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git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@14550 f3b2605a-c512-4ea7-a41b-209d697bcdaa
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LAMMPS Documentation
====================

29 Jan 2016 version
-------------------
3 Feb 2016 version
------------------

Version info:
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@@ -101,6 +101,27 @@ assignments for the Nth replica by comparing the Nth column of screen
output to the thermodynamic data in the corresponding log.lammps.N or
screen.N files as time proceeds.

You can have each replica create its own dump file in the following
manner:

.. parsed-literal::

   variable rep world 0 1 2 3 4 5 6 7
   dump 1 all atom 1000 dump.temper.$*rep*

.. note::

   Each replica's dump file will contain a continuous trajectory
   for its atoms where the temperature varies over time as swaps take
   place involving that replica.  If you want a series of dump files,
   each with snapshots (from all replicas) that are all at a single
   temperature, then you will need to post-process the dump files using
   the information from the log.lammps file.  E.g. you could produce one
   dump file with snapshots at 300K (from all replicas), another with
   snapshots at 310K, etc.  Note that these new dump files will not
   contain "continuous trajectories" for individual atoms, because two
   successive snapshots (in time) may be from different replicas.

The last argument *index* in the temper command is optional and is
used when restarting a tempering run from a set of restart files (one
for each replica) which had previously swapped to new temperatures.
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         ke = kinetic energy
         etotal = total energy (pe + ke)
         enthalpy = enthalpy (etotal + press*vol)
         evdwl = VanderWaal pairwise energy
         evdwl = VanderWaal pairwise energy (includes etail)
         ecoul = Coulombic pairwise energy
         epair = pairwise energy (evdwl + ecoul + elong + etail)
         epair = pairwise energy (evdwl + ecoul + elong)
         ebond = bond energy
         eangle = angle energy
         edihed = dihedral energy
@@ -215,9 +215,9 @@ to see which ones contribute.

A long-range tail correction *etail* for the VanderWaal pairwise
energy will be non-zero only if the :doc:`pair_modify tail <pair_modify>` option is turned on.  The *etail* contribution
is included in *evdwl*, *pe*, and *etotal*, and the corresponding tail
correction to the pressure is included in *press* and *pxx*, *pyy*,
etc.
is included in *evdwl*, *epair*, *pe*, and *etotal*, and the
corresponding tail correction to the pressure is included in *press*
and *pxx*, *pyy*, etc.


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@@ -212,6 +212,25 @@ temperature. You can verify this time sequence of temperature
assignments for the Nth replica by comparing the Nth column of screen
output to the thermodynamic data in the corresponding log.lammps.N or
screen.N files as time proceeds.</p>
<p>You can have each replica create its own dump file in the following
manner:</p>
<div class="highlight-python"><div class="highlight"><pre>variable rep world 0 1 2 3 4 5 6 7
dump 1 all atom 1000 dump.temper.$*rep*
</pre></div>
</div>
<div class="admonition note">
<p class="first admonition-title">Note</p>
<p class="last">Each replica&#8217;s dump file will contain a continuous trajectory
for its atoms where the temperature varies over time as swaps take
place involving that replica.  If you want a series of dump files,
each with snapshots (from all replicas) that are all at a single
temperature, then you will need to post-process the dump files using
the information from the log.lammps file.  E.g. you could produce one
dump file with snapshots at 300K (from all replicas), another with
snapshots at 310K, etc.  Note that these new dump files will not
contain &#8220;continuous trajectories&#8221; for individual atoms, because two
successive snapshots (in time) may be from different replicas.</p>
</div>
<p>The last argument <em>index</em> in the temper command is optional and is
used when restarting a tempering run from a set of restart files (one
for each replica) which had previously swapped to new temperatures.
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