring.html,
@@ -618,14 +681,17 @@ package"_Section_start.html#start_3.
 "atc"_fix_atc.html,
 "ave/correlate/long"_fix_ave_correlate_long.html,
 "colvars"_fix_colvars.html,
+"dpd/energy"_fix_dpd_energy.html,
 "drude"_fix_drude.html,
 "drude/transform/direct"_fix_drude_transform.html,
 "drude/transform/reverse"_fix_drude_transform.html,
 "eos/cv"_fix_eos_cv.html,
 "eos/table"_fix_eos_table.html,
 "eos/table/rx"_fix_eos_table_rx.html,
+"filter/corotate"_fix_filter_corotate.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,
@@ -638,7 +704,10 @@ package"_Section_start.html#start_3.
 "meso"_fix_meso.html,
 "manifoldforce"_fix_manifoldforce.html,
 "meso/stationary"_fix_meso_stationary.html,
+"nve/dot"_fix_nve_dot.html,
+"nve/dotc/langevin"_fix_nve_dotc_langevin.html,
 "nve/manifold/rattle"_fix_nve_manifold_rattle.html,
+"nvk"_fix_nvk.html,
 "nvt/manifold/rattle"_fix_nvt_manifold_rattle.html,
 "nph/eff"_fix_nh_eff.html,
 "npt/eff"_fix_nh_eff.html,
@@ -648,7 +717,7 @@ package"_Section_start.html#start_3.
 "phonon"_fix_phonon.html,
 "pimd"_fix_pimd.html,
 "qbmsst"_fix_qbmsst.html,
-"qeq/reax"_fix_qeq_reax.html,
+"qeq/reax (ko)"_fix_qeq_reax.html,
 "qmmm"_fix_qmmm.html,
 "qtb"_fix_qtb.html,
 "reax/c/bonds"_fix_reax_bonds.html,
@@ -665,7 +734,9 @@ package"_Section_start.html#start_3.
 "smd/wall/surface"_fix_smd_wall_surface.html,
 "temp/rescale/eff"_fix_temp_rescale_eff.html,
 "ti/spring"_fix_ti_spring.html,
-"ttm/mod"_fix_ttm.html :tb(c=6,ea=c)
+"ttm/mod"_fix_ttm.html,
+"wall/ees"_fix_wall_ees.html,
+"wall/region/ees"_fix_wall_ees.html :tb(c=6,ea=c)
 
 :line
 
@@ -704,6 +775,7 @@ KOKKOS, o = USER-OMP, t = OPT.
 "erotate/sphere"_compute_erotate_sphere.html,
 "erotate/sphere/atom"_compute_erotate_sphere_atom.html,
 "event/displace"_compute_event_displace.html,
+"global/atom"_compute_global_atom.html,
 "group/group"_compute_group_group.html,
 "gyration"_compute_gyration.html,
 "gyration/chunk"_compute_gyration_chunk.html,
@@ -761,6 +833,7 @@ package"_Section_start.html#start_3.
 
