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319 Commits

Author SHA1 Message Date
78533e25dc git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16053 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-26 21:05:57 +00:00
be3cacddef git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16052 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-26 21:05:55 +00:00
5d3e441e59 sync with latest GHub bug fixes
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16051 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-26 20:54:58 +00:00
43e2d2443f Added validated parameter file for 2NN Tungsten potential
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16050 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-26 02:07:37 +00:00
406a4da000 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16049 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-23 23:04:40 +00:00
841cae3682 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16048 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-23 22:40:21 +00:00
28af591168 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16046 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-20 20:23:11 +00:00
20805d47b3 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16045 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-20 20:23:08 +00:00
4008b967ee git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16044 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-20 20:21:13 +00:00
c79a21970b sync latest bug fixes from GHub
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16043 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-20 20:20:31 +00:00
c771e00a1c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16042 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-19 20:47:38 +00:00
507b038f41 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16041 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-19 15:50:30 +00:00
bd4d5bdcac git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16040 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-19 15:50:18 +00:00
e0d0ef12cc git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16039 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-19 15:14:59 +00:00
43370b75a1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16038 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-19 15:11:33 +00:00
60f2b25b3f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16037 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-19 15:11:17 +00:00
9a3d05a86a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16036 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 23:40:20 +00:00
88eca7c181 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16035 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 23:32:26 +00:00
298e62ae70 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16034 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 23:32:09 +00:00
6ac456e751 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16033 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 23:15:15 +00:00
02b6519599 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16032 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 22:08:26 +00:00
b471be9638 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16031 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 20:07:25 +00:00
019d28ae7d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16030 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 20:04:19 +00:00
062450abc8 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16029 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 18:36:08 +00:00
e13633b881 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16028 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-18 18:34:39 +00:00
52c45f67f3 sync with GHub and new OXDNA user package
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16027 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-18 18:33:29 +00:00
1f0e32e0ae git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16024 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 17:06:43 +00:00
465f33d3f4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16023 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 17:06:41 +00:00
fdef2e7011 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16022 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 17:06:28 +00:00
e878b8fd52 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16021 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 16:53:53 +00:00
460202c149 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16020 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 16:53:04 +00:00
e6adb5c2a1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16019 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 16:51:53 +00:00
9b01275837 neighbor list bug fixes, new compute coord/atom option
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16018 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-17 16:44:40 +00:00
23cfb88bb9 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16017 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-17 16:00:09 +00:00
645d30dfa4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16016 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-11 20:57:49 +00:00
6dc24ea90d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16015 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-11 17:25:33 +00:00
1820b6785f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16014 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-10 23:31:32 +00:00
9c01b1b75f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16013 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-10 21:33:27 +00:00
9619521426 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16011 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:31:56 +00:00
f5b8906eb6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16010 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:31:54 +00:00
eb79a5f03c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16009 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:30:53 +00:00
9daf579909 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16008 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:30:12 +00:00
515a68d663 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16007 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:29:27 +00:00
2bf46e0c11 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16006 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:20:07 +00:00
de83ad9df1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16003 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 20:11:26 +00:00
27805f36b2 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16002 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 19:56:54 +00:00
f9f2c96d17 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16001 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 18:26:52 +00:00
c093ec15a5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@16000 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 18:15:09 +00:00
663f6403ef git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15999 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 18:15:00 +00:00
f22fcaed9f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15998 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 17:47:31 +00:00
fd2bdcd5d5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15997 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 17:46:25 +00:00
f8ee20372b git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15996 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 17:39:37 +00:00
3e5991f7da git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15995 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 17:38:53 +00:00
8423271025 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15994 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-09 16:17:20 +00:00
77339b61b7 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15992 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-06 18:12:13 +00:00
72c5cf7045 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15991 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-06 18:12:10 +00:00
fd8876234a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15990 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-06 17:24:38 +00:00
2b77cb5c5d sync with GHub
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15989 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-06 17:16:03 +00:00
a56413c0da git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15988 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 23:38:44 +00:00
8b3c8341e1 Updating modify_kokkos to match modify
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15987 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-05 22:50:55 +00:00
6e26482003 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15986 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 22:08:14 +00:00
9e91ee9ffc Updating modify_kokkos to match modify
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15985 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2017-01-05 21:31:06 +00:00
171530acc1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15984 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:55:13 +00:00
58fb78379d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15983 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:13:13 +00:00
102f30005c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15982 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:12:52 +00:00
f7bd264706 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15981 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:11:35 +00:00
35a929015e git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15980 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:10:41 +00:00
13a8dbca4a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15979 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:09:54 +00:00
5a46527886 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15978 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:08:12 +00:00
c0165e1261 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15977 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 20:07:11 +00:00
f55a51e1b5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15976 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 19:57:44 +00:00
b597aa6dac git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15975 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 19:56:46 +00:00
702b480cc0 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15974 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 19:56:42 +00:00
07c0fccf7b git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15973 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 19:56:37 +00:00
d85648ae2d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15972 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-05 19:56:10 +00:00
9c1de594e8 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15971 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-04 23:26:22 +00:00
139a159a5d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15970 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-04 23:25:56 +00:00
2854350708 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15969 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-04 19:55:04 +00:00
d289d195e9 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15968 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-04 16:12:26 +00:00
ac342f3687 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15967 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-04 15:52:53 +00:00
0f819c1e25 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15966 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-03 23:41:02 +00:00
c28560301d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15965 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-03 23:36:00 +00:00
2449e14f6d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15964 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2017-01-03 23:31:04 +00:00
8486258c73 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15959 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-21 16:53:12 +00:00
e1b30b2787 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15958 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-21 16:53:09 +00:00
a47b59c303 sync with GHub
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15957 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-12-21 16:51:39 +00:00
4732f90521 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15956 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-21 16:44:36 +00:00
7339480095 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15952 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-17 00:46:28 +00:00
68a358a0f4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15951 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-17 00:43:52 +00:00
34216ead1f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15950 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 20:08:46 +00:00
0bb23c5810 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15948 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 18:36:32 +00:00
f9f487f5ca git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15947 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 18:36:30 +00:00
44fd05c97d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15946 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 18:32:09 +00:00
4b8b9b97cc git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15944 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 17:29:46 +00:00
fbc8fa111a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15943 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 17:29:44 +00:00
c71bba1980 sync with GHub
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15942 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-12-16 17:26:10 +00:00
47a6449148 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15941 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 17:22:59 +00:00
e72aa59d83 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15940 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 17:22:46 +00:00
1b7e8eb7aa git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15939 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-16 16:24:33 +00:00
bee06997fb git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15938 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 16:11:08 +00:00
60e08ad7b7 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15936 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 00:10:56 +00:00
104ad18e0c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15935 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 00:10:53 +00:00
155dccacda git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15933 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 00:04:50 +00:00
35f8a9009d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15932 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 00:04:35 +00:00
5f04559071 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15931 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 00:00:20 +00:00
89719fb171 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15930 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-14 00:00:07 +00:00
6963dd2d83 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15929 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-13 23:58:45 +00:00
11e436ab43 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15928 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-13 23:44:51 +00:00
b0d24754a3 changes to all neighbor classes
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15927 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-12-13 23:27:33 +00:00
8320f9dcee git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15926 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-13 23:20:43 +00:00
45715f993c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15925 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-13 22:56:08 +00:00
abab6e8d99 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15924 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-13 22:46:40 +00:00
3846395e09 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15923 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-12-09 15:31:23 +00:00
c24d10ad7c Fixing bug in ewald disp
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15922 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-12-08 20:03:23 +00:00
e14a2bf12d Tweaking ewald disp error estimator
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15921 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-12-08 16:54:30 +00:00
2d36ae2f8d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15920 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 23:04:18 +00:00
0d64dd3eea git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15919 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 22:49:05 +00:00
8bd4c37e0e git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15918 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 22:45:53 +00:00
a70e2f6db4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15916 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 21:04:12 +00:00
8d7ba77ab2 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15915 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 21:04:08 +00:00
745050a374 sync with GHub
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2016-11-30 21:03:35 +00:00
c2b852f940 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15913 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 20:59:16 +00:00
489272ed91 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15912 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 20:57:03 +00:00
a5ee9da9c5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15911 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 20:56:54 +00:00
7a3103c911 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15910 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 20:10:37 +00:00
ecfa2d85f5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15908 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-30 20:06:19 +00:00
9b9291b417 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15906 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 20:18:28 +00:00
fa304895ea git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15905 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 20:17:01 +00:00
64c021824a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15904 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 18:17:52 +00:00
6a5a95d0b0 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15902 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 16:21:57 +00:00
810a7bca52 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15901 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 16:21:55 +00:00
09a388e5d4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15897 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 16:10:37 +00:00
09eb377cb8 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15896 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:58:36 +00:00
a70d5f71b9 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15895 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:55:07 +00:00
d692a47d73 sync with recent GHub PRs
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15894 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-22 15:52:42 +00:00
40762e69ce git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15893 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:47:10 +00:00
3856965055 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15892 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:43:59 +00:00
a4eaf200b5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15891 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:43:28 +00:00
1a3a1b1e72 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15890 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:20:24 +00:00
da9bea2355 new temper_grem command
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15889 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-22 15:16:29 +00:00
98b025d053 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15888 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-22 15:14:36 +00:00
2af2091bd2 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15886 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 23:13:20 +00:00
6471c2750b git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15885 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 23:13:17 +00:00
76182cb892 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15884 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 23:10:42 +00:00
dad749b37f Updated explanation of how virial is computed
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15883 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-17 19:36:20 +00:00
0701201e03 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15882 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 17:37:27 +00:00
80d6518602 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15880 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 17:21:17 +00:00
e81c5e3fdf git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15879 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 16:23:37 +00:00
47be003191 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15878 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-17 16:15:56 +00:00
41745a3b90 pair vashishta/kk, pair tersoff/mod/c, pair agni
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15877 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-17 16:06:01 +00:00
5692ea7977 Added note on pressure for periodic systems
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15876 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-16 19:53:05 +00:00
597f874f3d Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15875 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-15 19:37:05 +00:00
2b82e83d13 Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15874 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-15 19:33:36 +00:00
23b468e74f Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15873 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-15 17:41:16 +00:00
16efa68d35 Fixing clang compile error
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15872 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-15 17:07:06 +00:00
fa8d7c1d6e Adding missing Kokkos dependency
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15871 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-15 15:42:30 +00:00
846f11db5c Fixing bug with Kokkos/CUDA
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15870 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-15 15:28:36 +00:00
1ee5247500 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15869 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-14 21:49:29 +00:00
1d8db38a75 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15868 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-11 15:59:32 +00:00
f378934817 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15866 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:47:02 +00:00
aa8cce5b06 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15865 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:46:59 +00:00
57c0d77c71 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15863 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:42:46 +00:00
b1f7de2776 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15862 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:41:53 +00:00
ebe6ee813c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15861 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:41:17 +00:00
b222f8b946 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15860 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:40:33 +00:00
6b0a8628f2 sync pointer changes with GHub and 2 new pair styles
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15859 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-09 22:37:03 +00:00
5c141edca7 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15858 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 22:35:41 +00:00
3a2cea52d8 Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15857 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-09 20:00:27 +00:00
45f2940225 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15856 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-09 18:45:21 +00:00
07bb6fe443 Adding support for CommTiledKokkos
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15854 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-08 16:23:24 +00:00
b6b7c3ad67 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15852 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-08 16:04:44 +00:00
55fa0f2e8a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15851 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-08 16:04:40 +00:00
c770e270f2 Adding support for CommTiledKokkos
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15848 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-08 15:43:15 +00:00
d077a8b024 Adding support for CommTiledKokkos
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15847 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-08 15:30:12 +00:00
e147701e87 Updating Kokkos phi Makefile
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15846 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-08 15:26:08 +00:00
cc0be86470 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15841 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-07 15:23:10 +00:00
34966b3a38 Added 4-stage version of coord2ssaAIR
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15840 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-05 12:48:53 +00:00
9197eea89b Fixed a few errors and updated citations
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15838 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-04 17:10:33 +00:00
b682c8d98a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15837 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-04 17:08:10 +00:00
c7d3af81f1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15836 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-04 17:07:58 +00:00
8ded262792 sync with GHub
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15835 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-04 17:01:14 +00:00
7830537091 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15834 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-11-04 16:54:31 +00:00
e24fff05b3 Fixed a few things I forgot
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15833 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-03 00:26:41 +00:00
30e14c7f37 Added threebody tests for sw, tersoff, vashishta
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15832 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-03 00:16:18 +00:00
5ffdbc1a97 Edited some of the comments in the file headers
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15831 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-02 23:31:41 +00:00
639b22cd56 Updating docs for Kokkkos
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15830 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-01 15:22:44 +00:00
8e0b69478a Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15829 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-11-01 00:22:36 +00:00
dd296bf237 Improving performance of Kokkos ReaxFF
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15828 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-31 22:00:06 +00:00
8de4680898 Adding short neighbor lists
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15827 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-28 18:42:43 +00:00
ef4dc21c15 Adding short neighbor list to tersoff Kokkos from C. Trott
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15826 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-27 21:55:25 +00:00
ceff3565d6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15825 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-27 17:09:15 +00:00
41f666db52 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15823 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-27 15:32:57 +00:00
f2df16e0f0 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15822 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-27 15:32:53 +00:00
4475897049 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15821 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-27 15:32:32 +00:00
02ae428e37 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15820 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-27 15:28:59 +00:00
21887831ff git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15819 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-27 14:29:02 +00:00
7a13d54a0d Fixed typo in temperature formula
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15818 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-26 22:28:56 +00:00
01209d450c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15817 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-26 22:24:50 +00:00
bc250ab7b9 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15816 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-26 22:24:31 +00:00
0270a33ab4 Fixing clang compile error
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15815 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-26 20:28:23 +00:00
287c57daf4 Adding Kokkos error check
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15814 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-26 17:36:13 +00:00
7d3d315753 Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15813 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-26 16:46:30 +00:00
77fa5ee08d Fixing Kokkos bug
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15812 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-26 16:41:57 +00:00
0fd26f7b9d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15811 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 22:49:56 +00:00
f092df34d4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15810 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 22:49:20 +00:00
e517e5a5a5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15809 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 22:48:44 +00:00
79250a7916 Adding support for FixReaxCBonds and FixReaxCSpecies to the Kokkos ReaxFF
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15808 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-25 22:31:05 +00:00
3de6f5b9c3 Adding support for FixReaxCBonds and FixReaxCSpecies to the Kokkos ReaxFF
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15807 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-25 22:15:00 +00:00
b42db824da Adding support for FixReaxCBonds and FixReaxCBonds to the Kokkos ReaxFF
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15806 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-25 20:47:40 +00:00
c587a3106f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15805 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 19:26:35 +00:00
d7304c5843 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15804 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 16:55:25 +00:00
8ed519045f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15803 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 16:55:11 +00:00
18b452c9c2 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15802 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 16:55:06 +00:00
8770adf78a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15801 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 16:54:48 +00:00
2a07f06924 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15800 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-25 16:53:20 +00:00
bb78ea0248 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15799 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-25 16:33:34 +00:00
bfdaa09a72 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15798 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-25 15:47:44 +00:00
a1cb91486b git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15796 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-24 14:19:10 +00:00
b9fc540733 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15795 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-24 14:16:13 +00:00
c0b98f5299 Recommitting reverted change
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15794 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-19 19:02:08 +00:00
5d076bafea git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15792 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 17:03:39 +00:00
51e7c77aec git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15791 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 17:03:33 +00:00
8fa049edda git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15790 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 16:29:44 +00:00
218ab76d0b git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15789 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 16:27:17 +00:00
09a3a259c2 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15788 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 16:27:13 +00:00
aab7de9579 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15787 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-19 14:58:39 +00:00
616724091e git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15786 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 14:50:50 +00:00
252c52b9b8 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15785 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 14:43:54 +00:00
3089edfce1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15784 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 14:42:40 +00:00
82badf85a4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15783 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-19 14:42:24 +00:00
6d759f1b6f sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15782 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-19 14:39:50 +00:00
2babec1b38 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15780 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 19:09:14 +00:00
15dbceee76 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15779 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 19:09:11 +00:00
49f6e138e6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15778 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 19:04:11 +00:00
773aec0f1c sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15777 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-18 18:59:37 +00:00
a9b065ca3a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15776 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 17:14:54 +00:00
bc43acd4e9 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15775 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 17:10:29 +00:00
95ed575b66 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15774 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 15:40:09 +00:00
4f1ea743bd git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15773 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-18 15:39:51 +00:00
9a6dc87fa6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15772 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-17 15:41:42 +00:00
daf719470f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15771 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-14 14:36:10 +00:00
fdd61cf314 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15769 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-13 23:03:30 +00:00
3593ca7f48 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15768 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-13 23:03:27 +00:00
d58e86625b sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15767 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-13 23:01:03 +00:00
06fa6ce105 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15766 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-13 19:58:01 +00:00
c3c2587fef Added fix for problem with energy_full and shake
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15765 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-13 19:11:48 +00:00
115d67c1a0 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15764 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-13 19:07:38 +00:00
011568fae3 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15763 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-13 19:07:22 +00:00
0f1c56d0fc git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15762 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-13 19:04:21 +00:00
2f98f4ad98 Added fix for problem with energy_full and shake
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15761 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-13 18:56:05 +00:00
0145275cd2 Added fix for problem with energy_full and shake
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15760 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-13 18:52:26 +00:00
1ce8f1479e git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15759 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 23:39:29 +00:00
5661aea6d5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15758 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 23:39:17 +00:00
6ec1550081 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15757 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 21:13:30 +00:00
c660a813e4 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15756 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 20:52:53 +00:00
96eaa5d59f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15754 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 13:35:01 +00:00
409fe28ee9 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15753 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 13:34:58 +00:00
ab2998e4dd git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15752 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 13:34:48 +00:00
fb4cbf1a4a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15751 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-12 13:34:37 +00:00
1d501f05e4 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15750 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-12 13:32:56 +00:00
a6ceebf5b1 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15749 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 20:33:10 +00:00
338f6ae70a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15748 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 19:51:46 +00:00
7e37c5aecb sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15747 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-11 19:42:15 +00:00
e710053de6 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15746 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-11 18:43:51 +00:00
7a4da54a71 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15744 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 18:34:01 +00:00
d1145f14ee git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15743 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 18:33:59 +00:00
b195d32105 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15742 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 18:23:52 +00:00
66b073415b git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15741 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 18:23:09 +00:00
6888a80d7d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15740 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-11 18:20:53 +00:00
59215db1a3 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15739 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-10 20:02:41 +00:00
dcdb53cc79 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15737 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-10 19:40:11 +00:00
b31b4093ca Fixing Kokkos compile error
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15736 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-10 18:17:51 +00:00
c4ab7c8245 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15735 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-10 15:16:43 +00:00
c35d0d77e0 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15734 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 22:46:55 +00:00
fda969f1c9 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15733 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-06 21:50:57 +00:00
50ea9d151f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15731 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 21:41:42 +00:00
325aa50c67 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15730 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 21:41:40 +00:00
3b67310233 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15729 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 21:41:21 +00:00
5c8fb1d55c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15728 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 21:41:07 +00:00
94ebde04e3 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15722 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 21:06:14 +00:00
720c352a08 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15721 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 20:03:35 +00:00
65585e69a6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15720 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 20:03:13 +00:00
cd8d18dc71 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15719 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 20:01:30 +00:00
5bc562b095 Fixing Kokkos bugs
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15718 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-06 19:48:28 +00:00
2a52034786 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15717 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 19:17:50 +00:00
b35352153c sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15716 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-06 19:05:57 +00:00
4f01a3055a git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15715 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:59:16 +00:00
44ef94958c git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15714 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:46:54 +00:00
54413ce1b7 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15713 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:46:21 +00:00
2d6f118846 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15712 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:44:52 +00:00
47b3de2554 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15711 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:44:36 +00:00
e51650664f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15710 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:43:25 +00:00
df0694e4e5 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15709 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:43:06 +00:00
a227a63ddb git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15708 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:42:51 +00:00
3f7821ba1f git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15707 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:09:53 +00:00
2a93bca2a6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15706 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:09:45 +00:00
f9ff3bd0bd git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15705 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:08:43 +00:00
9327eb756d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15704 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-06 18:03:27 +00:00
8a8c9fa8e8 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15701 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 21:41:11 +00:00
f4948ad5ff git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15700 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 21:03:06 +00:00
f86f711115 python lib callback issue fixed
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15699 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-05 16:55:23 +00:00
26da91a157 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15698 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 16:32:33 +00:00
82cac1a0e6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15697 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 15:43:36 +00:00
ce665801ea git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15696 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 15:43:33 +00:00
28f88a6085 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15695 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 15:39:31 +00:00
44a8d082e8 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15694 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 15:32:07 +00:00
998c5b7d2d git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15693 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-05 15:07:50 +00:00
05c027fcaf git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15692 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-04 15:11:27 +00:00
57dfa51b97 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15691 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-10-04 00:00:38 +00:00
dc2bd269d6 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15690 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-03 23:56:44 +00:00
d86416aee3 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15689 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-03 23:56:06 +00:00
58f1297b61 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15688 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-10-03 22:23:47 +00:00
87540fbac0 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15684 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-09-30 15:25:09 +00:00
0311121190 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15683 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-09-30 15:25:07 +00:00
49e66858ab sync with GH: colvars update, add forgotten CMAP potential files
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15682 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-09-30 15:22:12 +00:00
40ec180798 git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15681 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-09-30 15:16:16 +00:00
bcd4dad2f1 sync with GH
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15680 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-09-29 21:52:57 +00:00
f60331a5fb git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15678 f3b2605a-c512-4ea7-a41b-209d697bcdaa 2016-09-29 20:32:11 +00:00
d7bb53e4d2 Fixing Kokkos bug and adding host version of CommTiled
git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@15676 f3b2605a-c512-4ea7-a41b-209d697bcdaa
2016-09-29 20:21:39 +00:00
1444 changed files with 63828 additions and 337575 deletions

34
.gitignore vendored
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@ -1,34 +0,0 @@
*~
*.o
*.so
*.cu_o
*.ptx
*_ptx.h
*.a
*.d
*.x
*.exe
*.dll
*.pyc
__pycache__
Obj_*
log.lammps
log.cite
*.bz2
*.gz
*.tar
.*.swp
*.orig
*.rej
.vagrant
\#*#
.#*
.DS_Store
.DS_Store?
._*
.Spotlight-V100
.Trashes
ehthumbs.db
Thumbs.db

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@ -14,7 +14,7 @@ lmp_linux_mixed
lmp_linux_double
The precision (single, mixed, double) refers to the GPU and USER-CUDA
package precision. See the README files in the lib/gpu and lib/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.

6
doc/.gitignore vendored
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@ -1,6 +0,0 @@
/html
/spelling
/LAMMPS.epub
/LAMMPS.mobi
/Manual.pdf
/Developer.pdf

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@ -6,7 +6,6 @@ BUILDDIR = /tmp/lammps-docs-$(SHA1)
RSTDIR = $(BUILDDIR)/rst
VENV = $(BUILDDIR)/docenv
TXT2RST = $(VENV)/bin/txt2rst
ANCHORCHECK = $(VENV)/bin/doc_anchor_check
PYTHON = $(shell which python3)
HAS_PYTHON3 = NO
@ -23,7 +22,7 @@ endif
SOURCES=$(wildcard src/*.txt)
OBJECTS=$(SOURCES:src/%.txt=$(RSTDIR)/%.rst)
.PHONY: help clean-all clean epub html pdf old venv spelling anchor_check
.PHONY: help clean-all clean epub html pdf old venv
# ------------------------------------------
@ -37,7 +36,6 @@ help:
@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"
# ------------------------------------------
@ -46,19 +44,12 @@ clean-all:
clean:
rm -rf $(RSTDIR) html
rm -rf spelling
clean-spelling:
rm -rf spelling
html: $(OBJECTS) $(ANCHORCHECK)
html: $(OBJECTS)
@(\
. $(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
@ -73,17 +64,6 @@ html: $(OBJECTS) $(ANCHORCHECK)
@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
@ -132,13 +112,6 @@ 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
@ -163,7 +136,7 @@ $(VENV):
deactivate;\
)
$(TXT2RST) $(ANCHORCHECK): $(VENV)
$(TXT2RST): $(VENV)
@( \
. $(VENV)/bin/activate; \
(cd utils/converters;\

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@ -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 parameter of
the cluster are of a bondtype specified by the 2nd paramter 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 constraints will be
an atom can be assigned to multiple constraints, the contraints 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" command to initialize velocities of atoms
used with "create temp" commmand 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" constraints on
the minimizer does not invoke the "fix style shake" contraints 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
specified mesh size will override the default
specifed 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; command)
allows program to restart from where it left off (see &quot;read restart&quot; commmand)
Default = 0
</PRE>

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@ -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 constraint
2-d flow of Lennard-Jones atoms in a channel using various contraint
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 specifies how many
examples/polymer for two sample def files) that specfies how many
chains of what length, a random number seed, etc.</P>
</BODY>
</HTML>

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@ -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 processor
maxbond = max # of bonds to compute on one procesor
<LI>
maxangle = max # of angles to compute on one processor
<LI>

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@ -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 &quot;fix style&quot; command
multiple groups of atoms can be assigned to the same constraint
an atom can be assigned to multiple constraints, the constraints will be
an atom can be assigned to multiple constraints, the contraints 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 &quot;create temp&quot; command to initialize velocities of atoms
used with &quot;create temp&quot; commmand to initialize velocities of atoms
by default, the &quot;create temp&quot; 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 &quot;create temp&quot; 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
specified mesh size will override the default
specifed 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; command)
allows program to restart from where it left off (see &quot;read restart&quot; commmand)
Default = 0
</PRE>

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

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

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

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@ -1,13 +0,0 @@
\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}

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@ -1,13 +0,0 @@
\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}

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@ -1,7 +1,7 @@
<!-- HTML_ONLY -->
<HEAD>
<TITLE>LAMMPS Users Manual</TITLE>
<META NAME="docnumber" CONTENT="11 Apr 2017 version">
<META NAME="docnumber" CONTENT="26 Jan 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 Apr 2017 version :c,h4
26 Jan 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 [development] version of LAMMPS. :ulb,l
describe the most current 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, stamoor at sandia.gov :l
Stan Moore, stamoore at sandia.gov :l
"Axel Kohlmeyer"_ako, akohlmey at gmail.com :l
:ule

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@ -281,12 +281,12 @@ the "minimize"_minimize.html command. A parallel tempering
3.4 Commands listed by category :link(cmd_4),h4
This section lists core LAMMPS commands, grouped by category.
The "next section"_#cmd_5 lists all commands alphabetically. The
This section lists all LAMMPS commands, grouped by category. The
"next section"_#cmd_5 lists the same 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.
included in these categories, but they are in the next section.
Initialization:
@ -361,7 +361,7 @@ Settings:
"timer"_timer.html,
"timestep"_timestep.html
Operations within timestepping (fixes) and diagnostics (computes):
Operations within timestepping (fixes) and diagnositics (computes):
"compute"_compute.html,
"compute_modify"_compute_modify.html,
@ -687,7 +687,6 @@ package"_Section_start.html#start_3.
"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,
@ -940,8 +939,6 @@ 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,
@ -972,7 +969,7 @@ KOKKOS, o = USER-OMP, t = OPT.
"lubricateU/poly"_pair_lubricateU.html,
"meam"_pair_meam.html,
"mie/cut (o)"_pair_mie.html,
"morse (gkot)"_pair_morse.html,
"morse (got)"_pair_morse.html,
"nb3b/harmonic (o)"_pair_nb3b_harmonic.html,
"nm/cut (o)"_pair_nm.html,
"nm/cut/coul/cut (o)"_pair_nm.html,
@ -1019,7 +1016,6 @@ package"_Section_start.html#start_3.
"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,
@ -1037,7 +1033,6 @@ package"_Section_start.html#start_3.
"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,
@ -1047,10 +1042,6 @@ package"_Section_start.html#start_3.
"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,
"smd/hertz"_pair_smd_hertz.html,
@ -1068,7 +1059,7 @@ package"_Section_start.html#start_3.
"table/rx"_pair_table_rx.html,
"tersoff/table (o)"_pair_tersoff.html,
"thole"_pair_thole.html,
"tip4p/long/soft (o)"_pair_lj_soft.html :tb(c=4,ea=c)
"tip4p/long/soft (o)"_pair_lj_soft.html :tb(c=4,ea=c)
:line
@ -1085,7 +1076,7 @@ KOKKOS, o = USER-OMP, t = OPT.
"none"_bond_none.html,
"zero"_bond_zero.html,
"hybrid"_bond_hybrid.html,
"class2 (ko)"_bond_class2.html,
"class2 (o)"_bond_class2.html,
"fene (iko)"_bond_fene.html,
"fene/expand (o)"_bond_fene_expand.html,
"harmonic (ko)"_bond_harmonic.html,
@ -1100,8 +1091,7 @@ package"_Section_start.html#start_3.
"harmonic/shift (o)"_bond_harmonic_shift.html,
"harmonic/shift/cut (o)"_bond_harmonic_shift_cut.html,
"oxdna/fene"_bond_oxdna.html,
"oxdna2/fene"_bond_oxdna.html :tb(c=4,ea=c)
"oxdna/fene"_bond_oxdna_fene.html :tb(c=4,ea=c)
:line
@ -1119,7 +1109,7 @@ USER-OMP, t = OPT.
"zero"_angle_zero.html,
"hybrid"_angle_hybrid.html,
"charmm (ko)"_angle_charmm.html,
"class2 (ko)"_angle_class2.html,
"class2 (o)"_angle_class2.html,
"cosine (o)"_angle_cosine.html,
"cosine/delta (o)"_angle_cosine_delta.html,
"cosine/periodic (o)"_angle_cosine_periodic.html,
@ -1155,8 +1145,7 @@ USER-OMP, t = OPT.
"zero"_dihedral_zero.html,
"hybrid"_dihedral_hybrid.html,
"charmm (ko)"_dihedral_charmm.html,
"charmmfsw"_dihedral_charmm.html,
"class2 (ko)"_dihedral_class2.html,
"class2 (o)"_dihedral_class2.html,
"harmonic (io)"_dihedral_harmonic.html,
"helix (o)"_dihedral_helix.html,
"multi/harmonic (o)"_dihedral_multi_harmonic.html,
@ -1188,7 +1177,7 @@ USER-OMP, t = OPT.
"none"_improper_none.html,
"zero"_improper_zero.html,
"hybrid"_improper_hybrid.html,
"class2 (ko)"_improper_class2.html,
"class2 (o)"_improper_class2.html,
"cvff (io)"_improper_cvff.html,
"harmonic (ko)"_improper_harmonic.html,
"umbrella (o)"_improper_umbrella.html :tb(c=4,ea=c)

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@ -22,7 +22,7 @@ either conceptually, or as printed out by the program.
12.1 Common problems :link(err_1),h4
If two LAMMPS runs do not produce the exact same answer on different
If two LAMMPS runs do not produce the same answer on different
machines or different numbers of processors, this is typically not a
bug. In theory you should get identical answers on any number of
processors and on any machine. In practice, numerical round-off can
@ -80,24 +80,12 @@ order. If you mess this up, LAMMPS will often flag the error, but it
may also simply read a bogus argument and assign a value that is
valid, but not what you wanted. E.g. trying to read the string "abc"
as an integer value of 0. Careful reading of the associated doc page
for the command should allow you to fix these problems. In most cases,
where LAMMPS expects to read a number, either integer or floating point,
it performs a stringent test on whether the provided input actually
is an integer or floating-point number, respectively, and reject the
input with an error message (for instance, when an integer is required,
but a floating-point number 1.0 is provided):
ERROR: Expected integer parameter in input script or data file :pre
Some commands allow for using variable references in place of numeric
constants so that the value can be evaluated and may change over the
course of a run. This is typically done with the syntax {v_name} for a
parameter, where name is the name of the variable. On the other hand,
immediate variable expansion with the syntax ${name} is performed while
reading the input and before parsing commands,
NOTE: Using a variable reference (i.e. {v_name}) is only allowed if
the documentation of the corresponding command explicitly says it is.
for the command should allow you to fix these problems. Note that
some commands allow for variables to be specified in place of numeric
constants so that the value can be evaluated and change over the
course of a run. This is typically done with the syntax {v_name} for
a parameter, where name is the name of the variable. This is only
allowed if the command documentation says it is.
Generally, LAMMPS will print a message to the screen and logfile and
exit gracefully when it encounters a fatal error. Sometimes it will
@ -574,11 +562,11 @@ group of atoms correctly. :dd
{Bad quadratic solve for particle/line collision} :dt
This is an internal error. It should normally not occur. :dd
This is an internal error. It should nornally not occur. :dd
{Bad quadratic solve for particle/tri collision} :dt
This is an internal error. It should normally not occur. :dd
This is an internal error. It should nornally not occur. :dd
{Bad real space Coulomb cutoff in fix tune/kspace} :dt
@ -912,7 +900,7 @@ Atoms can not be added afterwards to this fix option. :dd
{Cannot append atoms to a triclinic box} :dt
The simulation box must be defined with edges aligned with the
The simulation box must be defined with edges alligned with the
Cartesian axes. :dd
{Cannot balance in z dimension for 2d simulation} :dt
@ -992,7 +980,7 @@ file. :dd
LAMMPS failed to compute an initial guess for the PPPM_disp g_ewald_6
factor that partitions the computation between real space and k-space
for Dispersion interactions. :dd
for Disptersion interactions. :dd
{Cannot create an atom map unless atoms have IDs} :dt
@ -1327,7 +1315,7 @@ Self-explanatory. :dd
This file is created when you use some LAMMPS features, to indicate
what paper you should cite on behalf of those who implemented
the feature. Check that you have write privileges into the directory
the feature. Check that you have write priveleges into the directory
you are running in. :dd
{Cannot open log.lammps for writing} :dt
@ -2005,7 +1993,7 @@ Self-explanatory. :dd
{Cannot use fix reax/bonds without pair_style reax} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Cannot use fix rigid npt/nph and fix deform on same component of stress tensor} :dt
@ -2088,7 +2076,7 @@ Self-explanatory. :dd
{Cannot use lines with fix srd unless overlap is set} :dt
This is because line segments are connected to each other. :dd
This is because line segements are connected to each other. :dd
{Cannot use multiple fix wall commands with pair brownian} :dt
@ -2131,7 +2119,7 @@ Self-explanatory. :dd
{Cannot use newton pair with born/gpu pair style} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Cannot use newton pair with buck/coul/cut/gpu pair style} :dt
@ -2291,7 +2279,7 @@ Self-explanatory. :dd
{Cannot use newton pair with zbl/gpu pair style} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Cannot use non-zero forces in an energy minimization} :dt
@ -2641,11 +2629,11 @@ uses a pairwise neighbor list. :dd
{Compute chunk/atom bin/cylinder radius is too large for periodic box} :dt
Radius cannot be bigger than 1/2 of a non-axis periodic dimension. :dd
Radius cannot be bigger than 1/2 of a non-axis periodic dimention. :dd
{Compute chunk/atom bin/sphere radius is too large for periodic box} :dt
Radius cannot be bigger than 1/2 of any periodic dimension. :dd
Radius cannot be bigger than 1/2 of any periodic dimention. :dd
{Compute chunk/atom compute array is accessed out-of-range} :dt
@ -2706,15 +2694,15 @@ It will only store IDs if its compress option is enabled. :dd
{Compute chunk/atom stores no coord1 for compute property/chunk} :dt
Only certain binning options for compute chunk/atom store coordinates. :dd
Only certain binning options for comptue chunk/atom store coordinates. :dd
{Compute chunk/atom stores no coord2 for compute property/chunk} :dt
Only certain binning options for compute chunk/atom store coordinates. :dd
Only certain binning options for comptue chunk/atom store coordinates. :dd
{Compute chunk/atom stores no coord3 for compute property/chunk} :dt
Only certain binning options for compute chunk/atom store coordinates. :dd
Only certain binning options for comptue chunk/atom store coordinates. :dd
{Compute chunk/atom variable is not atom-style variable} :dt
@ -2735,11 +2723,11 @@ is used to find clusters. :dd
{Compute cna/atom cutoff is longer than pairwise cutoff} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Compute cna/atom requires a pair style be defined} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Compute com/chunk does not use chunk/atom compute} :dt
@ -2747,7 +2735,7 @@ The style of the specified compute is not chunk/atom. :dd
{Compute contact/atom requires a pair style be defined} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Compute contact/atom requires atom style sphere} :dt
@ -2760,7 +2748,7 @@ since those atoms are not in the neighbor list. :dd
{Compute coord/atom requires a pair style be defined} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Compute damage/atom requires peridynamic potential} :dt
@ -2790,7 +2778,7 @@ Self-explanatory. :dd
{Compute erotate/asphere requires extended particles} :dt
This compute cannot be used with point particles. :dd
This compute cannot be used with point paritlces. :dd
{Compute erotate/rigid with non-rigid fix-ID} :dt
@ -2835,7 +2823,7 @@ Cannot compute order parameter beyond cutoff. :dd
{Compute hexorder/atom requires a pair style be defined} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Compute improper/local used when impropers are not allowed} :dt
@ -2881,11 +2869,11 @@ Cannot compute order parameter beyond cutoff. :dd
{Compute orientorder/atom requires a pair style be defined} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Compute pair must use group all} :dt
Pair styles accumulate energy on all atoms. :dd
Pair styles accumlate energy on all atoms. :dd
{Compute pe must use group all} :dt
@ -2935,7 +2923,7 @@ The style of the specified compute is not chunk/atom. :dd
{Compute property/local cannot use these inputs together} :dt
Only inputs that generate the same number of datums can be used
together. E.g. bond and angle quantities cannot be mixed. :dd
togther. E.g. bond and angle quantities cannot be mixed. :dd
{Compute property/local does not (yet) work with atom_style template} :dt
@ -3079,7 +3067,7 @@ Self-explanatory. :dd
{Compute temp/asphere requires extended particles} :dt
This compute cannot be used with point particles. :dd
This compute cannot be used with point paritlces. :dd
{Compute temp/body requires atom style body} :dt
@ -3524,12 +3512,12 @@ path and name are correct. :dd
{Could not process Python file} :dt
The Python code in the specified file was not run successfully by
The Python code in the specified file was not run sucessfully by
Python, probably due to errors in the Python code. :dd
{Could not process Python string} :dt
The Python code in the here string was not run successfully by Python,
The Python code in the here string was not run sucessfully by Python,
probably due to errors in the Python code. :dd
{Coulomb PPPMDisp order has been reduced below minorder} :dt
@ -3638,7 +3626,7 @@ Self-explanatory. :dd
{Cutoffs missing in pair_style buck/long/coul/long} :dt
Self-explanatory. :dd
Self-exlanatory. :dd
{Cutoffs missing in pair_style lj/long/coul/long} :dt
@ -4385,7 +4373,7 @@ Self-explanatory. :dd
{Fix ave/chunk does not use chunk/atom compute} :dt
The specified compute is not for a compute chunk/atom command. :dd
The specified conpute is not for a compute chunk/atom command. :dd
{Fix ave/chunk fix does not calculate a per-atom array} :dt
@ -4617,11 +4605,11 @@ An index for the array is out of bounds. :dd
{Fix ave/time compute does not calculate a scalar} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Fix ave/time compute does not calculate a vector} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Fix ave/time compute does not calculate an array} :dt
@ -4970,7 +4958,7 @@ Self-explanatory. :dd
{Fix langevin angmom requires extended particles} :dt
This fix option cannot be used with point particles. :dd
This fix option cannot be used with point paritlces. :dd
{Fix langevin omega is not yet implemented with kokkos} :dt
@ -6171,7 +6159,7 @@ map command will force an atom map to be created. :dd
{Initial temperatures not all set in fix ttm} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Input line quote not followed by whitespace} :dt
@ -6199,7 +6187,7 @@ Eigensolve for rigid body was not sufficiently accurate. :dd
{Insufficient Jacobi rotations for triangle} :dt
The calculation of the inertia tensor of the triangle failed. This
The calculation of the intertia tensor of the triangle failed. This
should not happen if it is a reasonably shaped triangle. :dd
{Insufficient memory on accelerator} :dt
@ -6463,15 +6451,15 @@ Self-explanatory. :dd
{Invalid attribute in dump custom command} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Invalid attribute in dump local command} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Invalid attribute in dump modify command} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Invalid basis setting in create_atoms command} :dt
@ -6737,7 +6725,7 @@ or cause multiple files to be written. :dd
Filenames used with the dump xyz style cannot be binary or cause files
to be written by each processor. :dd
{Invalid dump_modify threshold operator} :dt
{Invalid dump_modify threshhold operator} :dt
Operator keyword used for threshold specification in not recognized. :dd
@ -6751,7 +6739,7 @@ The fix is not recognized. :dd
{Invalid fix ave/time off column} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Invalid fix box/relax command for a 2d simulation} :dt
@ -7313,7 +7301,7 @@ Self-explanatory. Check the input script or data file. :dd
{LJ6 off not supported in pair_style buck/long/coul/long} :dt
Self-explanatory. :dd
Self-exlanatory. :dd
{Label wasn't found in input script} :dt
@ -7361,7 +7349,7 @@ This should not occur. Report the problem to the developers. :dd
Lost atoms are checked for each time thermo output is done. See the
thermo_modify lost command for options. Lost atoms usually indicate
bad dynamics, e.g. atoms have been blown far out of the simulation
box, or moved further than one processor's sub-domain away before
box, or moved futher than one processor's sub-domain away before
reneighboring. :dd
{MEAM library error %d} :dt
@ -7526,7 +7514,7 @@ Self-explanatory. :dd
{Molecule template ID for create_atoms does not exist} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Molecule template ID for fix deposit does not exist} :dt
@ -7552,7 +7540,7 @@ Self-explanatory. :dd
Self-explanatory. :dd
{Molecule topology/atom exceeds system topology/atom} :dt
{Molecule toplogy/atom exceeds system topology/atom} :dt
The number of bonds, angles, etc per-atom in the molecule exceeds the
system setting. See the create_box command for how to specify these
@ -7792,7 +7780,7 @@ Self-explanatory. :dd
{Must use variable energy with fix addforce} :dt
Must define an energy variable when applying a dynamic
Must define an energy vartiable when applyting a dynamic
force during minimization. :dd
{Must use variable energy with fix efield} :dt
@ -8042,7 +8030,7 @@ Self-explanatory. :dd
{Non digit character between brackets in variable} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Non integer # of swaps in temper command} :dt
@ -8663,7 +8651,7 @@ not be invoked by bond_style quartic. :dd
{Pair style does not support compute group/group} :dt
The pair_style does not have a single() function, so it cannot be
invoked by the compute group/group command. :dd
invokded by the compute group/group command. :dd
{Pair style does not support compute pair/local} :dt
@ -8948,11 +8936,11 @@ Self-explanatory. :dd
{Pair yukawa/colloid requires atom style sphere} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Pair yukawa/colloid requires atoms with same type have same radius} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Pair yukawa/colloid/gpu requires atom style sphere} :dt
@ -9166,7 +9154,7 @@ Self-explanatory. :dd
{Python function evaluation failed} :dt
The Python function did not run successfully and/or did not return a
The Python function did not run succesfully and/or did not return a
value (if it is supposed to return a value). This is probably due to
some error condition in the function. :dd
@ -10025,7 +10013,7 @@ make sense in between runs. :dd
{Threshhold for an atom property that isn't allocated} :dt
A dump threshold has been requested on a quantity that is
A dump threshhold has been requested on a quantity that is
not defined by the atom style used in this simulation. :dd
{Timestep must be >= 0} :dt
@ -10087,7 +10075,7 @@ to a large size. :dd
{Too many atom triplets for pair bop} :dt
The number of three atom groups for angle determinations exceeds the
expected number. Check your atomic structure to ensure that it is
expected number. Check your atomic structrure to ensure that it is
realistic. :dd
{Too many atoms for dump dcd} :dt
@ -10155,7 +10143,7 @@ to a large size. :dd
{Too many timesteps} :dt
The cumulative timesteps must fit in a 64-bit integer. :dd
The cummulative timesteps must fit in a 64-bit integer. :dd
{Too many timesteps for NEB} :dt
@ -10654,7 +10642,7 @@ Only atom-style variables can be used. :dd
{Variable for region cylinder is invalid style} :dt
Only equal-style variables are allowed. :dd
Only equal-style varaibles are allowed. :dd
{Variable for region is invalid style} :dt
@ -10666,7 +10654,7 @@ Self-explanatory. :dd
{Variable for region sphere is invalid style} :dt
Only equal-style variables are allowed. :dd
Only equal-style varaibles are allowed. :dd
{Variable for restart is invalid style} :dt
@ -10707,7 +10695,7 @@ Self-explanatory. :dd
{Variable has circular dependency} :dt
A circular dependency is when variable "a" in used by variable "b" and
variable "b" is also used by variable "a". Circular dependencies with
variable "b" is also used by varaible "a". Circular dependencies with
longer chains of dependence are also not allowed. :dd
{Variable name between brackets must be alphanumeric or underscore characters} :dt
@ -10796,7 +10784,7 @@ Self-explanatory. :dd
{Variable name for fix deform does not exist} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Variable name for fix efield does not exist} :dt
@ -11083,7 +11071,7 @@ for a dihedral) and adding a small amount of stretch. :dd
{Both groups in compute group/group have a net charge; the Kspace boundary correction to energy will be non-zero} :dt
Self-explanatory. :dd
Self-explantory. :dd
{Calling write_dump before a full system init.} :dt
@ -11414,7 +11402,7 @@ The command options you have used caused atoms to be lost. :dd
Lost atoms are checked for each time thermo output is done. See the
thermo_modify lost command for options. Lost atoms usually indicate
bad dynamics, e.g. atoms have been blown far out of the simulation
box, or moved further than one processor's sub-domain away before
box, or moved futher than one processor's sub-domain away before
reneighboring. :dd
{MSM mesh too small, increasing to 2 points in each direction} :dt
@ -11452,7 +11440,7 @@ i.e. the first molecule in the template. :dd
{Molecule template for fix shake has multiple molecules} :dt
The fix shake command will only recognize molecules of a single
The fix shake command will only recoginze molecules of a single
type, i.e. the first molecule in the template. :dd
{More than one compute centro/atom} :dt
@ -11537,7 +11525,7 @@ neigh_modify exclude command. :dd
If a thermo_style command is used after a thermo_modify command, the
settings changed by the thermo_modify command will be reset to their
default values. This is because the thermo_modify command acts on
default values. This is because the thermo_modify commmand acts on
the currently defined thermo style, and a thermo_style command creates
a new style. :dd
@ -11589,7 +11577,7 @@ This may not be what you intended. :dd
{One or more dynamic groups may not be updated at correct point in timestep} :dt
If there are other fixes that act immediately after the initial stage
If there are other fixes that act immediately after the intitial stage
of time integration within a timestep (i.e. after atoms move), then
the command that sets up the dynamic group should appear after those
fixes. This will insure that dynamic group assignments are made
@ -11886,7 +11874,7 @@ Self-explanatory. :dd
{Using largest cutoff for buck/long/coul/long} :dt
Self-explanatory. :dd
Self-exlanatory. :dd
{Using largest cutoff for lj/long/coul/long} :dt

View File

@ -25,7 +25,9 @@ files and image files.
If you uncomment the "dump"_dump.html command in the input script, a
text dump file will be produced, which can be animated by various
"visualization programs"_http://lammps.sandia.gov/viz.html.
"visualization programs"_http://lammps.sandia.gov/viz.html. It can
also be animated using the xmovie tool described in the "Additional
Tools"_Section_tools.html section of the LAMMPS documentation.
If you uncomment the "dump image"_dump.html command in the input
script, and assuming you have built LAMMPS with a JPG library, JPG
@ -51,11 +53,9 @@ Lowercase directories :h4
accelerate: run with various acceleration options (OpenMP, GPU, Phi)
balance: dynamic load balancing, 2d system
body: body particles, 2d system
cmap: CMAP 5-body contributions to CHARMM force field
colloid: big colloid particles in a small particle solvent, 2d system
comb: models using the COMB potential
coreshell: core/shell model using CORESHELL package
controller: use of fix controller as a thermostat
crack: crack propagation in a 2d solid
deposit: deposit atoms and molecules on a surface
dipole: point dipolar particles, 2d system
@ -64,8 +64,6 @@ eim: NaCl using the EIM potential
ellipse: ellipsoidal particles in spherical solvent, 2d system
flow: Couette and Poiseuille flow in a 2d channel
friction: frictional contact of spherical asperities between 2d surfaces
gcmc: Grand Canonical Monte Carlo (GCMC) via the fix gcmc command
granregion: use of fix wall/region/gran as boundary on granular particles
hugoniostat: Hugoniostat shock dynamics
indent: spherical indenter into a 2d solid
kim: use of potentials in Knowledge Base for Interatomic Models (KIM)
@ -73,7 +71,6 @@ meam: MEAM test for SiC and shear (same as shear examples)
melt: rapid melt of 3d LJ system
micelle: self-assembly of small lipid-like molecules into 2d bilayers
min: energy minimization of 2d LJ melt
mscg: parameterize a multi-scale coarse-graining (MSCG) model
msst: MSST shock dynamics
nb3b: use of nonbonded 3-body harmonic pair style
neb: nudged elastic band (NEB) calculation for barrier finding
@ -92,8 +89,7 @@ snap: NVE dynamics for BCC tantalum crystal using SNAP potential
srd: stochastic rotation dynamics (SRD) particles as solvent
streitz: use of Streitz/Mintmire potential with charge equilibration
tad: temperature-accelerated dynamics of vacancy diffusion in bulk Si
vashishta: use of the Vashishta potential
voronoi: Voronoi tesselation via compute voronoi/atom command :tb(s=:)
vashishta: use of the Vashishta potential :tb(s=:)
Here is how you can run and visualize one of the sample problems:

View File

@ -37,7 +37,7 @@ pitfalls or alternatives.
Please see some of the closed issues for examples of how to
suggest code enhancements, submit proposed changes, or report
possible bugs and how they are resolved.
possible bugs and how they are resoved.
As an alternative to using GitHub, you may e-mail the
"core developers"_http://lammps.sandia.gov/authors.html or send

View File

@ -165,16 +165,9 @@ Many of the example input scripts included in the LAMMPS distribution
are for 2d models.
NOTE: Some models in LAMMPS treat particles as finite-size spheres, as
opposed to point particles. See the "atom_style
sphere"_atom_style.html and "fix nve/sphere"_fix_nve_sphere.html
commands for details. By default, for 2d simulations, such particles
will still be modeled as 3d spheres, not 2d discs (circles), meaning
their moment of inertia will be that of a sphere. If you wish to
model them as 2d discs, see the "set density/disc"_set.html command
and the {disc} option for the "fix nve/sphere"_fix_nve_sphere.html,
"fix nvt/sphere"_fix_nvt_sphere.html, "fix
nph/sphere"_fix_nph_sphere.html, "fix npt/sphere"_fix_npt_sphere.html
commands.
opposed to point particles. In 2d, the particles will still be
spheres, not disks, meaning their moment of inertia will be the same
as in 3d.
:line
@ -204,10 +197,7 @@ documentation for the formula it computes.
"bond_style"_bond_harmonic.html harmonic
"angle_style"_angle_charmm.html charmm
"dihedral_style"_dihedral_charmm.html charmmfsh
"dihedral_style"_dihedral_charmm.html charmm
"pair_style"_pair_charmm.html lj/charmmfsw/coul/charmmfsh
"pair_style"_pair_charmm.html lj/charmmfsw/coul/long
"pair_style"_pair_charmm.html lj/charmm/coul/charmm
"pair_style"_pair_charmm.html lj/charmm/coul/charmm/implicit
"pair_style"_pair_charmm.html lj/charmm/coul/long :ul
@ -215,12 +205,6 @@ documentation for the formula it computes.
"special_bonds"_special_bonds.html charmm
"special_bonds"_special_bonds.html amber :ul
NOTE: For CHARMM, newer {charmmfsw} or {charmmfsh} styles were
released in March 2017. We recommend they be used instead of the
older {charmm} styles. See discussion of the differences on the "pair
charmm"_pair_charmm.html and "dihedral charmm"_dihedral_charmm.html
doc pages.
DREIDING is a generic force field developed by the "Goddard
group"_http://www.wag.caltech.edu at Caltech and is useful for
predicting structures and dynamics of organic, biological and
@ -450,12 +434,6 @@ computations between frozen atoms by using this command:
"neigh_modify"_neigh_modify.html exclude :ul
NOTE: By default, for 2d systems, granular particles are still modeled
as 3d spheres, not 2d discs (circles), meaning their moment of inertia
will be the same as in 3d. If you wish to model granular particles in
2d as 2d discs, see the note on this topic in "Section
6.2"_Section_howto.html#howto_2, where 2d simulations are disussed.
:line
6.7 TIP3P water model :link(howto_7),h4
@ -473,7 +451,7 @@ atoms and the water molecule to run a rigid TIP3P-CHARMM model with a
cutoff. The K values can be used if a flexible TIP3P model (without
fix shake) is desired. If the LJ epsilon and sigma for HH and OH are
set to 0.0, it corresponds to the original 1983 TIP3P model
"(Jorgensen)"_#Jorgensen1.
"(Jorgensen)"_#Jorgensen.
O mass = 15.9994
H mass = 1.008
@ -491,7 +469,7 @@ K of HOH angle = 55
theta of HOH angle = 104.52 :all(b),p
These are the parameters to use for TIP3P with a long-range Coulombic
solver (e.g. Ewald or PPPM in LAMMPS), see "(Price)"_#Price1 for
solver (e.g. Ewald or PPPM in LAMMPS), see "(Price)"_#Price for
details:
O mass = 15.9994
@ -535,7 +513,7 @@ using the "fix shake"_fix_shake.html command.
These are the additional parameters (in real units) to set for O and H
atoms and the water molecule to run a rigid TIP4P model with a cutoff
"(Jorgensen)"_#Jorgensen1. Note that the OM distance is specified in
"(Jorgensen)"_#Jorgensen. Note that the OM distance is specified in
the "pair_style"_pair_style.html command, not as part of the pair
coefficients.
@ -595,7 +573,7 @@ LJ epsilon of O-O = 0.16275
LJ sigma of O-O = 3.16435
LJ epsilon, sigma of OH, HH = 0.0 :all(b),p
Note that the when using the TIP4P pair style, the neighbor list
Note that the when using the TIP4P pair style, the neighobr list
cutoff for Coulomb interactions is effectively extended by a distance
2 * (OM distance), to account for the offset distance of the
fictitious charges on O atoms in water molecules. Thus it is
@ -640,7 +618,7 @@ any of the parameters above, though it becomes a different model in
that mode of usage.
The SPC/E (extended) water model is the same, except
the partial charge assignments change:
the partial charge assignemnts change:
O charge = -0.8476
H charge = 0.4238 :all(b),p
@ -759,14 +737,23 @@ LAMMPS itself does not do visualization, but snapshots from LAMMPS
simulations can be visualized (and analyzed) in a variety of ways.
LAMMPS snapshots are created by the "dump"_dump.html command which can
create files in several formats. The native LAMMPS dump format is a
create files in several formats. The native LAMMPS dump format is a
text file (see "dump atom" or "dump custom") which can be visualized
by several popular visualization tools. The "dump image"_dump_image.html
and "dump movie"_dump_image.html styles can output internally rendered
images and convert a sequence of them to a movie during the MD run.
by the "xmovie"_Section_tools.html#xmovie program, included with the
LAMMPS package. This produces simple, fast 2d projections of 3d
systems, and can be useful for rapid debugging of simulation geometry
and atom trajectories.
Several programs included with LAMMPS as auxiliary tools can convert
between LAMMPS format files and other formats.
See the "Section 9"_Section_tools.html doc page for details.
native LAMMPS dump files to other formats. See the
"Section 9"_Section_tools.html doc page for details. The first is
the "ch2lmp tool"_Section_tools.html#charmm, which contains a
lammps2pdb Perl script which converts LAMMPS dump files into PDB
files. The second is the "lmp2arc tool"_Section_tools.html#arc which
converts LAMMPS dump files into Accelrys' Insight MD program files.
The third is the "lmp2cfg tool"_Section_tools.html#cfg which converts
LAMMPS dump files into CFG files which can be read into the
"AtomEye"_atomeye visualizer.
A Python-based toolkit distributed by our group can read native LAMMPS
dump files, including custom dump files with additional columns of
@ -779,7 +766,22 @@ RasMol visualization programs. Pizza.py has tools that do interactive
3d OpenGL visualization and one that creates SVG images of dump file
snapshots.
LAMMPS can create XYZ files directly (via "dump xyz") which is a
simple text-based file format used by many visualization programs
including "VMD"_vmd.
LAMMPS can create DCD files directly (via "dump dcd") which can be
read by "VMD"_vmd in conjunction with a CHARMM PSF file. Using this
form of output avoids the need to convert LAMMPS snapshots to PDB
files. See the "dump"_dump.html command for more information on DCD
files.
LAMMPS can create XTC files directly (via "dump xtc") which is GROMACS
file format which can also be read by "VMD"_vmd for visualization.
See the "dump"_dump.html command for more information on XTC files.
:link(pizza,http://www.sandia.gov/~sjplimp/pizza.html)
:link(vmd,http://www.ks.uiuc.edu/Research/vmd)
:link(ensight,http://www.ensight.com)
:link(atomeye,http://mt.seas.upenn.edu/Archive/Graphics/A)
@ -861,7 +863,7 @@ boundary conditions in specific dimensions. See the command doc pages
for details.
The 9 parameters (xlo,xhi,ylo,yhi,zlo,zhi,xy,xz,yz) are defined at the
time the simulation box is created. This happens in one of 3 ways.
time the simluation box is created. This happens in one of 3 ways.
If the "create_box"_create_box.html command is used with a region of
style {prism}, then a triclinic box is setup. See the
"region"_region.html command for details. If the
@ -980,10 +982,10 @@ used with non-orthogonal basis vectors to define a lattice that will
tile a triclinic simulation box via the
"create_atoms"_create_atoms.html command.
A second use is to run Parinello-Rahman dynamics via the "fix
A second use is to run Parinello-Rahman dyanamics via the "fix
npt"_fix_nh.html command, which will adjust the xy, xz, yz tilt
factors to compensate for off-diagonal components of the pressure
tensor. The analog for an "energy minimization"_minimize.html is
tensor. The analalog for an "energy minimization"_minimize.html is
the "fix box/relax"_fix_box_relax.html command.
A third use is to shear a bulk solid to study the response of the
@ -1030,10 +1032,6 @@ profile consistent with the applied shear strain rate.
An alternative method for calculating viscosities is provided via the
"fix viscosity"_fix_viscosity.html command.
NEMD simulations can also be used to measure transport properties of a fluid
through a pore or channel. Simulations of steady-state flow can be performed
using the "fix flow/gauss"_fix_flow_gauss.html command.
:line
6.14 Finite-size spherical and aspherical particles :link(howto_14),h4
@ -1394,7 +1392,7 @@ custom"_dump.html command.
There is also a "dump local"_dump.html format where the user specifies
what local values to output. A pre-defined index keyword can be
specified to enumerate the local values. Two additional kinds of
specified to enumuerate the local values. Two additional kinds of
keywords can also be specified (c_ID, f_ID), where a
"compute"_compute.html or "fix"_fix.html or "variable"_variable.html
provides the values to be output. In each case, the compute or fix
@ -1527,7 +1525,7 @@ Variables that generate values to output :h5,link(variable)
"Variables"_variable.html defined in an input script can store one or
more strings. But equal-style, vector-style, and atom-style or
atomfile-style variables generate a global scalar value, global vector
or values, or a per-atom vector, respectively, when accessed. The
or values, or a per-atom vector, resepctively, when accessed. The
formulas used to define these variables can contain references to the
thermodynamic keywords and to global and per-atom data generated by
computes, fixes, and other variables. The values generated by
@ -1587,7 +1585,7 @@ Temperature is computed as kinetic energy divided by some number of
degrees of freedom (and the Boltzmann constant). Since kinetic energy
is a function of particle velocity, there is often a need to
distinguish between a particle's advection velocity (due to some
aggregate motion of particles) and its thermal velocity. The sum of
aggregate motiion of particles) and its thermal velocity. The sum of
the two is the particle's total velocity, but the latter is often what
is wanted to compute a temperature.
@ -1642,14 +1640,14 @@ nvt/asphere"_fix_nvt_asphere.html thermostat not only translation
velocities but also rotational velocities for spherical and aspherical
particles.
DPD thermostatting alters pairwise interactions in a manner analogous
DPD thermostatting alters pairwise interactions in a manner analagous
to the per-particle thermostatting of "fix
langevin"_fix_langevin.html.
Any of the thermostatting fixes can use temperature computes that
remove bias which has two effects. First, the current calculated
temperature, which is compared to the requested target temperature, is
calculated with the velocity bias removed. Second, the thermostat
caluclated with the velocity bias removed. Second, the thermostat
adjusts only the thermal temperature component of the particle's
velocities, which are the velocities with the bias removed. The
removed bias is then added back to the adjusted velocities. See the
@ -1686,7 +1684,7 @@ nph) and Berendsen:
The "fix npt"_fix_nh.html commands include a Nose-Hoover thermostat
and barostat. "Fix nph"_fix_nh.html is just a Nose/Hoover barostat;
it does no thermostatting. Both "fix nph"_fix_nh.html and "fix
press/berendsen"_fix_press_berendsen.html can be used in conjunction
press/bernendsen"_fix_press_berendsen.html can be used in conjunction
with any of the thermostatting fixes.
As with the thermostats, "fix npt"_fix_nh.html and "fix
@ -1836,7 +1834,7 @@ the deformation must be chosen judiciously, and care must be taken to
fully equilibrate the deformed cell before sampling the stress
tensor. Another approach is to sample the triclinic cell fluctuations
that occur in an NPT simulation. This method can also be slow to
converge and requires careful post-processing "(Shinoda)"_#Shinoda1
converge and requires careful post-processing "(Shinoda)"_#Shinoda
:line
@ -1890,7 +1888,7 @@ instances of LAMMPS to perform different calculations.
The lammps_open_no_mpi() function is similar except that no MPI
communicator is passed from the caller. Instead, MPI_COMM_WORLD is
used to instantiate LAMMPS, and MPI is initialized if necessary.
used to instantiate LAMMPS, and MPI is initialzed if necessary.
The lammps_close() function is used to shut down an instance of LAMMPS
and free all its memory.
@ -1959,12 +1957,9 @@ The extract functions return a pointer to various global or per-atom
quantities stored in LAMMPS or to values calculated by a compute, fix,
or variable. The pointer returned by the extract_global() function
can be used as a permanent reference to a value which may change. For
the extract_atom() method, see the extract() method in the
src/atom.cpp file for a list of valid per-atom properties. New names
could easily be added if the property you want is not listed. For the
other extract functions, the underlying storage may be reallocated as
LAMMPS runs, so you need to re-call the function to assure a current
pointer or returned value(s).
the other extract functions, the underlying storage may be reallocated
as LAMMPS runs, so you need to re-call the function to assure a
current pointer or returned value(s).
The lammps_reset_box() function resets the size and shape of the
simulation box, e.g. as part of restoring a previously extracted and
@ -1980,20 +1975,11 @@ keyword as a double precision value.
The lammps_get_natoms() function returns the total number of atoms in
the system and can be used by the caller to allocate space for the
lammps_gather_atoms() and lammps_scatter_atoms() functions. The
gather function collects peratom info of the requested type (atom
coords, types, forces, etc) from all processors, orders them by atom
ID, and returns a full list to each calling processor. The scatter
function does the inverse. It distributes the same peratom values,
gather function collects atom info of the requested type (atom coords,
types, forces, etc) from all procsesors, orders them by atom ID, and
returns a full list to each calling processor. The scatter function
does the inverse. It distributes the same kinds of values,
passed by the caller, to each atom owned by individual processors.
Both methods are thus a means to extract or assign (overwrite) any
peratom quantities within LAMMPS. See the extract() method in the
src/atom.cpp file for a list of valid per-atom properties. New names
could easily be added if the property you want is not listed.
A special treatment is applied for accessing image flags via the
"image" property. Image flags are stored in a packed format with all
three image flags stored in a single integer. When signaling to access
the image flags as 3 individual values per atom instead of 1, the data
is transparently packed or unpacked by the library interface.
The lammps_create_atoms() function takes a list of N atoms as input
with atom types and coords (required), an optionally atom IDs and
@ -2027,7 +2013,7 @@ a simple Lennard-Jones fluid model. Also, see "this
section"_Section_howto.html#howto_21 of the manual for an analogous
discussion for viscosity.
The thermal conductivity tensor kappa is a measure of the propensity
The thermal conducitivity tensor kappa is a measure of the propensity
of a material to transmit heat energy in a diffusive manner as given
by Fourier's law
@ -2113,7 +2099,7 @@ and grad(Vstream) is the spatial gradient of the velocity of the fluid
moving in another direction, normal to the area through which the
momentum flows. Viscosity thus has units of pressure-time.
The first method is to perform a non-equilibrium MD (NEMD) simulation
The first method is to perform a non-equlibrium MD (NEMD) simulation
by shearing the simulation box via the "fix deform"_fix_deform.html
command, and using the "fix nvt/sllod"_fix_nvt_sllod.html command to
thermostat the fluid via the SLLOD equations of motion.
@ -2139,7 +2125,7 @@ the rNEMD algorithm of Muller-Plathe. Momentum in one dimension is
swapped between atoms in two different layers of the simulation box in
a different dimension. This induces a velocity gradient which can be
monitored with the "fix ave/chunk"_fix_ave_chunk.html command.
The fix tallies the cumulative momentum transfer that it performs.
The fix tallies the cummulative momentum transfer that it performs.
See the "fix viscosity"_fix_viscosity.html command for details.
The fourth method is based on the Green-Kubo (GK) formula which
@ -2282,7 +2268,7 @@ atoms with same local defect structure | chunk ID = output of "compute centro/at
Note that chunk IDs are integer values, so for atom properties or
computes that produce a floating point value, they will be truncated
to an integer. You could also use the compute in a variable that
scales the floating point value to spread it across multiple integers.
scales the floating point value to spread it across multiple intergers.
Spatial bins can be of various kinds, e.g. 1d bins = slabs, 2d bins =
pencils, 3d bins = boxes, spherical bins, cylindrical bins.
@ -2367,7 +2353,7 @@ largest cluster or fastest diffusing molecule. :l
Example calculations with chunks :h5
Here are examples using chunk commands to calculate various
Here are eaxmples using chunk commands to calculate various
properties:
(1) Average velocity in each of 1000 2d spatial bins:
@ -2438,7 +2424,7 @@ which both have their up- and downsides.
The first approach is to set desired real-space an kspace accuracies
via the {kspace_modify force/disp/real} and {kspace_modify
force/disp/kspace} commands. Note that the accuracies have to be
specified in force units and are thus dependent on the chosen unit
specified in force units and are thus dependend on the chosen unit
settings. For real units, 0.0001 and 0.002 seem to provide reasonable
accurate and efficient computations for the real-space and kspace
accuracies. 0.002 and 0.05 work well for most systems using lj
@ -2458,7 +2444,7 @@ performance. This approach provides a fast initialization of the
simulation. However, it is sensitive to errors: A combination of
parameters that will perform well for one system might result in
far-from-optimal conditions for other simulations. For example,
parameters that provide accurate and fast computations for
parametes that provide accurate and fast computations for
all-atomistic force fields can provide insufficient accuracy or
united-atomistic force fields (which is related to that the latter
typically have larger dispersion coefficients).
@ -2492,7 +2478,7 @@ arithmetic mixing rule substantially increases the computational cost.
The computational overhead can be reduced using the {kspace_modify
mix/disp geom} and {kspace_modify splittol} commands. The first
command simply enforces geometric mixing of the dispersion
coefficients in kspace computations. This introduces some error in
coeffiecients in kspace computations. This introduces some error in
the computations but will also significantly speed-up the
simulations. The second keyword sets the accuracy with which the
dispersion coefficients are approximated using a matrix factorization
@ -2511,7 +2497,7 @@ to specify this command explicitly.
6.25 Polarizable models :link(howto_25),h4
In polarizable force fields the charge distributions in molecules and
materials respond to their electrostatic environments. Polarizable
materials respond to their electrostatic environements. Polarizable
systems can be simulated in LAMMPS using three methods:
the fluctuating charge method, implemented in the "QEQ"_fix_qeq.html
@ -2565,7 +2551,7 @@ this is done by "fix qeq/dynamic"_fix_qeq.html, and for the
charge-on-spring models by the methods outlined in the next two
sections. The assignment of masses to the additional degrees of
freedom can lead to unphysical trajectories if care is not exerted in
choosing the parameters of the polarizable models and the simulation
choosing the parameters of the poarizable models and the simulation
conditions.
In the core-shell model the vibration of the shells is kept faster
@ -2587,7 +2573,7 @@ well.
6.26 Adiabatic core/shell model :link(howto_26),h4
The adiabatic core-shell model by "Mitchell and
Fincham"_#MitchellFincham is a simple method for adding
Finchham"_#MitchellFinchham is a simple method for adding
polarizability to a system. In order to mimic the electron shell of
an ion, a satellite particle is attached to it. This way the ions are
split into a core and a shell where the latter is meant to react to
@ -2681,16 +2667,13 @@ bond_coeff 1 63.014 0.0
bond_coeff 2 25.724 0.0 :pre
When running dynamics with the adiabatic core/shell model, the
following issues should be considered. The relative motion of
the core and shell particles corresponds to the polarization,
hereby an instantaneous relaxation of the shells is approximated
and a fast core/shell spring frequency ensures a nearly constant
internal kinetic energy during the simulation.
Thermostats can alter this polarization behaviour, by scaling the
internal kinetic energy, meaning the shell will not react freely to
its electrostatic environment.
Therefore it is typically desirable to decouple the relative motion of
the core/shell pair, which is an imaginary degree of freedom, from the
following issues should be considered. Since the relative motion of
the core and shell particles corresponds to the polarization, typical
thermostats can alter the polarization behaviour, meaning the shell
will not react freely to its electrostatic environment. This is
critical during the equilibration of the system. Therefore
it's typically desirable to decouple the relative motion of the
core/shell pair, which is an imaginary degree of freedom, from the
real physical system. To do that, the "compute
temp/cs"_compute_temp_cs.html command can be used, in conjunction with
any of the thermostat fixes, such as "fix nvt"_fix_nh.html or "fix
@ -2721,54 +2704,44 @@ fix thermostatequ all nve # integrator as needed f
fix_modify thermoberendsen temp CSequ
thermo_modify temp CSequ # output of center-of-mass derived temperature :pre
The pressure for the core/shell system is computed via the regular
LAMMPS convention by "treating the cores and shells as individual
particles"_#MitchellFincham2. For the thermo output of the pressure
as well as for the application of a barostat, it is necessary to
use an additional "pressure"_compute_pressure compute based on the
default "temperature"_compute_temp and specifying it as a second
argument in "fix modify"_fix_modify.html and
"thermo_modify"_thermo_modify.html resulting in:
(...)
compute CSequ all temp/cs cores shells
compute thermo_press_lmp all pressure thermo_temp # pressure for individual particles
thermo_modify temp CSequ press thermo_press_lmp # modify thermo to regular pressure
fix press_bar all npt temp 300 300 0.04 iso 0 0 0.4
fix_modify press_bar temp CSequ press thermo_press_lmp # pressure modification for correct kinetic scalar :pre
If "compute temp/cs"_compute_temp_cs.html is used, the decoupled
relative motion of the core and the shell should in theory be
stable. However numerical fluctuation can introduce a small
momentum to the system, which is noticable over long trajectories.
Therefore it is recommendable to use the "fix
Therefore it is recomendable to use the "fix
momentum"_fix_momentum.html command in combination with "compute
temp/cs"_compute_temp_cs.html when equilibrating the system to
prevent any drift.
When initializing the velocities of a system with core/shell pairs, it
When intializing the velocities of a system with core/shell pairs, it
is also desirable to not introduce energy into the relative motion of
the core/shell particles, but only assign a center-of-mass velocity to
the pairs. This can be done by using the {bias} keyword of the
"velocity create"_velocity.html command and assigning the "compute
temp/cs"_compute_temp_cs.html command to the {temp} keyword of the
"velocity"_velocity.html command, e.g.
"velocity"_velocity.html commmand, e.g.
velocity all create 1427 134 bias yes temp CSequ
velocity all scale 1427 temp CSequ :pre
To maintain the correct polarizability of the core/shell pairs, the
kinetic energy of the internal motion shall remain nearly constant.
Therefore the choice of spring force and mass ratio need to ensure
much faster relative motion of the 2 atoms within the core/shell pair
than their center-of-mass velocity. This allows the shells to
effectively react instantaneously to the electrostatic environment and
limits energy transfer to or from the core/shell oscillators.
This fast movement also dictates the timestep that can be used.
It is important to note that the polarizability of the core/shell
pairs is based on their relative motion. Therefore the choice of
spring force and mass ratio need to ensure much faster relative motion
of the 2 atoms within the core/shell pair than their center-of-mass
velocity. This allow the shells to effectively react instantaneously
to the electrostatic environment. This fast movement also limits the
timestep size that can be used.
The primary literature of the adiabatic core/shell model suggests that
the fast relative motion of the core/shell pairs only allows negligible
energy transfer to the environment.
energy transfer to the environment. Therefore it is not intended to
decouple the core/shell degree of freedom from the physical system
during production runs. In other words, the "compute
temp/cs"_compute_temp_cs.html command should not be used during
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 small drift
in total energy over time. This internal energy can be monitored
using the "compute chunk/atom"_compute_chunk_atom.html and "compute
@ -2788,20 +2761,14 @@ command, to use as input to the "compute
chunk/atom"_compute_chunk_atom.html command to define the core/shell
pairs as chunks.
For example if core/shell pairs are the only molecules:
read_data NaCl_CS_x0.1_prop.data
compute prop all property/atom molecule
compute cs_chunk all chunk/atom c_prop
compute cstherm all temp/chunk cs_chunk temp internal com yes cdof 3.0 # note the chosen degrees of freedom for the core/shell pairs
fix ave_chunk all ave/time 10 1 10 c_cstherm file chunk.dump mode vector :pre
For example if core/shell pairs and other molecules are present:
For example,
fix csinfo all property/atom i_CSID # property/atom command
read_data NaCl_CS_x0.1_prop.data fix csinfo NULL CS-Info # atom property added in the data-file
compute prop all property/atom i_CSID
(...) :pre
compute cs_chunk all chunk/atom c_prop
compute cstherm all temp/chunk cs_chunk temp internal com yes cdof 3.0 # note the chosen degrees of freedom for the core/shell pairs
fix ave_chunk all ave/time 10 1 10 c_cstherm file chunk.dump mode vector :pre
The additional section in the date file would be formatted like this:
@ -2822,7 +2789,7 @@ CS-Info # header of additional section :pre
6.27 Drude induced dipoles :link(howto_27),h4
The thermalized Drude model, similarly to the "core-shell"_#howto_26
model, represents induced dipoles by a pair of charges (the core atom
model, representes induced dipoles by a pair of charges (the core atom
and the Drude particle) connected by a harmonic spring. The Drude
model has a number of features aimed at its use in molecular systems
("Lamoureux and Roux"_#howto-Lamoureux):
@ -2913,23 +2880,19 @@ Fischer, Gao, Guo, Ha, et al, J Phys Chem, 102, 3586 (1998).
[(Mayo)] Mayo, Olfason, Goddard III, J Phys Chem, 94, 8897-8909
(1990).
:link(Jorgensen1)
:link(Jorgensen)
[(Jorgensen)] Jorgensen, Chandrasekhar, Madura, Impey, Klein, J Chem
Phys, 79, 926 (1983).
:link(Price1)
:link(Price)
[(Price)] Price and Brooks, J Chem Phys, 121, 10096 (2004).
:link(Shinoda1)
:link(Shinoda)
[(Shinoda)] Shinoda, Shiga, and Mikami, Phys Rev B, 69, 134103 (2004).
:link(MitchellFincham)
[(Mitchell and Fincham)] Mitchell, Fincham, J Phys Condensed Matter,
:link(MitchellFinchham)
[(Mitchell and Finchham)] Mitchell, Finchham, J Phys Condensed Matter,
5, 1031-1038 (1993).
:link(MitchellFincham2)
[(Fincham)] Fincham, Mackrodt and Mitchell, J Phys Condensed Matter,
6, 393-404 (1994).
:link(howto-Lamoureux)
[(Lamoureux and Roux)] G. Lamoureux, B. Roux, J. Chem. Phys 119, 3025 (2003)