 "ackland/atom"_compute_ackland_atom.html,
 "basal/atom"_compute_basal_atom.html,
+"cnp/atom"_compute_cnp_atom.html,
 "dpd"_compute_dpd.html,
 "dpd/atom"_compute_dpd_atom.html,
 "fep"_compute_fep.html,
@@ -825,6 +898,8 @@ 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,
@@ -848,10 +923,10 @@ 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 (gkiot)"_pair_eam.html,
 "eam/alloy (gkot)"_pair_eam.html,
 "eam/fs (gkot)"_pair_eam.html,
 "eim (o)"_pair_eim.html,
@@ -860,6 +935,8 @@ KOKKOS, o = USER-OMP, t = OPT.
 "gran/hertz/history (o)"_pair_gran.html,
 "gran/hooke (o)"_pair_gran.html,
 "gran/hooke/history (o)"_pair_gran.html,
+"gw"_pair_gw.html,
+"gw/zbl"_pair_gw.html,
 "hbond/dreiding/lj (o)"_pair_hbond_dreiding.html,
 "hbond/dreiding/morse (o)"_pair_hbond_dreiding.html,
 "kim"_pair_kim.html,
@@ -869,6 +946,8 @@ KOKKOS, o = USER-OMP, t = OPT.
 "lj/charmm/coul/charmm/implicit (ko)"_pair_charmm.html,
 "lj/charmm/coul/long (giko)"_pair_charmm.html,
 "lj/charmm/coul/msm"_pair_charmm.html,
+"lj/charmmfsw/coul/charmmfsh"_pair_charmm.html,
+"lj/charmmfsw/coul/long"_pair_charmm.html,
 "lj/class2 (gko)"_pair_class2.html,
 "lj/class2/coul/cut (ko)"_pair_class2.html,
 "lj/class2/coul/long (gko)"_pair_class2.html,
@@ -887,7 +966,7 @@ KOKKOS, o = USER-OMP, t = OPT.
 "lj/expand (gko)"_pair_lj_expand.html,
 "lj/gromacs (gko)"_pair_gromacs.html,
 "lj/gromacs/coul/gromacs (ko)"_pair_gromacs.html,
-"lj/long/coul/long (o)"_pair_lj_long.html,
+"lj/long/coul/long (io)"_pair_lj_long.html,
 "lj/long/dipole/long"_pair_dipole.html,
 "lj/long/tip4p/long"_pair_lj_long.html,
 "lj/smooth (o)"_pair_lj_smooth.html,
@@ -899,7 +978,7 @@ KOKKOS, o = USER-OMP, t = OPT.
 "lubricateU/poly"_pair_lubricateU.html,
 "meam"_pair_meam.html,
 "mie/cut (o)"_pair_mie.html,
-"morse (got)"_pair_morse.html,
+"morse (gkot)"_pair_morse.html,
 "nb3b/harmonic (o)"_pair_nb3b_harmonic.html,
 "nm/cut (o)"_pair_nm.html,
 "nm/cut/coul/cut (o)"_pair_nm.html,
@@ -909,6 +988,7 @@ KOKKOS, o = USER-OMP, t = OPT.
 "peri/pmb (o)"_pair_peri.html,
 "peri/ves"_pair_peri.html,
 "polymorphic"_pair_polymorphic.html,
+"python"_pair_python.html,
 "reax"_pair_reax.html,
 "rebo (o)"_pair_airebo.html,
 "resquared (go)"_pair_resquared.html,
@@ -918,11 +998,13 @@ 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,
 "zbl (go)"_pair_zbl.html :tb(c=4,ea=c)
@@ -931,6 +1013,7 @@ 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,
@@ -940,9 +1023,11 @@ package"_Section_start.html#start_3.
 "dpd/fdt/energy"_pair_dpd_fdt.html,
 "eam/cd (o)"_pair_eam.html,
 "edip (o)"_pair_edip.html,
+"edip/multi"_pair_edip.html,
 "eff/cut"_pair_eff.html,
 "exp6/rx"_pair_exp6_rx.html,
 "gauss/cut"_pair_gauss.html,
+"kolmogorov/crespi/z"_pair_kolmogorov_crespi_z.html,
 "lennard/mdf"_pair_mdf.html,
 "list"_pair_list.html,
 "lj/charmm/coul/long/soft (o)"_pair_charmm.html,
@@ -956,16 +1041,26 @@ package"_Section_start.html#start_3.
 "lj/sdk (gko)"_pair_sdk.html,
 "lj/sdk/coul/long (go)"_pair_sdk.html,
 "lj/sdk/coul/msm (o)"_pair_sdk.html,
-"lj/sf (o)"_pair_lj_sf.html,
+"meam/c"_pair_meam.html,
 "meam/spline (o)"_pair_meam_spline.html,
 "meam/sw/spline"_pair_meam_sw_spline.html,
 "mgpt"_pair_mgpt.html,
+"momb"_pair_momb.html,
 "morse/smooth/linear"_pair_morse.html,
 "morse/soft"_pair_morse.html,
 "multi/lucy"_pair_multi_lucy.html,
 "multi/lucy/rx"_pair_multi_lucy_rx.html,
+"oxdna/coaxstk"_pair_oxdna.html,
+"oxdna/excv"_pair_oxdna.html,
+"oxdna/hbond"_pair_oxdna.html,
+"oxdna/stk"_pair_oxdna.html,
+"oxdna/xstk"_pair_oxdna.html,
+"oxdna2/coaxstk"_pair_oxdna2.html,
+"oxdna2/dh"_pair_oxdna2.html,
+"oxdna2/excv"_pair_oxdna2.html,
+"oxdna2/stk"_pair_oxdna2.html,
 "quip"_pair_quip.html,
-"reax/c (k)"_pair_reax_c.html,
+"reax/c (ko)"_pair_reaxc.html,
 "smd/hertz"_pair_smd_hertz.html,
 "smd/tlsph"_pair_smd_tlsph.html,
 "smd/triangulated/surface"_pair_smd_triangulated_surface.html,
@@ -998,7 +1093,7 @@ KOKKOS, o = USER-OMP, t = OPT.
 "none"_bond_none.html,
 "zero"_bond_zero.html,
 "hybrid"_bond_hybrid.html,
-"class2 (o)"_bond_class2.html,
+"class2 (ko)"_bond_class2.html,
 "fene (iko)"_bond_fene.html,
 "fene/expand (o)"_bond_fene_expand.html,
 "harmonic (ko)"_bond_harmonic.html,
@@ -1012,7 +1107,9 @@ if "LAMMPS is built with the appropriate
 package"_Section_start.html#start_3.
 