View File

@ -338,13 +338,15 @@ dynamics timestepping, particularly if the computations are not
parallel, so it is often better to leave such analysis to
post-processing codes.
For high-quality visualization we recommend the
A very simple (yet fast) visualizer is provided with the LAMMPS
package - see the "xmovie"_Section_tools.html#xmovie tool in "this
section"_Section_tools.html. It creates xyz projection views of
atomic coordinates and animates them. We find it very useful for
debugging purposes. For high-quality visualization we recommend the
following packages:
"VMD"_http://www.ks.uiuc.edu/Research/vmd
"AtomEye"_http://mt.seas.upenn.edu/Archive/Graphics/A
"OVITO"_http://www.ovito.org/
"ParaView"_http://www.paraview.org/
"PyMol"_http://www.pymol.org
"Raster3d"_http://www.bmsc.washington.edu/raster3d/raster3d.html
"RasMol"_http://www.openrasmol.org :ul

View File

@ -159,17 +159,17 @@ pack_comm_vel: add velocity info to communication buffer (required)
pack_comm_hybrid: store extra info unique to this atom style (optional)
unpack_comm: retrieve an atom's info from the buffer (required)
unpack_comm_vel: also retrieve velocity info (required)
unpack_comm_hybrid: retrieve extra info unique to this atom style (optional)
unpack_comm_hybrid: retreive extra info unique to this atom style (optional)
pack_reverse: store an atom's info in a buffer communicating partial forces (required)
pack_reverse_hybrid: store extra info unique to this atom style (optional)
unpack_reverse: retrieve an atom's info from the buffer (required)
unpack_reverse_hybrid: retrieve extra info unique to this atom style (optional)
unpack_reverse_hybrid: retreive extra info unique to this atom style (optional)
pack_border: store an atom's info in a buffer communicated on neighbor re-builds (required)
pack_border_vel: add velocity info to buffer (required)
pack_border_hybrid: store extra info unique to this atom style (optional)
unpack_border: retrieve an atom's info from the buffer (required)
unpack_border_vel: also retrieve velocity info (required)
unpack_border_hybrid: retrieve extra info unique to this atom style (optional)
unpack_border_hybrid: retreive extra info unique to this atom style (optional)
pack_exchange: store all an atom's info to migrate to another processor (required)
unpack_exchange: retrieve an atom's info from the buffer (required)
size_restart: number of restart quantities associated with proc's atoms (required)
@ -369,7 +369,7 @@ pre_force_respa: same as pre_force, but for rRESPA (optional)
post_force_respa: same as post_force, but for rRESPA (optional)
final_integrate_respa: same as final_integrate, but for rRESPA (optional)
min_pre_force: called after pair & molecular forces are computed in minimizer (optional)
min_post_force: called after pair & molecular forces are computed and communicated in minimizer (optional)
min_post_force: called after pair & molecular forces are computed and communicated in minmizer (optional)
min_store: store extra data for linesearch based minimization on a LIFO stack (optional)
min_pushstore: push the minimization LIFO stack one element down (optional)
min_popstore: pop the minimization LIFO stack one element up (optional)
@ -517,7 +517,7 @@ class. See region.h for details.
inside: determine whether a point is in the region
surface_interior: determine if a point is within a cutoff distance inside of surc
surface_exterior: determine if a point is within a cutoff distance outside of surf
shape_update : change region shape if set by time-dependent variable :tb(s=:)
shape_update : change region shape if set by time-depedent variable :tb(s=:)
:line
@ -601,16 +601,16 @@ Adding keywords for the "thermo_style custom"_thermo_style.html command
"here"_Section_modify.html#mod_13 on this page.
Adding a new math function of one or two arguments can be done by
editing one section of the Variable::evaluate() method. Search for
editing one section of the Variable::evaulate() method. Search for
the word "customize" to find the appropriate location.
Adding a new group function can be done by editing one section of the
Variable::evaluate() method. Search for the word "customize" to find
Variable::evaulate() method. Search for the word "customize" to find
the appropriate location. You may need to add a new method to the
Group class as well (see the group.cpp file).
Accessing a new atom-based vector can be done by editing one section
of the Variable::evaluate() method. Search for the word "customize"
of the Variable::evaulate() method. Search for the word "customize"
to find the appropriate location.
Adding new "compute styles"_compute.html (whose calculated values can
@ -740,7 +740,7 @@ entry to add to the USER-MISC/README file in that dir, along with the
contribute several individual features. :l
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
it is several related featues, 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
@ -785,10 +785,10 @@ 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
prerequiste for building the HTML format files are Python 3.x and
virtualenv, the requirement for generating the PDF format manual
is the "htmldoc"_http://www.htmldoc.org/ software. Please run at least
"make html" and carefully inspect and proofread the resulting HTML format
"make html" and carefully inspect and proofread the resuling HTML format
doc page before submitting your code. :l
For a new package (or even a single command) you should include one or

View File

@ -94,7 +94,7 @@ Package, Description, Author(s), Doc page, Example, Library
:tb(ea=c)
The "Authors" column lists a name(s) if a specific person is
responsible for creating and maintaining the package.
responible for creating and maintaining the package.
(1) The COLLOID package includes Fast Lubrication Dynamics pair styles
which were created by Amit Kumar and Michael Bybee from Jonathan
@ -462,7 +462,7 @@ options you are optimizing for: CPU acceleration via OpenMP, GPU
acceleration, or Intel Xeon Phi. (You can build multiple times to
create LAMMPS executables for different hardware.) It also requires a
C++11 compatible compiler. For GPUs, the NVIDIA "nvcc" compiler is
used, and an appropriate KOKKOS_ARCH setting should be made in your
used, and an appopriate KOKKOS_ARCH setting should be made in your
Makefile.machine for your GPU hardware and NVIDIA software.
The simplest way to do this is to use Makefile.kokkos_cuda or
@ -955,8 +955,8 @@ multi-replica simulations in LAMMPS. Multi-replica methods included
in the package are nudged elastic band (NEB), parallel replica
dynamics (PRD), temperature accelerated dynamics (TAD), parallel
tempering, and a verlet/split algorithm for performing long-range
Coulombics on one set of processors, and the remainder of the force
field calculation on another set.
Coulombics on one set of processors, and the remainded of the force
field calcalation on another set.
To install via make or Make.py:
@ -1140,7 +1140,7 @@ Package, Description, Author(s), Doc page, Example, Pic/movie, Library
"USER-ATC"_#USER-ATC, atom-to-continuum coupling, Jones & Templeton & Zimmerman (1), "fix atc"_fix_atc.html, USER/atc, "atc"_atc, lib/atc
"USER-AWPMD"_#USER-AWPMD, wave-packet MD, Ilya Valuev (JIHT), "pair_style awpmd/cut"_pair_awpmd.html, USER/awpmd, -, lib/awpmd
"USER-CG-CMM"_#USER-CG-CMM, coarse-graining model, Axel Kohlmeyer (Temple U), "pair_style lj/sdk"_pair_sdk.html, USER/cg-cmm, "cg"_cg, -
"USER-CGDNA"_#USER-CGDNA, coarse-grained DNA force fields, Oliver Henrich (U Strathclyde Glasgow), src/USER-CGDNA/README, USER/cgdna, -, -
"USER-CGDNA"_#USER-CGDNA, coarse-grained DNA force fields, Oliver Henrich (U Edinburgh), src/USER-CGDNA/README, USER/cgdna, -, -
"USER-COLVARS"_#USER-COLVARS, collective variables, Fiorin & Henin & Kohlmeyer (2), "fix colvars"_fix_colvars.html, USER/colvars, "colvars"_colvars, lib/colvars
"USER-DIFFRACTION"_#USER-DIFFRACTION, virutal x-ray and electron diffraction, Shawn Coleman (ARL),"compute xrd"_compute_xrd.html, USER/diffraction, -, -
"USER-DPD"_#USER-DPD, reactive dissipative particle dynamics (DPD), Larentzos & Mattox & Brennan (5), src/USER-DPD/README, USER/dpd, -, -
@ -1176,7 +1176,7 @@ Package, Description, Author(s), Doc page, Example, Pic/movie, Library
:link(VMD,http://www.ks.uiuc.edu/Research/vmd)
The "Authors" column lists a name(s) if a specific person is
responsible for creating and maintaining the package.
responible for creating and maintaining the package.
(1) The ATC package was created by Reese Jones, Jeremy Templeton, and
Jon Zimmerman (Sandia).
@ -1288,29 +1288,25 @@ him directly if you have questions.
USER-CGDNA package :link(USER-CGDNA),h5
Contents: The CGDNA package implements coarse-grained force fields for
single- and double-stranded DNA. These are at the moment mainly the
oxDNA and oxDNA2 models, developed by Doye, Louis and Ouldridge at the University
single- and double-stranded DNA. This is at the moment mainly the
oxDNA model, developed by Doye, Louis and Ouldridge at the University
of Oxford. The package also contains Langevin-type rigid-body
integrators with improved stability.
See these doc pages to get started:
"bond_style oxdna/fene"_bond_oxdna.html
"bond_style oxdna2/fene"_bond_oxdna.html
"pair_style oxdna/..."_pair_oxdna.html
"pair_style oxdna2/..."_pair_oxdna2.html
"bond_style oxdna_fene"_bond_oxdna_fene.html
"pair_style oxdna_excv"_pair_oxdna_excv.html
"fix nve/dotc/langevin"_fix_nve_dotc_langevin.html :ul
Supporting info: /src/USER-CGDNA/README, "bond_style
oxdna/fene"_bond_oxdna.html, "bond_style
oxdna2/fene"_bond_oxdna.html, "pair_style
oxdna/..."_pair_oxdna.html, "pair_style
oxdna2/..."_pair_oxdna2.html, "fix
oxdna_fene"_bond_oxdna_fene.html, "pair_style
oxdna_excv"_pair_oxdna_excv.html, "fix
nve/dotc/langevin"_fix_nve_dotc_langevin.html
Author: Oliver Henrich at the University of Strathclyde, Glasgow
(oliver.henrich at strath.ac.uk, also ohenrich at ph.ed.ac.uk).
Contact him directly if you have any questions.
Author: Oliver Henrich at the University of Edinburgh, UK (o.henrich
at epcc.ed.ac.uk or ohenrich at ph.ed.ac.uk). Contact him directly if
you have any questions.
:line
@ -1782,7 +1778,7 @@ particularly with respect to the charge equilibration calculation. It
should also be easier to build and use since there are no complicating
issues with Fortran memory allocation or linking to a Fortran library.
For technical details about this implementation of ReaxFF, see
For technical details about this implemention of ReaxFF, see
this paper:
Parallel and Scalable Reactive Molecular Dynamics: Numerical Methods
@ -1852,7 +1848,7 @@ See this doc page to get started:
The persons who created the USER-SMTBQ package are Nicolas Salles,
Emile Maras, Olivier Politano, Robert Tetot, who can be contacted at
these email addresses: lammps@u-bourgogne.fr, nsalles@laas.fr. Contact
these email addreses: lammps@u-bourgogne.fr, nsalles@laas.fr. Contact
them directly if you have any questions.
Examples: examples/USER/smtbq

View File

@ -69,7 +69,7 @@ bench/in.lj input script.
For all the benchmarks, a useful metric is the CPU cost per atom per
timestep. Since performance scales roughly linearly with problem size
and timesteps for all LAMMPS models (i.e. interatomic or coarse-grained
and timesteps for all LAMMPS models (i.e. inteatomic or coarse-grained
potentials), the run time of any problem using the same model (atom
style, force field, cutoff, etc) can then be estimated.

View File

@ -97,7 +97,7 @@ current LAMMPS library interface and how to call them from Python.
Section 11.8 gives some examples of coupling LAMMPS to other tools via
Python. For example, LAMMPS can easily be coupled to a GUI or other
visualization tools that display graphs or animations in real time as
LAMMPS runs. Examples of such scripts are included in the python
LAMMPS runs. Examples of such scripts are inlcluded in the python
directory.
Two advantages of using Python to run LAMMPS are how concise the
@ -177,7 +177,7 @@ of Python and your machine to successfully build LAMMPS. See the
lib/python/README file for more info.
If you want to write Python code with callbacks to LAMMPS, then you
must also follow the steps overviewed in the preceding section (11.1)
must also follow the steps overviewed in the preceeding section (11.1)
for running LAMMPS from Python. I.e. you must build LAMMPS as a
shared library and insure that Python can find the python/lammps.py
file and the shared library.
@ -325,7 +325,7 @@ sudo python setup.py install :pre
Again, the "sudo" is only needed if required to copy PyPar files into
your Python distribution's site-packages directory.
If you have successfully installed PyPar, you should be able to run
If you have successully installed PyPar, you should be able to run
Python and type
import pypar :pre
@ -369,7 +369,7 @@ user privilege into the user local directory type
python setup.py install --user :pre
If you have successfully installed mpi4py, you should be able to run
If you have successully installed mpi4py, you should be able to run
Python and type
from mpi4py import MPI :pre
@ -594,10 +594,10 @@ flag = lmp.set_variable(name,value) # set existing named string-style vari
value = lmp.get_thermo(name) # return current value of a thermo keyword
natoms = lmp.get_natoms() # total # of atoms as int
data = lmp.gather_atoms(name,type,count) # return per-atom property of all atoms gathered into data, ordered by atom ID
data = lmp.gather_atoms(name,type,count) # return atom attribute of all atoms gathered into data, ordered by atom ID
# name = "x", "charge", "type", etc
# count = # of per-atom values, 1 or 3, etc
lmp.scatter_atoms(name,type,count,data) # scatter per-atom property to all atoms from data, ordered by atom ID
lmp.scatter_atoms(name,type,count,data) # scatter atom attribute of all atoms from data, ordered by atom ID
# name = "x", "charge", "type", etc
# count = # of per-atom values, 1 or 3, etc :pre
@ -610,7 +610,7 @@ lmp = lammps() :pre
create an instance of LAMMPS, wrapped in a Python class by the lammps
Python module, and return an instance of the Python class as lmp. It
is used to make all subsequent calls to the LAMMPS library.
is used to make all subequent calls to the LAMMPS library.
Additional arguments to lammps() can be used to tell Python the name
of the shared library to load or to pass arguments to the LAMMPS
@ -656,13 +656,13 @@ argument.
For extract_atom(), a pointer to internal LAMMPS atom-based data is
returned, which you can use via normal Python subscripting. See the
extract() method in the src/atom.cpp file for a list of valid names.
Again, new names could easily be added if the property you want is not
listed. A pointer to a vector of doubles or integers, or a pointer to
an array of doubles (double **) or integers (int **) is returned. You
need to specify the appropriate data type via the type argument.
Again, new names could easily be added. A pointer to a vector of
doubles or integers, or a pointer to an array of doubles (double **)
or integers (int **) is returned. You need to specify the appropriate
data type via the type argument.
For extract_compute() and extract_fix(), the global, per-atom, or
local data calculated by the compute or fix can be accessed. What is
local data calulated by the compute or fix can be accessed. What is
returned depends on whether the compute or fix calculates a scalar or
vector or array. For a scalar, a single double value is returned. If
the compute or fix calculates a vector or array, a pointer to the
@ -689,21 +689,12 @@ specified group.
The get_natoms() method returns the total number of atoms in the
simulation, as an int.
The gather_atoms() method allows any per-atom property (coordinates,
velocities, etc) to be extracted from LAMMPS. It returns a ctypes
vector of ints or doubles as specified by type, of length
count*natoms, for the named property for all atoms in the simulation.
The data is ordered by count and then by atom ID. See the extract()
method in the src/atom.cpp file for a list of valid names. Again, new
names could easily be added if the property you want is missing. The
vector can be used via normal Python subscripting. If atom IDs are
not consecutively ordered within LAMMPS, a None is returned as
indication of an error. A special treatment is applied for image flags
stored in the "image" property. All three image flags are stored in
a packed format in a single integer, so count would be 1 to retrieve
that integer, however also a count value of 3 can be used and then
the image flags will be unpacked into 3 individual integers, ordered
in a similar fashion as coordinates.
The gather_atoms() method returns a ctypes vector of ints or doubles
as specified by type, of length count*natoms, for the property of all
the atoms in the simulation specified by name, ordered by count and
then by atom ID. The vector can be used via normal Python
subscripting. If atom IDs are not consecutively ordered within
LAMMPS, a None is returned as indication of an error.
Note that the data structure gather_atoms("x") returns is different
from the data structure returned by extract_atom("x") in four ways.
@ -720,22 +711,14 @@ assigning a new values to the extract_atom() array. To do this with
the gather_atoms() vector, you need to change values in the vector,
then invoke the scatter_atoms() method.
The scatter_atoms() method allows any per-atom property (coordinates,
velocities, etc) to be inserted into LAMMPS, overwriting the current
property. It takes a vector of ints or doubles as specified by type,
of length count*natoms, for the named property for all atoms in the
simulation. The data should be ordered by count and then by atom ID.
See the extract() method in the src/atom.cpp file for a list of valid
names. Again, new names could easily be added if the property you
want is missing. It uses the vector of data to overwrite the
corresponding properties for each atom inside LAMMPS. This requires
LAMMPS to have its "map" option enabled; see the
"atom_modify"_atom_modify.html command for details. If it is not, or
if atom IDs are not consecutively ordered, no coordinates are reset.
Similar as for gather_atoms() a special treatment is applied for image
flags, which can be provided in packed (count = 1) or unpacked (count = 3)
format and in the latter case, they will be packed before applied to
atoms.
The scatter_atoms() method takes a vector of ints or doubles as
specified by type, of length count*natoms, for the property of all the
atoms in the simulation specified by name, ordered by bount and then
by atom ID. It uses the vector of data to overwrite the corresponding
properties for each atom inside LAMMPS. This requires LAMMPS to have
its "map" option enabled; see the "atom_modify"_atom_modify.html
command for details. If it is not, or if atom IDs are not
consecutively ordered, no coordinates are reset.
The array of coordinates passed to scatter_atoms() must be a ctypes
vector of ints or doubles, allocated and initialized something like
@ -751,7 +734,7 @@ x\[2\] = z coord of atom with ID 1
x\[3\] = x coord of atom with ID 2
...
x\[n3-1\] = z coord of atom with ID natoms
lmp.scatter_atoms("x",1,3,x) :pre
lmp.scatter_coords("x",1,3,x) :pre
Alternatively, you can just change values in the vector returned by
gather_atoms("x",1,3), since it is a ctypes vector of doubles.
@ -791,7 +774,7 @@ demo.py, invoke various LAMMPS library interface routines,
simple.py, run in parallel, similar to examples/COUPLE/simple/simple.cpp,
split.py, same as simple.py but running in parallel on a subset of procs,
gui.py, GUI go/stop/temperature-slider to control LAMMPS,
plot.py, real-time temperature plot with GnuPlot via Pizza.py,
plot.py, real-time temeperature plot with GnuPlot via Pizza.py,
viz_tool.py, real-time viz via some viz package,
vizplotgui_tool.py, combination of viz_tool.py and plot.py and gui.py :tb(c=2)

View File

@ -80,7 +80,7 @@ This section has the following sub-sections:
Read this first :h5,link(start_2_1)
If you want to avoid building LAMMPS yourself, read the preceding
If you want to avoid building LAMMPS yourself, read the preceeding
section about options available for downloading and installing
executables. Details are discussed on the "download"_download page.
@ -251,7 +251,7 @@ re-compile, after typing "make clean" (which will describe different
clean options).
The LMP_INC variable is used to include options that turn on ifdefs
within the LAMMPS code. The options that are currently recognized are:
within the LAMMPS code. The options that are currently recogized are:
-DLAMMPS_GZIP
-DLAMMPS_JPEG
@ -362,7 +362,7 @@ installed on your platform. If MPI is installed on your system in the
usual place (under /usr/local), you also may not need to specify these
3 variables, assuming /usr/local is in your path. On some large
parallel machines which use "modules" for their compile/link
environments, you may simply need to include the correct module in
environements, you may simply need to include the correct module in
your build environment, before building LAMMPS. Or the parallel
machine may have a vendor-provided MPI which the compiler has no
trouble finding.
@ -413,7 +413,7 @@ uses (for performing 1d FFTs) when running the particle-particle
particle-mesh (PPPM) option for long-range Coulombics via the
"kspace_style"_kspace_style.html command.
LAMMPS supports common open-source or vendor-supplied FFT libraries
LAMMPS supports various open-source or vendor-supplied FFT libraries
for this purpose. If you leave these 3 variables blank, LAMMPS will
use the open-source "KISS FFT library"_http://kissfft.sf.net, which is
included in the LAMMPS distribution. This library is portable to all
@ -423,14 +423,15 @@ package in your build, you can also leave the 3 variables blank.
Otherwise, select which kinds of FFTs to use as part of the FFT_INC
setting by a switch of the form -DFFT_XXX. Recommended values for XXX
are: MKL or FFTW3. FFTW2 and NONE are supported as legacy options.
Selecting -DFFT_FFTW will use the FFTW3 library and -DFFT_NONE will
use the KISS library described above.
are: MKL, SCSL, FFTW2, and FFTW3. Legacy options are: INTEL, SGI,
ACML, and T3E. For backward compatability, using -DFFT_FFTW will use
the FFTW2 library. Using -DFFT_NONE will use the KISS library
described above.
You may also need to set the FFT_INC, FFT_PATH, and FFT_LIB variables,
so the compiler and linker can find the needed FFT header and library
files. Note that on some large parallel machines which use "modules"
for their compile/link environments, you may simply need to include
for their compile/link environements, you may simply need to include
the correct module in your build environment. Or the parallel machine
may have a vendor-provided FFT library which the compiler has no
trouble finding.
@ -450,12 +451,13 @@ you must also manually specify the correct library, namely -lsfftw or
The FFT_INC variable also allows for a -DFFT_SINGLE setting that will
use single-precision FFTs with PPPM, which can speed-up long-range
calculations, particularly in parallel or on GPUs. Fourier transform
calulations, particularly in parallel or on GPUs. Fourier transform
and related PPPM operations are somewhat insensitive to floating point
truncation errors and thus do not always need to be performed in
double precision. Using the -DFFT_SINGLE setting trades off a little
accuracy for reduced memory use and parallel communication costs for
transposing 3d FFT data.
transposing 3d FFT data. Note that single precision FFTs have only
been tested with the FFTW3, FFTW2, MKL, and KISS FFT options.
Step 7 :h6
@ -681,7 +683,7 @@ various make commands that can be used to manipulate packages.
If you use a command in a LAMMPS input script that is part of a
package, you must have built LAMMPS with that package, else you will
get an error that the style is invalid or the command is unknown.
Every command's doc page specifies if it is part of a package. You can
Every command's doc page specfies if it is part of a package. You can
also type
lmp_machine -h :pre
@ -1007,7 +1009,7 @@ Instead, it creates src/MAKE/MINE/Makefile.auto, which you can save or
rename if desired. Likewise it creates an executable named
src/lmp_auto, which you can rename using the -o switch if desired.
The most recently executed Make.py command is saved in
The most recently executed Make.py commmand is saved in
src/Make.py.last. You can use the "-r" switch (for redo) to re-invoke
the last command, or you can save a sequence of one or more Make.py
commands to a file and invoke the file of commands using "-r". You
@ -1063,7 +1065,7 @@ src/MAKE/Makefile.foo and perform the build in the directory
Obj_shared_foo. This is so that each file can be compiled with the
-fPIC flag which is required for inclusion in a shared library. The
build will create the file liblammps_foo.so which another application
can link to dynamically. It will also create a soft link liblammps.so,
can link to dyamically. It will also create a soft link liblammps.so,
which will point to the most recently built shared library. This is
the file the Python wrapper loads by default.
@ -1415,8 +1417,8 @@ LAMMPS is compiled with CUDA=yes.
numa Nm :pre
This option is only relevant when using pthreads with hwloc support.
In this case Nm defines the number of NUMA regions (typically sockets)
on a node which will be utilized by a single MPI rank. By default Nm
In this case Nm defines the number of NUMA regions (typicaly sockets)
on a node which will be utilizied by a single MPI rank. By default Nm
= 1. If this option is used the total number of worker-threads per
MPI rank is threads*numa. Currently it is always almost better to
assign at least one MPI rank per NUMA region, and leave numa set to
@ -1480,7 +1482,7 @@ replica runs on on one or a few processors. Note that with MPI
installed on a machine (e.g. your desktop), you can run on more
(virtual) processors than you have physical processors.
To run multiple independent simulations from one input script, using
To run multiple independent simulatoins from one input script, using
multiple partitions, see "Section 6.4"_Section_howto.html#howto_4
of the manual. World- and universe-style "variables"_variable.html
are useful in this context.
@ -1759,7 +1761,7 @@ The first section provides a global loop timing summary. The {loop time}
is the total wall time for the section. The {Performance} line is
provided for convenience to help predicting the number of loop
continuations required and for comparing performance with other,
similar MD codes. The {CPU use} line provides the CPU utilization per
similar MD codes. The {CPU use} line provides the CPU utilzation per
MPI task; it should be close to 100% times the number of OpenMP
threads (or 1 of no OpenMP). Lower numbers correspond to delays due
to file I/O or insufficient thread utilization.

View File

@ -12,12 +12,9 @@ Section"_Section_modify.html :c
LAMMPS is designed to be a computational kernel for performing
molecular dynamics computations. Additional pre- and post-processing
steps are often necessary to setup and analyze a simulation. A
list of such tools can be found on the LAMMPS home page
at "http://lammps.sandia.gov/prepost.html"_http://lammps.sandia.gov/prepost.html
A few additional tools are provided with the LAMMPS distribution
and are described in this section.
steps are often necessary to setup and analyze a simulation. A few
additional tools are provided with the LAMMPS distribution and are
described in this section.
Our group has also written and released a separate toolkit called
"Pizza.py"_pizza which provides tools for doing setup, analysis,
@ -39,16 +36,16 @@ authors.
The source code for each of these codes is in the tools sub-directory
of the LAMMPS distribution. There is a Makefile (which you may need
to edit for your platform) which will build several of the tools which
reside in that directory. Most of them are larger packages in their
own sub-directories with their own Makefiles and/or README files.
reside in that directory. Some of them are larger packages in their
own sub-directories with their own Makefiles.
"amber2lmp"_#amber
"binary2txt"_#binary
"ch2lmp"_#charmm
"chain"_#chain
"colvars"_#colvars
"createatoms"_#createatoms
"drude"_#drude
"createatoms"_#create
"data2xmovie"_#data
"eam database"_#eamdb
"eam generate"_#eamgn
"eff"_#eff
@ -59,18 +56,20 @@ own sub-directories with their own Makefiles and/or README files.
"kate"_#kate
"lmp2arc"_#arc
"lmp2cfg"_#cfg
"lmp2vmd"_#vmd
"matlab"_#matlab
"micelle2d"_#micelle
"moltemplate"_#moltemplate
"msi2lmp"_#msi
"phonon"_#phonon
"polybond"_#polybond
"polymer bonding"_#polybond
"pymol_asphere"_#pymol
"python"_#pythontools
"reax"_#reax_tool
"smd"_#smd
"restart2data"_#restart
"vim"_#vim
"xmgrace"_#xmgrace
"xmovie"_#xmovie :ul
:line
@ -159,7 +158,7 @@ gmail.com) at ICTP, Italy.
:line
createatoms tool :h4,link(createatoms)
createatoms tool :h4,link(create)
The tools/createatoms directory contains a Fortran program called
createAtoms.f which can generate a variety of interesting crystal
@ -172,16 +171,16 @@ The tool is authored by Xiaowang Zhou (Sandia), xzhou at sandia.gov.
:line
drude tool :h4,link(drude)
data2xmovie tool :h4,link(data)
The tools/drude directory contains a Python script called
polarizer.py which can add Drude oscillators to a LAMMPS
data file in the required format.
The file data2xmovie.c converts a LAMMPS data file into a snapshot
suitable for visualizing with the "xmovie"_#xmovie tool, as if it had
been output with a dump command from LAMMPS itself. The syntax for
running the tool is
See the header of the polarizer.py file for details.
data2xmovie \[options\] < infile > outfile :pre
The tool is authored by Agilio Padua and Alain Dequidt: agilio.padua
at univ-bpclermont.fr, alain.dequidt at univ-bpclermont.fr
See the top of the data2xmovie.c file for a discussion of the options.
:line
@ -318,6 +317,18 @@ This tool was written by Ara Kooser at Sandia (askoose at sandia.gov).
:line
lmp2vmd tool :h4,link(vmd)
The lmp2vmd sub-directory contains a README.txt file that describes
details of scripts and plugin support within the "VMD
package"_http://www.ks.uiuc.edu/Research/vmd for visualizing LAMMPS
dump files.
The VMD plugins and other supporting scripts were written by Axel
Kohlmeyer (akohlmey at cmm.chem.upenn.edu) at U Penn.
:line
matlab tool :h4,link(matlab)
The matlab sub-directory contains several "MATLAB"_matlabhome scripts for
@ -370,14 +381,16 @@ supports it. It has its own WWW page at
msi2lmp tool :h4,link(msi)
The msi2lmp sub-directory contains a tool for creating LAMMPS input
data files from BIOVIA's Materias Studio files (formerly Accelrys'
Insight MD code, formerly MSI/Biosym and its Discover MD code).
data files from Accelrys' Insight MD code (formerly MSI/Biosym and
its Discover MD code). See the README file for more information.
This tool was written by John Carpenter (Cray), Michael Peachey
(Cray), and Steve Lustig (Dupont). Several people contributed changes
to remove bugs and adapt its output to changes in LAMMPS.
(Cray), and Steve Lustig (Dupont). John is now at the Mayo Clinic
(jec at mayo.edu), but still fields questions about the tool.
See the README file for more information.
This tool may be out-of-date with respect to the current LAMMPS and
Insight versions. Since we don't use it at Sandia, you'll need to
experiment with it yourself.
:line
@ -396,7 +409,7 @@ University.
:line
polybond tool :h4,link(polybond)
polymer bonding tool :h4,link(polybond)
The polybond sub-directory contains a Python-based tool useful for
performing "programmable polymer bonding". The Python file
@ -455,19 +468,48 @@ These tools were written by Aidan Thompson at Sandia.
:line
smd tool :h4,link(smd)
restart2data tool :h4,link(restart)
The smd sub-directory contains a C++ file dump2vtk_tris.cpp and
Makefile which can be compiled and used to convert triangle output
files created by the Smooth-Mach Dynamics (USER-SMD) package into a
VTK-compatible unstructured grid file. It could then be read in and
visualized by VTK.
NOTE: This tool is now obsolete and is not included in the current
LAMMPS distribution. This is becaues there is now a
"write_data"_write_data.html command, which can create a data file
from within an input script. Running LAMMPS with the "-r"
"command-line switch"_Section_start.html#start_7 as follows:
See the header of dump2vtk.cpp for more details.
lmp_g++ -r restartfile datafile
This tool was written by the USER-SMD package author, Georg
Ganzenmuller at the Fraunhofer-Institute for High-Speed Dynamics,
Ernst Mach Institute in Germany (georg.ganzenmueller at emi.fhg.de).
is the same as running a 2-line input script:
read_restart restartfile
write_data datafile
which will produce the same data file that the restart2data tool used
to create. The following information is included in case you have an
older version of LAMMPS which still includes the restart2data tool.
The file restart2data.cpp converts a binary LAMMPS restart file into
an ASCII data file. The syntax for running the tool is
restart2data restart-file data-file (input-file) :pre
Input-file is optional and if specified will contain LAMMPS input
commands for the masses and force field parameters, instead of putting
those in the data-file. Only a few force field styles currently
support this option.
This tool must be compiled on a platform that can read the binary file
created by a LAMMPS run, since binary files are not compatible across
all platforms.
Note that a text data file has less precision than a binary restart
file. Hence, continuing a run from a converted data file will
typically not conform as closely to a previous run as will restarting
from a binary restart file.
If a "%" appears in the specified restart-file, the tool expects a set
of multiple files to exist. See the "restart"_restart.html and
"write_restart"_write_restart.html commands for info on how such sets
of files are written by LAMMPS, and how the files are named.
:line
@ -495,3 +537,32 @@ See the README file for details.
These files were provided by Vikas Varshney (vv0210 at gmail.com)
:line
xmovie tool :h4,link(xmovie)
The xmovie tool is an X-based visualization package that can read
LAMMPS dump files and animate them. It is in its own sub-directory
with the tools directory. You may need to modify its Makefile so that
it can find the appropriate X libraries to link against.
The syntax for running xmovie is
xmovie \[options\] dump.file1 dump.file2 ... :pre
If you just type "xmovie" you will see a list of options. Note that
by default, LAMMPS dump files are in scaled coordinates, so you
typically need to use the -scale option with xmovie. When xmovie runs
it opens a visualization window and a control window. The control
options are straightforward to use.
Xmovie was mostly written by Mike Uttormark (U Wisconsin) while he
spent a summer at Sandia. It displays 2d projections of a 3d domain.
While simple in design, it is an amazingly fast program that can
render large numbers of atoms very quickly. It's a useful tool for
debugging LAMMPS input and output and making sure your simulation is
doing what you think it should. The animations on the Examples page
of the "LAMMPS WWW site"_lws were created with xmovie.
I've lost contact with Mike, so I hope he's comfortable with us
distributing his great tool!

View File

@ -27,7 +27,7 @@
syntax</a></h2>
<p>fix_modify AtC consistent_fe_initialization &lt;on | off&gt;</p>
<ul>
<li>&lt;on|off&gt; = switch to activiate/deactiviate the initial setting of FE intrinsic field to match the projected MD field </li>
<li>&lt;on|off&gt; = switch to activiate/deactiviate the intial setting of FE intrinsic field to match the projected MD field </li>
</ul>
<h2><a class="anchor" id="examples">
examples</a></h2>

View File

@ -20,7 +20,7 @@ coprocessors via offloading neighbor list and non-bonded force
calculations to the Phi. The same C++ code is used in both cases.
When offloading to a coprocessor from a CPU, the same routine is run
twice, once on the CPU and once with an offload flag. This allows
LAMMPS to run on the CPU cores and coprocessor cores simultaneously.
LAMMPS to run on the CPU cores and coprocessor cores simulataneously.
[Currently Available USER-INTEL Styles:]
@ -115,7 +115,7 @@ coprocessor and an Intel compiler are required. For this, the
recommended version of the Intel compiler is 14.0.1.106 or
versions 15.0.2.044 and higher.
Although any compiler can be used with the USER-INTEL package,
Although any compiler can be used with the USER-INTEL pacakge,
currently, vectorization directives are disabled by default when
not using Intel compilers due to lack of standard support and
observations of decreased performance. The OpenMP standard now
@ -428,7 +428,7 @@ to the card. This allows for overlap of MPI communication of forces
with computation on the coprocessor when the "newton"_newton.html
setting is "on". The default is dependent on the style being used,
however, better performance may be achieved by setting this option
explicitly.
explictly.
When using offload with CPU Hyper-Threading disabled, it may help
performance to use fewer MPI tasks and OpenMP threads than available
@ -464,7 +464,7 @@ supported.
[References:]
Brown, W.M., Carrillo, J.-M.Y., Mishra, B., Gavhane, N., Thakker, F.M., De Kraker, A.R., Yamada, M., Ang, J.A., Plimpton, S.J., "Optimizing Classical Molecular Dynamics in LAMMPS," in Intel Xeon Phi Processor High Performance Programming: Knights Landing Edition, J. Jeffers, J. Reinders, A. Sodani, Eds. Morgan Kaufmann. :ulb,l
Brown, W.M., Carrillo, J.-M.Y., Mishra, B., Gavhane, N., Thakker, F.M., De Kraker, A.R., Yamada, M., Ang, J.A., Plimpton, S.J., Optimizing Classical Molecular Dynamics in LAMMPS, in Intel Xeon Phi Processor High Performance Programming: Knights Landing Edition, J. Jeffers, J. Reinders, A. Sodani, Eds. Morgan Kaufmann. :ulb,l
Brown, W. M., Semin, A., Hebenstreit, M., Khvostov, S., Raman, K., Plimpton, S.J. Increasing Molecular Dynamics Simulation Rates with an 8-Fold Increase in Electrical Power Efficiency. 2016 International Conference for High Performance Computing. In press. :l

View File

@ -217,7 +217,7 @@ best performance its CCFLAGS setting should use -O3 and have a
KOKKOS_ARCH setting that matches the compute capability of your NVIDIA
hardware and software installation, e.g. KOKKOS_ARCH=Kepler30. Note
the minimal required compute capability is 2.0, but this will give
significantly reduced performance compared to Kepler generation GPUs
signicantly reduced performance compared to Kepler generation GPUs
with compute capability 3.x. For the LINK setting, "nvcc" should not
be used; instead use g++ or another compiler suitable for linking C++
applications. Often you will want to use your MPI compiler wrapper
@ -234,7 +234,7 @@ provides alternative methods via environment variables for binding
threads to hardware cores. More info on binding threads to cores is
given in "Section 5.3"_Section_accelerate.html#acc_3.
KOKKOS_ARCH=KNC enables compiler switches needed when compiling for an
KOKKOS_ARCH=KNC enables compiler switches needed when compling for an
Intel Phi processor.
KOKKOS_USE_TPLS=librt enables use of a more accurate timer mechanism
@ -272,7 +272,7 @@ coprocessor support you need to insure there are one or more MPI tasks
per coprocessor, and choose the number of coprocessor threads to use
per MPI task (via the "-k" command-line switch discussed below). The
product of MPI tasks * coprocessor threads/task should not exceed the
maximum number of threads the coprocessor is designed to run,
maximum number of threads the coproprocessor is designed to run,
otherwise performance will suffer. This value is 240 for current
generation Xeon Phi(TM) chips, which is 60 physical cores * 4
threads/core. Note that with the KOKKOS package you do not need to
@ -333,7 +333,7 @@ device=CUDA are the same.
You must still use the "-k on" "command-line
switch"_Section_start.html#start_7 to enable the KOKKOS package, and
specify its additional arguments for hardware options appropriate to
specify its additional arguments for hardware options appopriate to
your system, as documented above.
Use the "suffix kk"_suffix.html command, or you can explicitly add a

View File

@ -8,7 +8,6 @@
angle_style class2 command :h3
angle_style class2/omp command :h3
angle_style class2/kk command :h3
[Syntax:]

View File

@ -41,7 +41,7 @@ angle.
The torque on the dipole can be obtained by differentiating the
potential using the 'chain rule' as in appendix C.3 of
"(Allen)"_#Allen1:
"(Allen)"_#Allen:
:c,image(Eqs/angle_dipole_torque.jpg)
@ -121,6 +121,6 @@ This angle style should not be used with SHAKE.
[(Orsi)] Orsi & Essex, The ELBA force field for coarse-grain modeling of
lipid membranes, PloS ONE 6(12): e28637, 2011.
:link(Allen1)
:link(Allen)
[(Allen)] Allen & Tildesley, Computer Simulation of Liquids,
Clarendon Press, Oxford, 1987.

View File

@ -81,7 +81,7 @@ LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other angle styles, the hybrid angle style does not store angle
coefficient info for individual sub-styles in a "binary restart
files"_restart.html. Thus when restarting a simulation from a restart
files"_restart.html. Thus when retarting a simulation from a restart
file, you need to re-specify angle_coeff commands.
[Related commands:]

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@ -103,7 +103,7 @@ turns off the {first} option.
It is OK to use the {first} keyword with a group that has not yet been
defined, e.g. to use the atom_modify first command at the beginning of
your input script. LAMMPS does not use the group until a simulation
your input script. LAMMPS does not use the group until a simullation
is run.
The {sort} keyword turns on a spatial sorting or reordering of atoms
@ -116,7 +116,7 @@ various other factors. As a general rule, sorting is typically more
effective at speeding up simulations of liquids as opposed to solids.
In tests we have done, the speed-up can range from zero to 3-4x.
Reordering is performed every {Nfreq} timesteps during a dynamics run
Reordering is peformed every {Nfreq} timesteps during a dynamics run
or iterations during a minimization. More precisely, reordering
occurs at the first reneighboring that occurs after the target
timestep. The reordering is performed locally by each processor,
@ -130,7 +130,7 @@ the processor's 1d list of atoms.
The goal of this procedure is for atoms to put atoms close to each
other in the processor's one-dimensional list of atoms that are also
near to each other spatially. This can improve cache performance when
pairwise interactions and neighbor lists are computed. Note that if
pairwise intereractions and neighbor lists are computed. Note that if
bins are too small, there will be few atoms/bin. Likewise if bins are
too large, there will be many atoms/bin. In both cases, the goal of
cache locality will be undermined.
@ -138,7 +138,7 @@ cache locality will be undermined.
NOTE: Running a simulation with sorting on versus off should not
change the simulation results in a statistical sense. However, a
different ordering will induce round-off differences, which will lead
to diverging trajectories over time when comparing two simulations.
to diverging trajectories over time when comparing two simluations.
Various commands, particularly those which use random numbers
(e.g. "velocity create"_velocity.html, and "fix
langevin"_fix_langevin.html), may generate (statistically identical)

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@ -110,17 +110,12 @@ basis.
For the {sphere} style, the particles are spheres and each stores a
per-particle diameter and mass. If the diameter > 0.0, the particle
is a finite-size sphere. If the diameter = 0.0, it is a point
particle. Note that by use of the {disc} keyword with the "fix
nve/sphere"_fix_nve_sphere.html, "fix nvt/sphere"_fix_nvt_sphere.html,
"fix nph/sphere"_fix_nph_sphere.html, "fix
npt/sphere"_fix_npt_sphere.html commands, spheres can be effectively
treated as 2d discs for a 2d simulation if desired. See also the "set
density/disc"_set.html command.
particle.
For the {ellipsoid} style, the particles are ellipsoids and each
stores a flag which indicates whether it is a finite-size ellipsoid or
a point particle. If it is an ellipsoid, it also stores a shape
vector with the 3 diameters of the ellipsoid and a quaternion 4-vector
vector with the 3 diamters of the ellipsoid and a quaternion 4-vector
with its orientation.
For the {dipole} style, a point dipole is defined for each point
@ -154,7 +149,7 @@ Hydrodynamics. Both fluids and solids can be modeled. Particles
store the mass and volume of an integration point, a kernel diameter
used for calculating the field variables (e.g. stress and deformation)
and a contact radius for calculating repulsive forces which prevent
individual physical bodies from penetrating each other.
individual physical bodies from penetretating each other.
The {wavepacket} style is similar to {electron}, but the electrons may
consist of several Gaussian wave packets, summed up with coefficients
@ -170,7 +165,7 @@ For the {tri} style, the particles are planar triangles and each
stores a per-particle mass and size and orientation (i.e. the corner
points of the triangle).
The {template} style allows molecular topology (bonds,angles,etc) to be
The {template} style allows molecular topolgy (bonds,angles,etc) to be
defined via a molecule template using the "molecule"_molecule.html
command. The template stores one or more molecules with a single copy
of the topology info (bonds,angles,etc) of each. Individual atoms
@ -200,7 +195,7 @@ the {bstyle} argument. Body particles can represent complex entities,
such as surface meshes of discrete points, collections of
sub-particles, deformable objects, etc.
The "body"_body.html doc page describes the body styles LAMMPS
The "body"_body.html doc page descibes the body styles LAMMPS
currently supports, and provides more details as to the kind of body
particles they represent. For all styles, each body particle stores
moments of inertia and a quaternion 4-vector, so that its orientation
@ -285,7 +280,7 @@ The {dpd} style is part of the USER-DPD package for dissipative
particle dynamics (DPD).
The {meso} style is part of the USER-SPH package for smoothed particle
hydrodynamics (SPH). See "this PDF
hydrodyanmics (SPH). See "this PDF
guide"_USER/sph/SPH_LAMMPS_userguide.pdf to using SPH in LAMMPS.
The {wavepacket} style is part of the USER-AWPMD package for the