 "harmonic/shift (o)"_bond_harmonic_shift.html,
-"harmonic/shift/cut (o)"_bond_harmonic_shift_cut.html :tb(c=4,ea=c)
+"harmonic/shift/cut (o)"_bond_harmonic_shift_cut.html,
+"oxdna/fene"_bond_oxdna.html,
+"oxdna2/fene"_bond_oxdna.html :tb(c=4,ea=c)
 
 :line
 
@@ -1030,7 +1127,7 @@ USER-OMP, t = OPT.
 "zero"_angle_zero.html,
 "hybrid"_angle_hybrid.html,
 "charmm (ko)"_angle_charmm.html,
-"class2 (o)"_angle_class2.html,
+"class2 (ko)"_angle_class2.html,
 "cosine (o)"_angle_cosine.html,
 "cosine/delta (o)"_angle_cosine_delta.html,
 "cosine/periodic (o)"_angle_cosine_periodic.html,
@@ -1066,7 +1163,8 @@ USER-OMP, t = OPT.
 "zero"_dihedral_zero.html,
 "hybrid"_dihedral_hybrid.html,
 "charmm (ko)"_dihedral_charmm.html,
-"class2 (o)"_dihedral_class2.html,
+"charmmfsw"_dihedral_charmm.html,
+"class2 (ko)"_dihedral_class2.html,
 "harmonic (io)"_dihedral_harmonic.html,
 "helix (o)"_dihedral_helix.html,
 "multi/harmonic (o)"_dihedral_multi_harmonic.html,
@@ -1098,7 +1196,7 @@ USER-OMP, t = OPT.
 "none"_improper_none.html,
 "zero"_improper_zero.html,
 "hybrid"_improper_hybrid.html,
-"class2 (o)"_improper_class2.html,
+"class2 (ko)"_improper_class2.html,
 "cvff (io)"_improper_cvff.html,
 "harmonic (ko)"_improper_harmonic.html,
 "umbrella (o)"_improper_umbrella.html :tb(c=4,ea=c)
@@ -1130,7 +1228,7 @@ USER-OMP, t = OPT.
 "msm/cg (o)"_kspace_style.html,
 "pppm (go)"_kspace_style.html,
 "pppm/cg (o)"_kspace_style.html,
-"pppm/disp"_kspace_style.html,
+"pppm/disp (i)"_kspace_style.html,
 "pppm/disp/tip4p"_kspace_style.html,
 "pppm/stagger"_kspace_style.html,
 "pppm/tip4p (o)"_kspace_style.html :tb(c=4,ea=c)