View File

@ -12,7 +12,7 @@ balance command :h3
balance thresh style args ... keyword args ... :pre
thresh = imbalance threshold that must be exceeded to perform a re-balance :ulb,l
thresh = imbalance threshhold that must be exceeded to perform a re-balance :ulb,l
one style/arg pair can be used (or multiple for {x},{y},{z}) :l
style = {x} or {y} or {z} or {shift} or {rcb} :l
{x} args = {uniform} or Px-1 numbers between 0 and 1
@ -30,7 +30,7 @@ style = {x} or {y} or {z} or {shift} or {rcb} :l
{shift} args = dimstr Niter stopthresh
dimstr = sequence of letters containing "x" or "y" or "z", each not more than once
Niter = # of times to iterate within each dimension of dimstr sequence
stopthresh = stop balancing when this imbalance threshold is reached
stopthresh = stop balancing when this imbalance threshhold is reached
{rcb} args = none :pre
zero or more keyword/arg pairs may be appended :l
keyword = {weight} or {out} :l
@ -76,13 +76,13 @@ sub-domain sizes and shapes on-the-fly during a "run"_run.html.
Load-balancing is typically most useful if the particles in the
simulation box have a spatially-varying density distribution or when
the computational cost varies significantly between different
the computational cost varies signficantly between different
particles. E.g. a model of a vapor/liquid interface, or a solid with
an irregular-shaped geometry containing void regions, or "hybrid pair
style simulations"_pair_hybrid.html which combine pair styles with
different computational cost. In these cases, the LAMMPS default of
dividing the simulation box volume into a regular-spaced grid of 3d
bricks, with one equal-volume sub-domain per processor, may assign
bricks, with one equal-volume sub-domain per procesor, may assign
numbers of particles per processor in a way that the computational
effort varies significantly. This can lead to poor performance when
the simulation is run in parallel.
@ -91,7 +91,7 @@ The balancing can be performed with or without per-particle weighting.
With no weighting, the balancing attempts to assign an equal number of
particles to each processor. With weighting, the balancing attempts
to assign an equal aggregate computational weight to each processor,
which typically induces a different number of atoms assigned to each
which typically inducces a diffrent number of atoms assigned to each
processor. Details on the various weighting options and examples for
how they can be used are "given below"_#weighted_balance.
@ -222,7 +222,7 @@ listed in ascending order. They represent the fractional position of
the cutting place. The left (or lower) edge of the box is 0.0, and
the right (or upper) edge is 1.0. Neither of these values is
specified. Only the interior Ps-1 positions are specified. Thus is
there are 2 processors in the x dimension, you specify a single value
there are 2 procesors in the x dimension, you specify a single value
such as 0.75, which would make the left processor's sub-domain 3x
larger than the right processor's sub-domain.
@ -266,7 +266,7 @@ assigned, particles are migrated to their new owning processor, and
the balance procedure ends.
NOTE: At each rebalance operation, the bisectioning for each cutting
plane (line in 2d) typically starts with low and high bounds separated
plane (line in 2d) typcially starts with low and high bounds separated
by the extent of a processor's sub-domain in one dimension. The size
of this bracketing region shrinks by 1/2 every iteration. Thus if
{Niter} is specified as 10, the cutting plane will typically be
@ -286,32 +286,24 @@ above. It performs a recursive coordinate bisectioning (RCB) of the
simulation domain. The basic idea is as follows.
The simulation domain is cut into 2 boxes by an axis-aligned cut in
one of the dimensions, leaving one new sub-box on either side of the
cut. Which dimension is chosen for the cut depends on the particle
(weight) distribution within the parent box. Normally the longest
dimension of the box is cut, but if all (or most) of the particles are
at one end of the box, a cut may be performed in another dimension to
induce sub-boxes that are more cube-ish (3d) or square-ish (2d) in
shape.
After the cut is made, all the processors are also partitioned into 2
groups, half assigned to the box on the lower side of the cut, and
half to the box on the upper side. (If the processor count is odd,
one side gets an extra processor.) The cut is positioned so that the
number of (weighted) particles in the lower box is exactly the number
that the processors assigned to that box should own for load balance
to be perfect. This also makes load balance for the upper box
perfect. The positioning of the cut is done iteratively, by a
bisectioning method (median search). Note that counting particles on
either side of the cut requires communication between all processors
at each iteration.
the longest dimension, leaving one new box on either side of the cut.
All the processors are also partitioned into 2 groups, half assigned
to the box on the lower side of the cut, and half to the box on the
upper side. (If the processor count is odd, one side gets an extra
processor.) The cut is positioned so that the number of particles in
the lower box is exactly the number that the processors assigned to
that box should own for load balance to be perfect. This also makes
load balance for the upper box perfect. The positioning is done
iteratively, by a bisectioning method. Note that counting particles
on either side of the cut requires communication between all
processors at each iteration.
That is the procedure for the first cut. Subsequent cuts are made
recursively, in exactly the same manner. The subset of processors
assigned to each box make a new cut in one dimension of that box,
splitting the box, the subset of processors, and the particles in the
box in two. The recursion continues until every processor is assigned
a sub-box of the entire simulation domain, and owns the (weighted)
assigned to each box make a new cut in the longest dimension of that
box, splitting the box, the subset of processsors, and the particles
in the box in two. The recursion continues until every processor is
assigned a sub-box of the entire simulation domain, and owns the
particles in that sub-box.
:line
@ -376,7 +368,7 @@ of about 0.8 often results in the best performance, since the number
of neighbors is likely to overestimate the ideal weight.
This weight style is useful for systems where there are different
cutoffs used for different pairs of interactions, or the density
cutoffs used for different pairs of interations, or the density
fluctuates, or a large number of particles are in the vicinity of a
wall, or a combination of these effects. If a simulation uses
multiple neighbor lists, this weight style will use the first suitable
@ -410,7 +402,7 @@ decrease the weights so that the ratio of max weight to min weight
decreases by {factor}. In both cases the intermediate weight values
increase/decrease proportionally as well. A value = 1.0 has no effect
on the {time} weights. As a rule of thumb, effective values to use
are typically between 0.5 and 1.2. Note that the timer quantities
are typicall between 0.5 and 1.2. Note that the timer quantities
mentioned above can be affected by communication which occurs in the
middle of the operations, e.g. pair styles with intermediate exchange
of data witin the force computation, and likewise for KSpace solves.

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@ -82,7 +82,7 @@ internal stress that induces fragmentation :ul
then the interaction between pairs of particles is likely to be more
complex than the summation of simple sub-particle interactions. An
example is contact or frictional forces between particles with planar
surfaces that inter-penetrate.
sufaces that inter-penetrate.
These are additional LAMMPS commands that can be used with body
particles of different styles
@ -105,7 +105,7 @@ in the sections below.
The {nparticle} body style represents body particles as a rigid body
with a variable number N of sub-particles. It is provided as a
vanilla, prototypical example of a body particle, although as
vanillia, prototypical example of a body particle, although as
mentioned above, the "fix rigid"_fix_rigid.html command already
duplicates its functionality.
@ -140,7 +140,7 @@ for more details.
The 6 moments of inertia (ixx,iyy,izz,ixy,ixz,iyz) should be the
values consistent with the current orientation of the rigid body
around its center of mass. The values are with respect to the
simulation box XYZ axes, not with respect to the principal axes of the
simulation box XYZ axes, not with respect to the prinicpal axes of the
rigid body itself. LAMMPS performs the latter calculation internally.
The coordinates of each sub-particle are specified as its x,y,z
displacement from the center-of-mass of the body particle. The
@ -218,7 +218,7 @@ wish; see the "read_data"_read_data.html command for more details.
The 6 moments of inertia (ixx,iyy,izz,ixy,ixz,iyz) should be the
values consistent with the current orientation of the rigid body
around its center of mass. The values are with respect to the
simulation box XYZ axes, not with respect to the principal axes of the
simulation box XYZ axes, not with respect to the prinicpal axes of the
rigid body itself. LAMMPS performs the latter calculation internally.
The coordinates of each vertex are specified as its x,y,z displacement
from the center-of-mass of the body particle. The center-of-mass

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@ -8,7 +8,6 @@
bond_style class2 command :h3
bond_style class2/omp command :h3
bond_style class2/kk command :h3
[Syntax:]

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@ -64,7 +64,7 @@ LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other bond styles, the hybrid bond style does not store bond
coefficient info for individual sub-styles in a "binary restart
files"_restart.html. Thus when restarting a simulation from a restart
files"_restart.html. Thus when retarting a simulation from a restart
file, you need to re-specify bond_coeff commands.
[Related commands:]

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@ -6,25 +6,20 @@
:line
bond_style oxdna/fene command :h3
bond_style oxdna2/fene command :h3
bond_style oxdna_fene command :h3
[Syntax:]
bond_style oxdna/fene :pre
bond_style oxdna2/fene :pre
bond_style oxdna_fene :pre
[Examples:]
bond_style oxdna/fene
bond_style oxdna_fene
bond_coeff * 2.0 0.25 0.7525 :pre
bond_style oxdna2/fene
bond_coeff * 2.0 0.25 0.7564 :pre
[Description:]
The {oxdna/fene} and {oxdna2/fene} bond styles use the potential
The {oxdna_fene} bond style uses the potential
:c,image(Eqs/bond_oxdna_fene.jpg)
@ -41,16 +36,15 @@ epsilon (energy)
Delta (distance)
r0 (distance) :ul
NOTE: The oxDNA bond style has to be used together with the corresponding oxDNA pair styles
for excluded volume interaction {oxdna/excv}, stacking {oxdna/stk}, cross-stacking {oxdna/xstk}
and coaxial stacking interaction {oxdna/coaxstk} as well as hydrogen-bonding interaction {oxdna/hbond} (see also documentation of
"pair_style oxdna/excv"_pair_oxdna.html). For the oxDNA2 "(Snodin)"_#oxdna2 bond style the analogous pair styles and an additional Debye-Hueckel pair
style {oxdna2/dh} have to be defined.
The coefficients in the above example have to be kept fixed and cannot be changed without reparametrizing the entire model.
NOTE: This bond style has to be used together with the corresponding oxDNA pair styles
for excluded volume interaction {oxdna_excv}, stacking {oxdna_stk}, cross-stacking {oxdna_xstk}
and coaxial stacking interaction {oxdna_coaxstk} as well as hydrogen-bonding interaction {oxdna_hbond} (see also documentation of
"pair_style oxdna_excv"_pair_oxdna_excv.html). The coefficients
in the above example have to be kept fixed and cannot be changed without reparametrizing the entire model.
Example input and data files for DNA duplexes can be found in examples/USER/cgdna/examples/oxDNA/ and /oxDNA2/.
Example input and data files can be found in /examples/USER/cgdna/examples/duplex1/ and /duplex2/.
A simple python setup tool which creates single straight or helical DNA strands,
DNA duplexes or arrays of DNA duplexes can be found in examples/USER/cgdna/util/.
DNA duplexes or arrays of DNA duplexes can be found in /examples/USER/cgdna/util/.
A technical report with more information on the model, the structure of the input file,
the setup tool and the performance of the LAMMPS-implementation of oxDNA
can be found "here"_PDF/USER-CGDNA-overview.pdf.
@ -66,7 +60,7 @@ LAMMPS"_Section_start.html#start_3 section for more info on packages.
[Related commands:]
"pair_style oxdna/excv"_pair_oxdna.html, "pair_style oxdna2/excv"_pair_oxdna2.html, "fix nve/dotc/langevin"_fix_nve_dotc_langevin.html, "bond_coeff"_bond_coeff.html
"pair_style oxdna_excv"_pair_oxdna_excv.html, "fix nve/dotc/langevin"_fix_nve_dotc_langevin.html, "bond_coeff"_bond_coeff.html
[Default:] none
@ -74,6 +68,3 @@ LAMMPS"_Section_start.html#start_3 section for more info on packages.
:link(oxdna_fene)
[(Ouldridge)] T.E. Ouldridge, A.A. Louis, J.P.K. Doye, J. Chem. Phys. 134, 085101 (2011).
:link(oxdna2)
[(Snodin)] B.E. Snodin, F. Randisi, M. Mosayebi, et al., J. Chem. Phys. 142, 234901 (2015).

View File

@ -15,8 +15,7 @@ Bond Styles :h1
bond_morse
bond_none
bond_nonlinear
bond_oxdna
bond_oxdna2
bond_oxdna_fene
bond_quartic
bond_table
bond_zero

View File

@ -101,11 +101,11 @@ Instead you could do something like this, assuming the simulation box
is non-periodic and atoms extend from 0 to 20 in all dimensions:
change_box all x final -10 20
create_atoms 1 single -5 5 5 # this will fail to insert an atom :pre
create_atoms 1 single -5 5 5 # this will fail to insert an atom :pre
change_box all x final -10 20 boundary f s s
create_atoms 1 single -5 5 5
change_box all boundary s s s # this will work :pre
change_box boundary s s s # this will work :pre
NOTE: Unlike the earlier "displace_box" version of this command, atom
remapping is NOT performed by default. This command allows remapping
@ -258,8 +258,8 @@ command.
:line
The {ortho} and {triclinic} keywords convert the simulation box to be
orthogonal or triclinic (non-orthogonal). See "this
section"_Section_howto#howto_13 for a discussion of how non-orthogonal
orthogonal or triclinic (non-orthongonal). See "this
section"_Section_howto#howto_13 for a discussion of how non-orthongal
boxes are represented in LAMMPS.
The simulation box is defined as either orthogonal or triclinic when
@ -289,7 +289,7 @@ the create_box command is encountered in the input script.
The {remap} keyword remaps atom coordinates from the last saved box
size/shape to the current box state. For example, if you stretch the
box in the x dimension or tilt it in the xy plane via the {x} and {xy}
keywords, then the {remap} command will dilate or tilt the atoms to
keywords, then the {remap} commmand will dilate or tilt the atoms to
conform to the new box size/shape, as if the atoms moved with the box
as it deformed.

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@ -39,7 +39,7 @@ sizes and shapes. Again there is one tile per processor. To acquire
information for nearby atoms, communication must now be done with a
more complex pattern of neighboring processors.
Note that this command does not actually define a partitioning of the
Note that this command does not actually define a partitoining of the
simulation box (a domain decomposition), rather it determines what
kinds of decompositions are allowed and the pattern of communication
used to enable the decomposition. A decomposition is created when the

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@ -235,7 +235,7 @@ section of "this page"_Section_commands.html#cmd_5.
"temp/ramp"_compute_temp_ramp.html - temperature excluding ramped velocity component
"temp/region"_compute_temp_region.html - temperature of a region of atoms
"temp/sphere"_compute_temp_sphere.html - temperature of spherical particles
"ti"_compute_ti.html - thermodynamic integration free energy values
"ti"_compute_ti.html - thermodyanmic integration free energy values
"torque/chunk"_compute_torque_chunk.html - torque applied on each chunk
"vacf"_compute_vacf.html - velocity-autocorrelation function of group of atoms
"vcm/chunk"_compute_vcm_chunk.html - velocity of center-of-mass for each chunk

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@ -22,7 +22,7 @@ compute 1 fluid angmom/chunk molchunk :pre
[Description:]
Define a computation that calculates the angular momentum of multiple
Define a computation that calculates the angular momemtum of multiple
chunks of atoms.
In LAMMPS, chunks are collections of atoms defined by a "compute

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@ -18,8 +18,8 @@ lattice = {fcc} or {bcc} or N = # of neighbors per atom to include :l
zero or more keyword/value pairs may be appended :l
keyword = {axes} :l
{axes} value = {no} or {yes}
{no} = do not calculate 3 symmetry axes
{yes} = calculate 3 symmetry axes :pre
{no} = do not calulate 3 symmetry axes
{yes} = calulate 3 symmetry axes :pre
:ule
[Examples:]
@ -108,7 +108,7 @@ symmetry axis, followed by the second, and third symmetry axes in
columns 5-7 and 8-10.
The centrosymmetry values are unitless values >= 0.0. Their magnitude
depends on the lattice style due to the number of contributing neighbor
depends on the lattice style due to the number of contibuting neighbor
pairs in the summation in the formula above. And it depends on the
local defects surrounding the central atom, as described above. For
the {axes yes} case, the vector components are also unitless, since

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@ -148,9 +148,7 @@ described further below where the keywords are discussed.
The {binning} styles perform a spatial binning of atoms, and assign an
atom the chunk ID corresponding to the bin number it is in. {Nchunk}
is set to the number of bins, which can change if the simulation box
size changes. This also depends on the setting of the {units}
keyword; e.g. for {reduced} units the number of chunks may not change
even if the box size does.
size changes.
The {bin/1d}, {bin/2d}, and {bin/3d} styles define bins as 1d layers
(slabs), 2d pencils, or 3d boxes. The {dim}, {origin}, and {delta}
@ -388,7 +386,7 @@ If {compress yes} is set, and the {compress} keyword comes before the
{limit} keyword, the compression operation is performed first, as
described below, which resets {Nchunk}. The {limit} keyword is then
applied to the new {Nchunk} value, exactly as described in the
preceding paragraph. Note that in this case, all atoms will end up
preceeding paragraph. Note that in this case, all atoms will end up
with chunk IDs <= {Nc}, but their original values (e.g. molecule ID or
compute/fix/variable value) may have been > {Nc}, because of the
compression operation.
@ -461,7 +459,7 @@ The original chunk IDs (before renumbering) can be accessed by the
which outputs the original IDs as one of the columns in its global
output array. For example, using the "compute cluster/atom" command
discussed above, the original 5 unique chunk IDs might be atom IDs
(27,4982,58374,857838,1000000). After compression, these will be
(27,4982,58374,857838,1000000). After compresion, these will be
renumbered to (1,2,3,4,5). The original values (27,...,1000000) can
be output to a file by the "fix ave/chunk"_fix_ave_chunk.html command,
or by using the "fix ave/time"_fix_ave_time.html command in
@ -540,7 +538,7 @@ is set to {yes}, an out-of-domain atom will have its chunk ID set to
to the first or last bin in both the radial and axis dimensions. If
{discard} is set to {mixed}, which is the default, the radial
dimension is treated the same as for {discard} = no. But for the axis
dimension, it will only have its chunk ID set to the first or last
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
dimension. This is the case if the {bound} keyword settings are
{lower} and {upper}, which is the default. If the {bound} keyword

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@ -42,7 +42,7 @@ performed on mono-component systems.
The CNA calculation can be sensitive to the specified cutoff value.
You should insure the appropriate nearest neighbors of an atom are
found within the cutoff distance for the presumed crystal structure.
found within the cutoff distance for the presumed crystal strucure.
E.g. 12 nearest neighbor for perfect FCC and HCP crystals, 14 nearest
neighbors for perfect BCC crystals. These formulas can be used to
obtain a good cutoff distance:

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@ -25,7 +25,7 @@ Define a computation that calculates the center-of-mass of the group
of atoms, including all effects due to atoms passing thru periodic
boundaries.
A vector of three quantities is calculated by this compute, which
A vector of three quantites is calculated by this compute, which
are the x,y,z coordinates of the center of mass.
NOTE: The coordinates of an atom contribute to the center-of-mass in

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@ -64,13 +64,13 @@ defined by the orientational order parameter calculated by the
"compute orientorder/atom"_compute_orientorder_atom.html command.
This {cstyle} thus allows one to apply the ten Wolde's criterion to
identify crystal-like atoms in a system, as discussed in "ten
Wolde"_#tenWolde1.
Wolde"_#tenWolde.
The ID of the previously specified "compute
orientorder/atom"_compute_orientorder/atom command is specified as
{orientorderID}. The compute must invoke its {components} option to
calculate components of the {Ybar_lm} vector for each atoms, as
described in its documentation. Note that orientorder/atom compute
described in its documenation. Note that orientorder/atom compute
defines its own criteria for identifying neighboring atoms. If the
scalar product ({Ybar_lm(i)},{Ybar_lm(j)}), calculated by the
orientorder/atom compute is larger than the specified {threshold},
@ -127,6 +127,6 @@ explained above.
:line
:link(tenWolde1)
:link(tenWolde)
[(tenWolde)] P. R. ten Wolde, M. J. Ruiz-Montero, D. Frenkel,
J. Chem. Phys. 104, 9932 (1996).

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@ -47,7 +47,7 @@ any command that uses per-atom values from a compute as input. See
"Section 6.15"_Section_howto.html#howto_15 for an overview of
LAMMPS output options.
The per-atom vector values are unitless numbers (damage) >= 0.0.
The per-atom vector values are unitlesss numbers (damage) >= 0.0.
[Restrictions:]

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@ -50,7 +50,7 @@ This compute calculates a per-atom vector, which can be accessed by
any command that uses per-atom values from a compute as input. See
Section_howto 15 for an overview of LAMMPS output options.
The per-atom vector values are unitless numbers (theta) >= 0.0.
The per-atom vector values are unitlesss numbers (theta) >= 0.0.
[Restrictions:]

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@ -25,7 +25,7 @@ Define a computation that calculates the current displacement of each
atom in the group from its original coordinates, including all effects
due to atoms passing thru periodic boundaries.
A vector of four quantities per atom is calculated by this compute.
A vector of four quantites per atom is calculated by this compute.
The first 3 elements of the vector are the dx,dy,dz displacements.
The 4th component is the total displacement, i.e. sqrt(dx*dx + dy*dy +
dz*dz).

View File

@ -64,7 +64,7 @@ command.
:line
:link(Larentzos1)
:link(Larentzos)
[(Larentzos)] J.P. Larentzos, J.K. Brennan, J.D. Moore, and
W.D. Mattson, "LAMMPS Implementation of Constant Energy Dissipative
Particle Dynamics (DPD-E)", ARL-TR-6863, U.S. Army Research

View File

@ -59,7 +59,7 @@ command.
:line
:link(Larentzos2)
:link(Larentzos)
[(Larentzos)] J.P. Larentzos, J.K. Brennan, J.D. Moore, and
W.D. Mattson, "LAMMPS Implementation of Constant Energy Dissipative
Particle Dynamics (DPD-E)", ARL-TR-6863, U.S. Army Research

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@ -14,7 +14,7 @@ compute ID group-ID event/displace threshold :pre
ID, group-ID are documented in "compute"_compute.html command
event/displace = style name of this compute command
threshold = minimum distance any particle must move to trigger an event (distance units) :ul
threshold = minimum distance anyparticle must move to trigger an event (distance units) :ul
[Examples:]
@ -37,7 +37,7 @@ further than the threshold distance.
NOTE: If the system is undergoing significant center-of-mass motion,
due to thermal motion, an external force, or an initial net momentum,
then this compute will not be able to distinguish that motion from
local atom displacements and may generate "false positives."
local atom displacements and may generate "false postives."
[Output info:]

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@ -55,7 +55,7 @@ M is the actual length of the input vector, then an output value of
0.0 is assigned to the atom.
An example of how this command is useful, is in the context of
"chunks" which are static or dynamic subsets of atoms. The "compute
"chunks" which are static or dyanmic subsets of atoms. The "compute
chunk/atom"_compute_chunk_atom.html command assigns unique chunk IDs
to each atom. It's output can be used as the {index} parameter for
this command. Various other computes with "chunk" in their style
@ -192,7 +192,7 @@ reference thermodynamic keywords and various other attributes of
atoms, or invoke other computes, fixes, or variables when they are
evaluated, so this is a very general means of generating a vector of
global quantities which the {index} parameter will reference for
assignment of global values to atoms.
assignement of global values to atoms.
:line
@ -207,7 +207,7 @@ See "Section 6.15"_Section_howto.html#howto_15 for an overview of
LAMMPS output options.
The per-atom vector or array values will be in whatever units the
corresponding input values are in.
corresponsing input values are in.
[Restrictions:] none

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@ -16,11 +16,10 @@ ID, group-ID are documented in "compute"_compute.html command :ulb,l
group/group = style name of this compute command :l
group2-ID = group ID of second (or same) group :l
zero or more keyword/value pairs may be appended :l
keyword = {pair} or {kspace} or {boundary} or {molecule} :l
keyword = {pair} or {kspace} or {boundary} :l
{pair} value = {yes} or {no}
{kspace} value = {yes} or {no}
{boundary} value = {yes} or {no}
{molecule} value = {off} or {inter} or {intra} :pre
{boundary} value = {yes} or {no} :pre
:ule
[Examples:]
@ -47,13 +46,6 @@ NOTE: The energies computed by the {pair} keyword do not include tail
corrections, even if they are enabled via the
"pair_modify"_pair_modify.html command.
If the {molecule} keyword is set to {inter} or {intra} than an
additional check is made based on the molecule IDs of the two atoms in
each pair before including their pairwise interaction energy and
force. For the {inter} setting, the two atoms must be in different
molecules. For the {intra} setting, the two atoms must be in the same
molecule.
If the {kspace} keyword is set to {yes}, which is not the default, and
if a "kspace_style"_kspace_style.html is defined, then the interaction
energy will include a Kspace component which is the long-range
@ -74,10 +66,6 @@ affect the force calculation and will be zero if one or both of the
groups are charge neutral. This energy correction term is the same as
that included in the regular Ewald and PPPM routines.
NOTE: The {molecule} setting only affects the group/group
contributions calculated by the {pair} keyword. It does not affect
the group/group contributions calculated by the {kspace} keyword.
This compute does not calculate any bond or angle or dihedral or
improper interactions between atoms in the two groups.
@ -90,22 +78,6 @@ work (FFTs, Ewald summation) as computing long-range forces for the
entire system. Thus it can be costly to invoke this compute too
frequently.
NOTE: If you have a bonded system, then the settings of
"special_bonds"_special_bonds.html command can remove pairwise
interactions between atoms in the same bond, angle, or dihedral. This
is the default setting for the "special_bonds"_special_bonds.html
command, and means those pairwise interactions do not appear in the
neighbor list. Because this compute uses a neighbor list, it also
means those pairs will not be included in the group/group interaction.
This does not apply when using long-range coulomb interactions
({coul/long}, {coul/msm}, {coul/wolf} or similar. One way to get
around this would be to set special_bond scaling factors to very tiny
numbers that are not exactly zero (e.g. 1.0e-50). Another workaround
is to write a dump file, and use the "rerun"_rerun.html command to
compute the group/group interactions for snapshots in the dump file.
The rerun script can use a "special_bonds"_special_bonds.html command
that includes all pairs in the neighbor list.
If you desire a breakdown of the interactions into a pairwise and
Kspace component, simply invoke the compute twice with the appropriate
yes/no settings for the {pair} and {kspace} keywords. This is no more
@ -147,8 +119,7 @@ The {ewald} and {pppm} styles do.
[Default:]
The option defaults are pair = yes, kspace = no, boundary = yes,
molecule = off.
The option defaults are pair = yes, kspace = no, and boundary = yes.
:line

View File

@ -38,7 +38,7 @@ subtracted to a group of atoms.
The compute takes three arguments which are IDs of other
"computes"_compute.html. One calculates per-atom kinetic energy
({ke-ID}), one calculates per-atom potential energy ({pe-ID)}, and the
third calculates per-atom stress ({stress-ID}).
third calcualtes per-atom stress ({stress-ID}).
NOTE: These other computes should provide values for all the atoms in
the group this compute specifies. That means the other computes could
@ -83,7 +83,7 @@ The heat flux can be output every so many timesteps (e.g. via the
post-processing operation, an autocorrelation can be performed, its
integral estimated, and the Green-Kubo formula above evaluated.
The "fix ave/correlate"_fix_ave_correlate.html command can calculate
The "fix ave/correlate"_fix_ave_correlate.html command can calclate
the autocorrelation. The trap() function in the
"variable"_variable.html command can calculate the integral.

View File

@ -35,7 +35,7 @@ chunk/atom"_compute_chunk_atom.html doc page and "Section
defined and examples of how they can be used to measure properties of
a system.
This compute calculates the 6 components of the symmetric inertia
This compute calculates the 6 components of the symmetric intertia
tensor for each chunk, ordered Ixx,Iyy,Izz,Ixy,Iyz,Ixz. The
calculation includes all effects due to atoms passing thru periodic
boundaries.

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@ -14,29 +14,27 @@ compute_modify compute-ID keyword value ... :pre
compute-ID = ID of the compute to modify :ulb,l
one or more keyword/value pairs may be listed :l
keyword = {extra/dof} or {extra} or {dynamic/dof} or {dynamic} :l
{extra/dof} value = N
keyword = {extra} or {dynamic} :l
{extra} value = N
N = # of extra degrees of freedom to subtract
{extra} syntax is identical to {extra/dof}, will be disabled at some point
{dynamic/dof} value = {yes} or {no}
yes/no = do or do not recompute the number of degrees of freedom (DOF) contributing to the temperature
{dynamic} syntax is identical to {dynamic/dof}, will be disabled at some point :pre
{dynamic} value = {yes} or {no}
yes/no = do or do not recompute the number of atoms contributing to the temperature :pre
:ule
[Examples:]
compute_modify myTemp extra/dof 0
compute_modify newtemp dynamic/dof yes extra/dof 600 :pre
compute_modify myTemp extra 0
compute_modify newtemp dynamic yes extra 600 :pre
[Description:]
Modify one or more parameters of a previously defined compute. Not
all compute styles support all parameters.
The {extra/dof} or {extra} keyword refers to how many
degrees-of-freedom are subtracted (typically from 3N) as a normalizing
factor in a temperature computation. Only computes that compute a
temperature use this option. The default is 2 or 3 for "2d or 3d
The {extra} keyword refers to how many degrees-of-freedom are
subtracted (typically from 3N) as a normalizing factor in a
temperature computation. Only computes that compute a temperature use
this option. The default is 2 or 3 for "2d or 3d
systems"_dimension.html which is a correction factor for an ensemble
of velocities with zero total linear momentum. For compute
temp/partial, if one or more velocity components are excluded, the
@ -45,21 +43,14 @@ number for the {extra} parameter if you need to add
degrees-of-freedom. See the "compute
temp/asphere"_compute_temp_asphere.html command for an example.
The {dynamic/dof} or {dynamic} keyword determines whether the number
of atoms N in the compute group and their associated degrees of
freedom are re-computed each time a temperature is computed. Only
compute styles that calculate a temperature use this option. By
default, N and their DOF are assumed to be constant. If you are
adding atoms or molecules to the system (see the "fix
pour"_fix_pour.html, "fix deposit"_fix_deposit.html, and "fix
gcmc"_fix_gcmc.html commands) or expect atoms or molecules to be lost
(e.g. due to exiting the simulation box or via "fix
evaporate"_fix_evaporate.html), then this option should be used to
insure the temperature is correctly normalized.
NOTE: The {extra} and {dynamic} keywords should not be used as they
are deprecated (March 2017) and will eventually be disabled. Instead,
use the equivalent {extra/dof} and {dynamic/dof} keywords.
The {dynamic} keyword determines whether the number of atoms N in the
compute group is re-computed each time a temperature is computed.
Only compute styles that calculate a temperature use this option. By
default, N is assumed to be constant. If you are adding atoms to the
system (see the "fix pour"_fix_pour.html or "fix
deposit"_fix_deposit.html commands) or expect atoms to be lost
(e.g. due to evaporation), then this option should be used to insure
the temperature is correctly normalized.
[Restrictions:] none
@ -69,5 +60,5 @@ use the equivalent {extra/dof} and {dynamic/dof} keywords.
[Default:]
The option defaults are extra/dof = 2 or 3 for 2d or 3d systems and
dynamic/dof = no.
The option defaults are extra = 2 or 3 for 2d or 3d systems and
dynamic = no.

View File

@ -33,7 +33,7 @@ passing thru periodic boundaries. For computation of the non-Gaussian
parameter of mean-squared displacement, see the "compute
msd/nongauss"_compute_msd_nongauss.html command.
A vector of four quantities is calculated by this compute. The first 3
A vector of four quantites is calculated by this compute. The first 3
elements of the vector are the squared dx,dy,dz displacements, summed
and averaged over atoms in the group. The 4th element is the total
squared displacement, i.e. (dx*dx + dy*dy + dz*dz), summed and

View File

@ -35,7 +35,7 @@ chunk/atom"_compute_chunk_atom.html doc page and "Section
defined and examples of how they can be used to measure properties of
a system.
Four quantities are calculated by this compute for each chunk. The
Four quantites are calculated by this compute for each chunk. The
first 3 quantities are the squared dx,dy,dz displacements of the
center-of-mass. The 4th component is the total squared displacement,
i.e. (dx*dx + dy*dy + dz*dz) of the center-of-mass. These

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@ -30,12 +30,12 @@ Define a computation that calculates the mean-squared displacement
(MSD) and non-Gaussian parameter (NGP) of the group of atoms,
including all effects due to atoms passing thru periodic boundaries.
A vector of three quantities is calculated by this compute. The first
A vector of three quantites is calculated by this compute. The first
element of the vector is the total squared dx,dy,dz displacements
drsquared = (dx*dx + dy*dy + dz*dz) of atoms, and the second is the
fourth power of these displacements drfourth = (dx*dx + dy*dy +
dz*dz)*(dx*dx + dy*dy + dz*dz), summed and averaged over atoms in the
group. The 3rd component is the nonGaussian diffusion parameter NGP =
group. The 3rd component is the nonGaussian diffusion paramter NGP =
3*drfourth/(5*drsquared*drsquared), i.e.
:c,image(Eqs/compute_msd_nongauss.jpg)
@ -48,7 +48,7 @@ others.
If the {com} option is set to {yes} then the effect of any drift in
the center-of-mass of the group of atoms is subtracted out before the
displacment of each atom is calculated.
displacment of each atom is calcluated.
See the "compute msd"_compute_msd.html doc page for further important
NOTEs, which also apply to this compute.

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@ -78,7 +78,7 @@ normalized complex vector {Ybar_lm} of degree {ldegree}, which must be
explicitly included in the keyword {degrees}. This option can be used
in conjunction with "compute coord_atom"_compute_coord_atom.html to
calculate the ten Wolde's criterion to identify crystal-like
particles, as discussed in "ten Wolde"_#tenWolde2.
particles, as discussed in "ten Wolde"_#tenWolde.
The value of {Ql} is set to zero for atoms not in the
specified compute group, as well as for atoms that have less than
@ -143,6 +143,6 @@ Phys. Rev. B 28, 784 (1983).
[(Mickel)] W. Mickel, S. C. Kapfer, G. E. Schroeder-Turkand, K. Mecke,
J. Chem. Phys. 138, 044501 (2013).
:link(tenWolde2)
:link(tenWolde)
[(tenWolde)] P. R. ten Wolde, M. J. Ruiz-Montero, D. Frenkel,
J. Chem. Phys. 104, 9932 (1996).

View File

@ -43,7 +43,7 @@ style van der Waals interaction or not) is tallied in {evdwl}. If
as a global scalar by this compute. This is useful when using
"pair_style hybrid"_pair_hybrid.html if you want to know the portion
of the total energy contributed by one sub-style. If {evalue} is
specified as {evdwl} or {ecoul}, then just that portion of the energy
specfied as {evdwl} or {ecoul}, then just that portion of the energy
is stored as a global scalar.
NOTE: The energy returned by the {evdwl} keyword does not include tail
@ -52,7 +52,7 @@ corrections, even if they are enabled via the
Some pair styles tally additional quantities, e.g. a breakdown of
potential energy into a dozen or so components is tallied by the
"pair_style reax"_pair_reax.html command. These values (1 or more)
"pair_style reax"_pair_reax.html commmand. These values (1 or more)
are stored as a global vector by this compute. See the doc page for
"individual pair styles"_pair_style.html for info on these values.

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@ -47,7 +47,7 @@ force cutoff distance for that interaction, as defined by the
"pair_style"_pair_style.html and "pair_coeff"_pair_coeff.html
commands.
The value {dist} is the distance between the pair of atoms.
The value {dist} is the distance bewteen the pair of atoms.
The value {eng} is the interaction energy for the pair of atoms.

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@ -49,9 +49,9 @@ pairwise interactions between 1-4 atoms. The energy contribution of
these terms is included in the pair energy, not the dihedral energy.
The KSpace contribution is calculated using the method in
"(Heyes)"_#Heyes1 for the Ewald method and a related method for PPPM,
"(Heyes)"_#Heyes for the Ewald method and a related method for PPPM,
as specified by the "kspace_style pppm"_kspace_style.html command.
For PPPM, the calculation requires 1 extra FFT each timestep that
For PPPM, the calcluation requires 1 extra FFT each timestep that
per-atom energy is calculated. This "document"_PDF/kspace.pdf
describes how the long-range per-atom energy calculation is performed.
@ -97,5 +97,5 @@ stress/atom"_compute_stress_atom.html
:line
:link(Heyes1)
:link(Heyes)
[(Heyes)] Heyes, Phys Rev B 49, 755 (1994),

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@ -44,7 +44,7 @@ This compute calculates a per-atom vector, which can be accessed by
any command that uses per-atom values from a compute as input. See
Section_howto 15 for an overview of LAMMPS output options.
The per-atom vector values are unitless numbers (lambda) >= 0.0.
The per-atom vector values are unitlesss numbers (lambda) >= 0.0.
[Restrictions:]

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@ -70,7 +70,7 @@ means include all terms except the kinetic energy {ke}.
Details of how LAMMPS computes the virial efficiently for the entire
system, including for manybody potentials and accounting for the
effects of periodic boundary conditions are discussed in
"(Thompson)"_#Thompson1.
"(Thompson)"_#Thompson.
The temperature and kinetic energy tensor is not calculated by this
compute, but rather by the temperature compute specified with the
@ -89,7 +89,7 @@ commands"_compute.html to determine which ones include a bias.
Also note that the N in the first formula above is really
degrees-of-freedom divided by d = dimensionality, where the DOF value
is calculated by the temperature compute. See the various "compute
is calcluated by the temperature compute. See the various "compute
temperature"_compute.html styles for details.
A compute of this style with the ID of "thermo_press" is created when
@ -150,5 +150,5 @@ stress/atom"_compute_stress_atom.html,
:line
:link(Thompson1)
:link(Thompson)
[(Thompson)] Thompson, Plimpton, Mattson, J Chem Phys, 131, 154107 (2009).

View File

@ -64,7 +64,7 @@ can only be used if the {compress} keyword was set to {yes} for the
"compute chunk/atom"_compute_chunk_atom.html command referenced by
chunkID. This means that the original chunk IDs (e.g. molecule IDs)
will have been compressed to remove chunk IDs with no atoms assigned
to them. Thus a compressed chunk ID of 3 may correspond to an original
to them. Thus a compresed chunk ID of 3 may correspond to an original
chunk ID (molecule ID in this case) of 415. The {id} attribute will
then be 415 for the 3rd chunk.

View File

@ -10,27 +10,21 @@ compute rdf command :h3
[Syntax:]
compute ID group-ID rdf Nbin itype1 jtype1 itype2 jtype2 ... keyword/value ... :pre
compute ID group-ID rdf Nbin itype1 jtype1 itype2 jtype2 ... :pre
ID, group-ID are documented in "compute"_compute.html command :ulb,l
rdf = style name of this compute command :l
Nbin = number of RDF bins :l
itypeN = central atom type for Nth RDF histogram (see asterisk form below) :l
jtypeN = distribution atom type for Nth RDF histogram (see asterisk form below) :l
zero or more keyword/value pairs may be appended :l
keyword = {cutoff} :l
{cutoff} value = Rcut
Rcut = cutoff distance for RDF computation (distance units) :pre
:ule
ID, group-ID are documented in "compute"_compute.html command
rdf = style name of this compute command
Nbin = number of RDF bins
itypeN = central atom type for Nth RDF histogram (see asterisk form below)
jtypeN = distribution atom type for Nth RDF histogram (see asterisk form below) :ul
[Examples:]
compute 1 all rdf 100
compute 1 all rdf 100 1 1
compute 1 all rdf 100 * 3 cutoff 5.0
compute 1 all rdf 100 * 3
compute 1 fluid rdf 500 1 1 1 2 2 1 2 2
compute 1 fluid rdf 500 1*3 2 5 *10 cutoff 3.5 :pre
compute 1 fluid rdf 500 1*3 2 5 *10 :pre
[Description:]
@ -38,8 +32,7 @@ Define a computation that calculates the radial distribution function
(RDF), also called g(r), and the coordination number for a group of
particles. Both are calculated in histogram form by binning pairwise
distances into {Nbin} bins from 0.0 to the maximum force cutoff
defined by the "pair_style"_pair_style.html command or the cutoff
distance {Rcut} specified via the {cutoff} keyword. The bins are of
defined by the "pair_style"_pair_style.html command. The bins are of
uniform size in radial distance. Thus a single bin encompasses a thin
shell of distances in 3d and a thin ring of distances in 2d.
@ -48,41 +41,17 @@ NOTE: If you have a bonded system, then the settings of
interactions between atoms in the same bond, angle, or dihedral. This
is the default setting for the "special_bonds"_special_bonds.html
command, and means those pairwise interactions do not appear in the
neighbor list. Because this fix uses a neighbor list, it also means
neighbor list. Because this fix uses the neighbor list, it also means
those pairs will not be included in the RDF. This does not apply when
using long-range coulomb interactions ({coul/long}, {coul/msm},
{coul/wolf} or similar. One way to get around this would be to set
special_bond scaling factors to very tiny numbers that are not exactly
zero (e.g. 1.0e-50). Another workaround is to write a dump file, and
use the "rerun"_rerun.html command to compute the RDF for snapshots in
the dump file. The rerun script can use a
using long-range coulomb ({coul/long}, {coul/msm}, {coul/wolf} or
similar. One way to get around this would be to set special_bond
scaling factors to very tiny numbers that are not exactly zero
(e.g. 1.0e-50). Another workaround is to write a dump file, and use
the "rerun"_rerun.html command to compute the RDF for snapshots in the
dump file. The rerun script can use a
"special_bonds"_special_bonds.html command that includes all pairs in
the neighbor list.
By default the RDF is computed out to the maximum force cutoff defined
by the "pair_style"_pair_style.html command. If the {cutoff} keyword
is used, then the RDF is computed accurately out to the {Rcut} > 0.0
distance specified.
NOTE: Normally, you should only use the {cutoff} keyword if no pair
style is defined, e.g. the "rerun"_rerun.html command is being used to
post-process a dump file of snapshots. Or if you really want the RDF
for distances beyond the pair_style force cutoff and cannot easily
post-process a dump file to calculate it. This is because using the
{cutoff} keyword incurs extra computation and possibly communication,
which may slow down your simulation. If you specify a {Rcut} <= force
cutoff, you will force an additional neighbor list to be built at
every timestep this command is invoked (or every reneighboring
timestep, whichever is less frequent), which is inefficient. LAMMPS
will warn you if this is the case. If you specify a {Rcut} > force
cutoff, you must insure ghost atom information out to {Rcut} + {skin}
is communicated, via the "comm_modify cutoff"_comm_modify.html
command, else the RDF computation cannot be performed, and LAMMPS will
give an error message. The {skin} value is what is specified with the
"neighbor"_neighbor.html command. In this case, you are forcing a
large neighbor list to be built just for the RDF computation, and
extra communication to be performed every timestep.
The {itypeN} and {jtypeN} arguments are optional. These arguments
must come in pairs. If no pairs are listed, then a single histogram
is computed for g(r) between all atom types. If one or more pairs are
@ -184,6 +153,4 @@ change from zero to one at the location of the spike in g(r).
"fix ave/time"_fix_ave_time.html
[Default:]
The keyword defaults are cutoff = 0.0 (use the pairwise force cutoff).
[Default:] none

View File

@ -123,7 +123,7 @@ The {vx}, {vy}, {vz}, {fx}, {fy}, {fz} attributes are components of
the COM velocity and force on the COM of the body.
The {omegax}, {omegay}, and {omegaz} attributes are the angular
velocity components of the body around its COM.
velocity componennts of the body around its COM.
The {angmomx}, {angmomy}, and {angmomz} attributes are the angular
momentum components of the body around its COM.

View File

@ -93,7 +93,7 @@ parameters will denote the z1=h, z2=k, and z3=l (in a global since)
zone axis of an intersecting Ewald sphere. Diffraction intensities
will only be computed at the intersection of the reciprocal lattice
mesh and a {dR_Ewald} thick surface of the Ewald sphere. See the
example 3D intensity data and the intersection of a \[010\] zone axis
example 3D intestiety data and the intersection of a \[010\] zone axis
in the below image.
:c,image(JPG/saed_ewald_intersect_small.jpg,JPG/saed_ewald_intersect.jpg)

View File

@ -35,7 +35,7 @@ any command that uses per-particle values from a compute as input.
See "Section 6.15"_Section_howto.html#howto_15 for an overview of
LAMMPS output options.
The per-particle values will be given dimensionless, see "units"_units.html.
The per-particle values will be given dimentionless, see "units"_units.html.
[Restrictions:]

View File

@ -24,7 +24,7 @@ twojmax = band limit for bispectrum components (non-negative integer) :l
R_1, R_2,... = list of cutoff radii, one for each type (distance units) :l
w_1, w_2,... = list of neighbor weights, one for each type :l
zero or more keyword/value pairs may be appended :l
keyword = {diagonal} or {rmin0} or {switchflag} or {bzeroflag} :l
keyword = {diagonal} or {rmin0} or {switchflag} :l
{diagonal} value = {0} or {1} or {2} or {3}
{0} = all j1, j2, j <= twojmax, j2 <= j1
{1} = subset satisfying j1 == j2
@ -33,10 +33,7 @@ keyword = {diagonal} or {rmin0} or {switchflag} or {bzeroflag} :l
{rmin0} value = parameter in distance to angle conversion (distance units)
{switchflag} value = {0} or {1}
{0} = do not use switching function
{1} = use switching function
{bzeroflag} value = {0} or {1}
{0} = do not subtract B0
{1} = subtract B0 :pre
{1} = use switching function :pre
:ule
[Examples:]
@ -53,12 +50,12 @@ for each atom in a group.
Bispectrum components of an atom are order parameters characterizing
the radial and angular distribution of neighbor atoms. The detailed
mathematical definition is given in the paper by Thompson et
al. "(Thompson)"_#Thompson20141
al. "(Thompson)"_#Thompson2014
The position of a neighbor atom {i'} relative to a central atom {i} is
a point within the 3D ball of radius {R_ii' = rcutfac*(R_i + R_i')}
Bartok et al. "(Bartok)"_#Bartok20101, proposed mapping this 3D ball
Bartok et al. "(Bartok)"_#Bartok2010, proposed mapping this 3D ball
onto the 3-sphere, the surface of the unit ball in a four-dimensional
space. The radial distance {r} within {R_ii'} is mapped on to a third
polar angle {theta0} defined by,
@ -95,7 +92,7 @@ The expansion coefficients {u^j_m,m'} are complex-valued and they are
not directly useful as descriptors, because they are not invariant
under rotation of the polar coordinate frame. However, the following
scalar triple products of expansion coefficients can be shown to be
real-valued and invariant under rotation "(Bartok)"_#Bartok20101.
real-valued and invariant under rotation "(Bartok)"_#Bartok2010.
:c,image(Eqs/compute_sna_atom3.jpg)
@ -156,12 +153,6 @@ ordered in which they are listed
The keyword {switchflag} can be used to turn off the switching
function.
The keyword {bzeroflag} determines whether or not {B0}, the bispectrum
components of an atom with no neighbors, are subtracted from
the calculated bispectrum components. This optional keyword is only
available for compute {sna/atom}, as {snad/atom} and {snav/atom}
are unaffected by the removal of constant terms.
NOTE: If you have a bonded system, then the settings of
"special_bonds"_special_bonds.html command can remove pairwise
interactions between atoms in the same bond, angle, or dihedral. This
@ -231,15 +222,15 @@ LAMMPS"_Section_start.html#start_3 section for more info.
[Default:]
The optional keyword defaults are {diagonal} = 0, {rmin0} = 0,
{switchflag} = 1, {bzeroflag} = 0.
{switchflag} = 1.
:line
:link(Thompson20141)
:link(Thompson2014)
[(Thompson)] Thompson, Swiler, Trott, Foiles, Tucker, under review, preprint
available at "arXiv:1409.3880"_http://arxiv.org/abs/1409.3880
:link(Bartok20101)
:link(Bartok2010)
[(Bartok)] Bartok, Payne, Risi, Csanyi, Phys Rev Lett, 104, 136403 (2010).
:link(Meremianin2006)

View File

@ -74,7 +74,7 @@ other atoms in the simulation, not just with other atoms in the group.
Details of how LAMMPS computes the virial for individual atoms for
either pairwise or manybody potentials, and including the effects of
periodic boundary conditions is discussed in "(Thompson)"_#Thompson2.
periodic boundary conditions is discussed in "(Thompson)"_#Thompson.
The basic idea for manybody potentials is to treat each component of
the force computation between a small cluster of atoms in the same
manner as in the formula above for bond, angle, dihedral, etc
@ -89,10 +89,10 @@ pairwise interactions between 1-4 atoms. The virial contribution of
these terms is included in the pair virial, not the dihedral virial.
The KSpace contribution is calculated using the method in
"(Heyes)"_#Heyes2 for the Ewald method and by the methodology described
in "(Sirk)"_#Sirk1 for PPPM. The choice of KSpace solver is specified
"(Heyes)"_#Heyes for the Ewald method and by the methodology described
in "(Sirk)"_#Sirk for PPPM. The choice of KSpace solver is specified
by the "kspace_style pppm"_kspace_style.html command. Note that for
PPPM, the calculation requires 6 extra FFTs each timestep that
PPPM, the calcluation requires 6 extra FFTs each timestep that
per-atom stress is calculated. Thus it can significantly increase the
cost of the PPPM calculation if it is needed on a large fraction of
the simulation timesteps.
@ -159,11 +159,11 @@ The per-atom array values will be in pressure*volume
:line
:link(Heyes2)
:link(Heyes)
[(Heyes)] Heyes, Phys Rev B 49, 755 (1994),
:link(Sirk1)
:link(Sirk)
[(Sirk)] Sirk, Moore, Brown, J Chem Phys, 138, 064505 (2013).
:link(Thompson2)
:link(Thompson)
[(Thompson)] Thompson, Plimpton, Mattson, J Chem Phys, 131, 154107 (2009).

2
doc/src/compute_temp_asphere.txt Normal file → Executable file
View File

@ -138,7 +138,7 @@ This compute is part of the ASPHERE 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.
This compute requires that atoms store angular momentum and a
This compute requires that atoms store angular momementum and a
quaternion as defined by the "atom_style ellipsoid"_atom_style.html
command.

2
doc/src/compute_temp_body.txt Normal file → Executable file
View File

@ -120,7 +120,7 @@ This compute is part of the BODY 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.
This compute requires that atoms store angular momentum and a
This compute requires that atoms store angular momementum and a
quaternion as defined by the "atom_style body"_atom_style.html
command.

View File

@ -44,7 +44,7 @@ compute 1 fluid temp/chunk molchunk bias tpartial adof 2.0 :pre
Define a computation that calculates the temperature of a group of
atoms that are also in chunks, after optionally subtracting out the
center-of-mass velocity of each chunk. By specifying optional values,
it can also calculate the per-chunk temperature or energies of the
it can also calulate the per-chunk temperature or energies of the
multiple chunks of atoms.
In LAMMPS, chunks are collections of atoms defined by a "compute
@ -122,7 +122,7 @@ concept is somewhat ill-defined. In some cases, you can use the
{adof} and {cdof} keywords to adjust the calculated degress of freedom
appropriately, as explained below.
Note that the per-chunk temperature calculated by this compute and the
Note that the per-chunk temperature calulated by this compute and the
"fix ave/chunk temp"_fix_ave_chunk.html command can be different.
This compute calculates the temperature for each chunk for a single
snapshot. Fix ave/chunk can do that but can also time average those
@ -208,7 +208,7 @@ This compute also optionally calculates a global array, if one or more
of the optional values are specified. The number of rows in the array
= the number of chunks {Nchunk} as calculated by the specified
"compute chunk/atom"_compute_chunk_atom.html command. The number of
columns is the number of specified values (1 or more). These values
columns is the number of specifed values (1 or more). These values
can be accessed by any command that uses global array values from a
compute as input. Again, see "Section
6.15"_Section_howto.html#howto_15 for an overview of LAMMPS output

View File

@ -27,7 +27,7 @@ compute core_shells all temp/cs cores shells :pre
Define a computation that calculates the temperature of a system based
on the center-of-mass velocity of atom pairs that are bonded to each
other. This compute is designed to be used with the adiabatic
core/shell model of "(Mitchell and Finchham)"_#MitchellFinchham1. See
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. Specifically, this
compute enables correct temperature calculation and thermostatting of
@ -114,6 +114,6 @@ temp/chunk"_compute_temp_chunk.html
:line
:link(MitchellFinchham1)
:link(MitchellFinchham)
[(Mitchell and Finchham)] Mitchell, Finchham, J Phys Condensed Matter,
5, 1031-1038 (1993).

View File

@ -43,7 +43,7 @@ atoms, after subtracting out a spatially-averaged center-of-mass
velocity field, before computing the kinetic energy. This can be
useful for thermostatting a collection of atoms undergoing a complex
flow, e.g. via a profile-unbiased thermostat (PUT) as described in
"(Evans)"_#Evans1. A compute of this style can be used by any command
"(Evans)"_#Evans. A compute of this style can be used by any command
that computes a temperature, e.g. "thermo_modify"_thermo_modify.html,
"fix temp/rescale"_fix_temp_rescale.html, "fix npt"_fix_nh.html, etc.
@ -75,7 +75,7 @@ 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
subtracted to adjust for the removal of the center-of-mass velocity in
each of Nx*Ny*Nz bins, as discussed in the "(Evans)"_#Evans1 paper.
each of Nx*Ny*Nz bins, as discussed in the "(Evans)"_#Evans paper.
If the {out} keyword is used with a {tensor} value, which is the
default, a kinetic energy tensor, stored as a 6-element vector, is
@ -118,7 +118,7 @@ needed, the subtracted degrees-of-freedom can be altered using the
NOTE: When using the {out} keyword with a value of {bin}, the
calculated temperature for each bin does not include the
degrees-of-freedom adjustment described in the preceding paragraph,
degrees-of-freedom adjustment described in the preceeding paragraph,
for fixes that constrain molecular motion. It does include the
adjustment due to the {extra} option, which is applied to each bin.
@ -126,7 +126,7 @@ See "this howto section"_Section_howto.html#howto_16 of the manual for
a discussion of different ways to compute temperature and perform
thermostatting. Using this compute in conjunction with a
thermostatting fix, as explained there, will effectively implement a
profile-unbiased thermostat (PUT), as described in "(Evans)"_#Evans1.
profile-unbiased thermostat (PUT), as described in "(Evans)"_#Evans.
[Output info:]
@ -178,5 +178,5 @@ The option default is out = tensor.
:line
:link(Evans1)
:link(Evans)
[(Evans)] Evans and Morriss, Phys Rev Lett, 56, 2172-2175 (1986).

0
doc/src/compute_temp_sphere.txt Normal file → Executable file
View File

View File

@ -27,7 +27,7 @@ function (VACF), averaged over a group of atoms. Each atom's
contribution to the VACF is its current velocity vector dotted into
its initial velocity vector at the time the compute was specified.
A vector of four quantities is calculated by this compute. The first 3
A vector of four quantites is calculated by this compute. The first 3
elements of the vector are vx * vx0 (and similarly for the y and z
components), summed and averaged over atoms in the group. Vx is the
current x-component of velocity for the atom, vx0 is the initial

View File

@ -217,10 +217,6 @@ This compute is part of the VORONOI 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.
It also requiers you have a copy of the Voro++ library built and
installed on your system. See instructions on obtaining and
installing the Voro++ software in the src/VORONOI/README file.
[Related commands:]
"dump custom"_dump.html, "dump local"_dump.html

View File

@ -101,7 +101,7 @@ positions.
For the {random} style, N particles are added to the system at
randomly generated coordinates, which can be useful for generating an
amorphous system. The particles are created one by one using the
specified random number {seed}, resulting in the same set of particles
speficied random number {seed}, resulting in the same set of particles
coordinates, independent of how many processors are being used in the
simulation. If the {region-ID} argument is specified as NULL, then
the created particles will be anywhere in the simulation box. If a
@ -134,17 +134,6 @@ not overlap existing atoms inappropriately, especially if molecules
are being added. The "delete_atoms"_delete_atoms.html command can be
used to remove overlapping atoms or molecules.
NOTE: You cannot use any of the styles explained above to create atoms
that are outside the simulation box; they will just be ignored by
LAMMPS. This is true even if you are using shrink-wrapped box
boundaries, as specified by the "boundary"_boundary.html command.
However, you can first use the "change_box"_change_box.html command to
temporarily expand the box, then add atoms via create_atoms, then
finally use change_box command again if needed to re-shrink-wrap the
new atoms. See the "change_box"_change_box.html doc page for an
example of how to do this, using the create_atoms {single} style to
insert a new atom outside the current simulation box.
:line
Individual atoms are inserted by this command, unless the {mol}

View File

@ -10,25 +10,21 @@ dihedral_style charmm command :h3
dihedral_style charmm/intel command :h3
dihedral_style charmm/kk command :h3
dihedral_style charmm/omp command :h3
dihedral_style charmmfsw command :h3
[Syntax:]
dihedral_style style :pre
style = {charmm} or {charmmfsw} :ul
dihedral_style charmm :pre
[Examples:]
dihedral_style charmm
dihedral_style charmmfsw
dihedral_coeff 1 0.2 1 180 1.0
dihedral_coeff 2 1.8 1 0 1.0
dihedral_coeff 1 3.1 2 180 0.5 :pre
[Description:]
The {charmm} and {charmmfsw} dihedral styles use the potential
The {charmm} dihedral style uses the potential
:c,image(Eqs/dihedral_charmm.jpg)
@ -38,16 +34,6 @@ field (see comment on weighting factors below). See
"(Cornell)"_#dihedral-Cornell for a description of the AMBER force
field.
NOTE: The newer {charmmfsw} style was released in March 2017. We
recommend it be used instead of the older {charmm} style when running
a simulation with the CHARMM force field, either with long-range
Coulombics or a Coulomb cutoff, via the "pair_style
lj/charmmfsw/coul/long"_pair_charmm.html and "pair_style
lj/charmmfsw/coul/charmmfsh"_pair_charmm.html commands respectively.
Otherwise the older {charmm} style is fine to use. See the discussion
below and more details on the "pair_style charmm"_pair_charmm.html doc
page.
The following coefficients must be defined for each dihedral type via the
"dihedral_coeff"_dihedral_coeff.html command as in the example above, or in
the data file or restart files read by the "read_data"_read_data.html
@ -87,29 +73,13 @@ special_bonds 1-4 scaling factor to 0.0 (which is the
default). Otherwise 1-4 non-bonded interactions in dihedrals will be
computed twice.
For simulations using the CHARMM force field with a Coulomb cutoff,
the difference between the {charmm} and {charmmfsw} styles is in the
computation of the 1-4 non-bond interactions, though only if the
distance between the two atoms is within the switching region of the
pairwise potential defined by the corresponding CHARMM pair style,
i.e. within the outer cutoff specified for the pair style. The
{charmmfsw} style should only be used when using the corresponding
"pair_style lj/charmmfsw/coul/charmmfsw"_pair_charmm.html or
"pair_style lj/charmmfsw/coul/long"_pair_charmm.html commands. Use
the {charmm} style with the older "pair_style"_pair_charmm.html
commands that have just "charmm" in their style name. See the
discussion on the "CHARMM pair_style"_pair_charmm.html doc page for
details.
Note that for AMBER force fields, which use pair styles with "lj/cut",
the special_bonds 1-4 scaling factor should be set to the AMBER
defaults (1/2 and 5/6) and all the dihedral weighting factors (4th
coeff above) must be set to 0.0. In this case, you can use any pair
style you wish, since the dihedral does not need any Lennard-Jones
parameter information and will not compute any 1-4 non-bonded
interactions. Likewise the {charmm} or {charmmfsw} styles are
identical in this case since no 1-4 non-bonded interactions are
computed.
Also note that for AMBER force fields, which use pair styles with
"lj/cut", the special_bonds 1-4 scaling factor should be set to the
AMBER defaults (1/2 and 5/6) and all the dihedral weighting factors
(4th coeff above) must be set to 0.0. In this case, you can use any
pair style you wish, since the dihedral does not need any
Lennard-Jones parameter information and will not compute any 1-4
non-bonded interactions.
:line

View File

@ -8,7 +8,6 @@
dihedral_style class2 command :h3
dihedral_style class2/omp command :h3
dihedral_style class2/kk command :h3
[Syntax:]

View File

@ -82,7 +82,7 @@ LAMMPS"_Section_start.html#start_3 section for more info on packages.
Unlike other dihedral styles, the hybrid dihedral style does not store
dihedral coefficient info for individual sub-styles in a "binary
restart files"_restart.html. Thus when restarting a simulation from a
restart files"_restart.html. Thus when retarting a simulation from a
restart file, you need to re-specify dihedral_coeff commands.
[Related commands:]

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@ -225,7 +225,7 @@ This bounding box is convenient for many visualization programs. The
meaning of the 6 character flags for "xx yy zz" is the same as above.
Note that the first two numbers on each line are now xlo_bound instead
of xlo, etc, since they represent a bounding box. See "this
of xlo, etc, since they repesent a bounding box. See "this
section"_Section_howto.html#howto_12 of the doc pages for a geometric
description of triclinic boxes, as defined by LAMMPS, simple formulas
for how the 6 bounding box extents (xlo_bound,xhi_bound,etc) are
@ -331,7 +331,10 @@ bonds and colors.
Note that {atom}, {custom}, {dcd}, {xtc}, and {xyz} style dump files
can be read directly by "VMD"_http://www.ks.uiuc.edu/Research/vmd, a
popular molecular viewing program.
popular molecular viewing program. See
"Section 9"_Section_tools.html#vmd of the manual and the
tools/lmp2vmd/README.txt file for more information about support in
VMD for reading and visualizing LAMMPS dump files.
:line
@ -542,7 +545,7 @@ that the coordinate values may be far outside the box bounds printed
with the snapshot. Using {xsu}, {ysu}, {zsu} is similar to using
{xu}, {yu}, {zu}, except that the unwrapped coordinates are scaled by
the box size. Atoms that have passed through a periodic boundary will
have the corresponding coordinate increased or decreased by 1.0.
have the corresponding cooordinate increased or decreased by 1.0.
The image flags can be printed directly using the {ix}, {iy}, {iz}
attributes. For periodic dimensions, they specify which image of the

View File

@ -26,6 +26,7 @@ args = list of arguments for a particular style :l
q, mux, muy, muz, mu,
radius, diameter, omegax, omegay, omegaz,
angmomx, angmomy, angmomz, tqx, tqy, tqz,
spin, eradius, ervel, erforce,
c_ID, c_ID\[N\], f_ID, f_ID\[N\], v_name :pre
id = atom ID
@ -50,18 +51,17 @@ args = list of arguments for a particular style :l
angmomx,angmomy,angmomz = angular momentum of aspherical particle
tqx,tqy,tqz = torque on finite-size particles
c_ID = per-atom vector calculated by a compute with ID
c_ID\[I\] = Ith column of per-atom array calculated by a compute with ID, I can include wildcard (see below)
c_ID\[N\] = Nth column of per-atom array calculated by a compute with ID
f_ID = per-atom vector calculated by a fix with ID
f_ID\[I\] = Ith column of per-atom array calculated by a fix with ID, I can include wildcard (see below)
v_name = per-atom vector calculated by an atom-style variable with name
d_name = per-atom floating point vector with name, managed by fix property/atom
i_name = per-atom integer vector with name, managed by fix property/atom :pre
f_ID\[N\] = Nth column of per-atom array calculated by a fix with ID
v_name = per-atom vector calculated by an atom-style variable with name :pre
:ule
[Examples:]
dump dmpvtk all custom/vtk 100 dump*.myforce.vtk id type vx fx
dump dmpvtp flow custom/vtk 100 dump*.%.displace.vtp id type c_myD\[1\] c_myD\[2\] c_myD\[3\] v_ke :pre
dump dmpvtp flow custom/vtk 100 dump*.%.displace.vtp id type c_myD\[1\] c_myD\[2\] c_myD\[3\] v_ke
dump e_data all custom/vtk 100 dump*.vtu id type spin eradius fx fy fz eforce :pre
The style {custom/vtk} is similar to the "custom"_dump.html style but
uses the VTK library to write data to VTK simple legacy or XML format
@ -199,38 +199,32 @@ part of the {custom/vtk} style.
The {id}, {mol}, {proc}, {procp1}, {type}, {element}, {mass}, {vx},
{vy}, {vz}, {fx}, {fy}, {fz}, {q} attributes are self-explanatory.
{Id} is the atom ID. {Mol} is the molecule ID, included in the data
file for molecular systems. {Proc} is the ID of the processor (0 to
Nprocs-1) that currently owns the atom. {Procp1} is the proc ID+1,
which can be convenient in place of a {type} attribute (1 to Ntypes)
for coloring atoms in a visualization program. {Type} is the atom
type (1 to Ntypes). {Element} is typically the chemical name of an
element, which you must assign to each type via the "dump_modify
element"_dump_modify.html command. More generally, it can be any
string you wish to associated with an atom type. {Mass} is the atom
mass. {Vx}, {vy}, {vz}, {fx}, {fy}, {fz}, and {q} are components of
atom velocity and force and atomic charge.
{id} is the atom ID. {mol} is the molecule ID, included in the data
file for molecular systems. {type} is the atom type. {element} is
typically the chemical name of an element, which you must assign to
each type via the "dump_modify element"_dump_modify.html command.
More generally, it can be any string you wish to associate with an
atom type. {mass} is the atom mass. {vx}, {vy}, {vz}, {fx}, {fy},
{fz}, and {q} are components of atom velocity and force and atomic
charge.
There are several options for outputting atom coordinates. The {x},
{y}, {z} attributes write atom coordinates "unscaled", in the
appropriate distance "units"_units.html (Angstroms, sigma, etc). Use
{xs}, {ys}, {zs} if you want the coordinates "scaled" to the box size,
so that each value is 0.0 to 1.0. If the simulation box is triclinic
(tilted), then all atom coords will still be between 0.0 and 1.0.
I.e. actual unscaled (x,y,z) = xs*A + ys*B + zs*C, where (A,B,C) are
the non-orthogonal vectors of the simulation box edges, as discussed
in "Section 6.12"_Section_howto.html#howto_12.
Use {xu}, {yu}, {zu} if you want the coordinates "unwrapped" by the
image flags for each atom. Unwrapped means that if the atom has
passed thru a periodic boundary one or more times, the value is
printed for what the coordinate would be if it had not been wrapped
back into the periodic box. Note that using {xu}, {yu}, {zu} means
that the coordinate values may be far outside the box bounds printed
with the snapshot. Using {xsu}, {ysu}, {zsu} is similar to using
{xu}, {yu}, {zu}, except that the unwrapped coordinates are scaled by
the box size. Atoms that have passed through a periodic boundary will
have the corresponding coordinate increased or decreased by 1.0.
{y}, {z} attributes are used to write atom coordinates "unscaled", in
the appropriate distance "units"_units.html (Angstroms, sigma, etc).
Additionaly, you can use {xs}, {ys}, {zs} if you want to also save the
coordinates "scaled" to the box size, so that each value is 0.0 to
1.0. If the simulation box is triclinic (tilted), then all atom
coords will still be between 0.0 and 1.0. Use {xu}, {yu}, {zu} if you
want the coordinates "unwrapped" by the image flags for each atom.
Unwrapped means that if the atom has passed through a periodic
boundary one or more times, the value is printed for what the
coordinate would be if it had not been wrapped back into the periodic
box. Note that using {xu}, {yu}, {zu} means that the coordinate
values may be far outside the box bounds printed with the snapshot.
Using {xsu}, {ysu}, {zsu} is similar to using {xu}, {yu}, {zu}, except
that the unwrapped coordinates are scaled by the box size. Atoms that
have passed through a periodic boundary will have the corresponding
cooordinate increased or decreased by 1.0.
The image flags can be printed directly using the {ix}, {iy}, {iz}
attributes. For periodic dimensions, they specify which image of the
@ -261,7 +255,13 @@ The {tqx}, {tqy}, {tqz} attributes are for finite-size particles that
can sustain a rotational torque due to interactions with other
particles.
The {c_ID} and {c_ID\[I\]} attributes allow per-atom vectors or arrays
The {spin}, {eradius}, {ervel}, and {erforce} attributes are for
particles that represent nuclei and electrons modeled with the
electronic force field (EFF). See "atom_style
electron"_atom_style.html and "pair_style eff"_pair_eff.html for more
details.
The {c_ID} and {c_ID\[N\]} attributes allow per-atom vectors or arrays
calculated by a "compute"_compute.html to be output. The ID in the
attribute should be replaced by the actual ID of the compute that has
been defined previously in the input script. See the
@ -275,14 +275,12 @@ command. Instead, global quantities can be output by the
"thermo_style custom"_thermo_style.html command, and local quantities
can be output by the dump local command.
If {c_ID} is used as a attribute, then the per-atom vector calculated
by the compute is printed. If {c_ID\[I\]} is used, then I must be in
the range from 1-M, which will print the Ith column of the per-atom
array with M columns calculated by the compute. See the discussion
above for how I can be specified with a wildcard asterisk to
effectively specify multiple values.
If {c_ID} is used as an attribute, then the per-atom vector calculated
by the compute is printed. If {c_ID\[N\]} is used, then N must be in
the range from 1-M, which will print the Nth column of the M-length
per-atom array calculated by the compute.
The {f_ID} and {f_ID\[I\]} attributes allow vector or array per-atom
The {f_ID} and {f_ID\[N\]} attributes allow vector or array per-atom
quantities calculated by a "fix"_fix.html to be output. The ID in the
attribute should be replaced by the actual ID of the fix that has been
defined previously in the input script. The "fix
@ -293,11 +291,9 @@ any "compute"_compute.html, "fix"_fix.html, or atom-style
be written to a dump file.
If {f_ID} is used as a attribute, then the per-atom vector calculated
by the fix is printed. If {f_ID\[I\]} is used, then I must be in the
range from 1-M, which will print the Ith column of the per-atom array
with M columns calculated by the fix. See the discussion above for
how I can be specified with a wildcard asterisk to effectively specify
multiple values.
by the fix is printed. If {f_ID\[N\]} is used, then N must be in the
range from 1-M, which will print the Nth column of the M-length
per-atom array calculated by the fix.
The {v_name} attribute allows per-atom vectors calculated by a
"variable"_variable.html to be output. The name in the attribute
@ -310,10 +306,6 @@ invoke other computes, fixes, or variables when they are evaluated, so
this is a very general means of creating quantities to output to a
dump file.
The {d_name} and {i_name} attributes allow to output custom per atom
floating point or integer properties that are managed by
"fix property/atom"_fix_property_atom.html.
See "Section 10"_Section_modify.html of the manual for information
on how to add new compute and fix styles to LAMMPS to calculate
per-atom quantities which could then be output into dump files.

View File

@ -99,7 +99,7 @@ included in the image or movie and how it appears. A series of such
images can easily be manually converted into an animated movie of your
simulation or the process can be automated without writing the
intermediate files using the dump movie style; see further details
below. Other dump styles store snapshots of numerical data associated
below. Other dump styles store snapshots of numerical data asociated
with atoms in various formats, as discussed on the "dump"_dump.html
doc page.
@ -237,7 +237,7 @@ diameter, which can be used as the {diameter} setting.
:line
The various keywords listed above control how the image is rendered.
The various kewords listed above control how the image is rendered.
As listed below, all of the keywords have defaults, most of which you
will likely not need to change. The "dump modify"_dump_modify.html
also has options specific to the dump image style, particularly for
@ -261,7 +261,7 @@ the input script defines, e.g. Angstroms.
The {bond} keyword allows to you to alter how bonds are drawn. A bond
is only drawn if both atoms in the bond are being drawn due to being
in the specified group and due to other selection criteria
(e.g. region, threshold settings of the
(e.g. region, threshhold settings of the
"dump_modify"_dump_modify.html command). By default, bonds are drawn
if they are defined in the input data file as read by the
"read_data"_read_data.html command. Using {none} for both the bond
@ -356,7 +356,7 @@ is used to define body particles with internal state
body style. If this keyword is not used, such particles will be drawn
as spheres, the same as if they were regular atoms.
The "body"_body.html doc page describes the body styles LAMMPS
The "body"_body.html doc page descibes the body styles LAMMPS
currently supports, and provides more details as to the kind of body
particles they represent and how they are drawn by this dump image
command. For all the body styles, individual atoms can be either a
@ -442,7 +442,7 @@ degrees.
The {center} keyword determines the point in simulation space that
will be at the center of the image. {Cx}, {Cy}, and {Cz} are
specified as fractions of the box dimensions, so that (0.5,0.5,0.5) is
speficied as fractions of the box dimensions, so that (0.5,0.5,0.5) is
the center of the simulation box. These values do not have to be
between 0.0 and 1.0, if you want the simulation box to be offset from
the center of the image. Note, however, that if you choose strange
@ -476,8 +476,8 @@ smaller. {Zfactor} must be a value > 0.0.
The {persp} keyword determines how much depth perspective is present
in the image. Depth perspective makes lines that are parallel in
simulation space appear non-parallel in the image. A {pfactor} value
of 0.0 means that parallel lines will meet at infinity (1.0/pfactor),
which is an orthographic rendering with no perspective. A {pfactor}
of 0.0 means that parallel lines will meet at infininty (1.0/pfactor),
which is an orthographic rendering with no persepctive. A {pfactor}
value between 0.0 and 1.0 will introduce more perspective. A {pfactor}
value > 1 will create a highly skewed image with a large amount of
perspective.
@ -638,7 +638,7 @@ pipe:: Input/output error :pre
which can be safely ignored. Other warnings
and errors have to be addressed according to the FFmpeg documentation.
One known issue is that certain movie file formats (e.g. MPEG level 1
and 2 format streams) have video bandwidth limits that can be crossed
and 2 format streams) have video bandwith limits that can be crossed
when rendering too large of image sizes. Typical warnings look like
this:

View File

@ -426,7 +426,7 @@ regions.
The {scale} keyword applies only to the dump {atom} style. A scale
value of {yes} means atom coords are written in normalized units from
0.0 to 1.0 in each box dimension. If the simulation box is triclinic
0.0 to 1.0 in each box dimension. If the simluation box is triclinic
(tilted), then all atom coords will still be between 0.0 and 1.0. A
value of {no} means they are written in absolute distance units
(e.g. Angstroms or sigma).
@ -470,7 +470,7 @@ stress of atoms whose energy is above some threshold.
If an atom-style variable is used as the attribute, then it can
produce continuous numeric values or effective Boolean 0/1 values
which may be useful for the comparison operator. Boolean values can
which may be useful for the comparision operator. Boolean values can
be generated by variable formulas that use comparison or Boolean math
operators or special functions like gmask() and rmask() and grmask().
See the "variable"_variable.html command doc page for details.

View File

@ -34,7 +34,10 @@ to one or more files every N timesteps in one of several formats.
Only information for atoms in the specified group is dumped. This
specific dump style uses molfile plugins that are bundled with the
"VMD"_http://www.ks.uiuc.edu/Research/vmd molecular visualization and
analysis program.
analysis program. See "Section 9"_Section_tools.html#vmd of the
manual and the tools/lmp2vmd/README.txt file for more information
about support in VMD for reading and visualizing native LAMMPS dump
files.
Unless the filename contains a * character, the output will be written
to one single file with the specified format. Otherwise there will be

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