Merge remote-tracking branch 'lammps-ro/master' into lammps-icms

# Resolved Conflicts:
#	doc/Manual.txt
#	doc/improper_distance.txt
#	doc/pair_mdf.txt
#	python/lammps.py
#	src/MANYBODY/pair_polymorphic.cpp
#	src/MANYBODY/pair_polymorphic.h
This commit is contained in:
Axel Kohlmeyer
2015-12-10 06:29:32 -05:00
1118 changed files with 13893 additions and 120024 deletions

Binary file not shown.

After

Width:  |  Height:  |  Size: 2.9 KiB

View File

@ -3,8 +3,8 @@
\begin{document}
\begin{eqnarray*}
F_{i1}^{SRP} & = & F^{SRP}_{ij}(L) \\
F_{i2}^{SRP} & = & F^{SRP}_{ij}(1-L)
-\vec{T_j} & = & \vec{r_{ij}} \times \vec{F_i}\\
\vec{F_j} & = & -\vec{F_i} \\
\end{eqnarray*}
\end{document}

View File

@ -135,7 +135,7 @@
<H1></H1><div class="section" id="lammps-documentation">
<h1>LAMMPS-ICMS Documentation<a class="headerlink" href="#lammps-documentation" title="Permalink to this headline"></a></h1>
<div class="section" id="dec-2015-version">
<h2>7 Dec 2015 version<a class="headerlink" href="#dec-2015-version" title="Permalink to this headline"></a></h2>
<h2>10 Dec 2015 version<a class="headerlink" href="#dec-2015-version" title="Permalink to this headline"></a></h2>
</div>
<div class="section" id="version-info">
<h2>Version info:<a class="headerlink" href="#version-info" title="Permalink to this headline"></a></h2>

View File

@ -1,7 +1,7 @@
<!-- HTML_ONLY -->
<HEAD>
<TITLE>LAMMPS-ICMS Users Manual</TITLE>
<META NAME="docnumber" CONTENT="7 Dec 2015 version">
<META NAME="docnumber" CONTENT="10 Dec 2015 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-ICMS Documentation :c,h3
7 Dec 2015 version :c,h4
10 Dec 2015 version :c,h4
Version info: :h4

View File

@ -710,7 +710,7 @@ g = GPU, i = USER-INTEL, k = KOKKOS, o = USER-OMP, t = OPT.</p>
<tr class="row-odd"><td><a class="reference internal" href="fix_rigid.html"><em>rigid/small/npt</em></a></td>
<td><a class="reference internal" href="fix_rigid.html"><em>rigid/small/nve</em></a></td>
<td><a class="reference internal" href="fix_rigid.html"><em>rigid/small/nvt</em></a></td>
<td><a class="reference internal" href="fix_setforce.html"><em>setforce (c)</em></a></td>
<td><a class="reference internal" href="fix_setforce.html"><em>setforce (ck)</em></a></td>
<td><a class="reference internal" href="fix_shake.html"><em>shake (c)</em></a></td>
<td><a class="reference internal" href="fix_spring.html"><em>spring</em></a></td>
<td><a class="reference internal" href="fix_spring_rg.html"><em>spring/rg</em></a></td>
@ -1157,61 +1157,66 @@ KOKKOS, o = USER-OMP, t = OPT.</p>
if <a class="reference internal" href="Section_start.html#start-3"><span>LAMMPS is built with the appropriate package</span></a>.</p>
<table border="1" class="docutils">
<colgroup>
<col width="21%" />
<col width="25%" />
<col width="31%" />
<col width="23%" />
<col width="21%" />
<col width="24%" />
</colgroup>
<tbody valign="top">
<tr class="row-odd"><td><a class="reference internal" href="pair_awpmd.html"><em>awpmd/cut</em></a></td>
<td><a class="reference internal" href="pair_mdf.html"><em>buck/mdf</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>coul/cut/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_coul_diel.html"><em>coul/diel (o)</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>coul/long/soft (o)</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_eam.html"><em>eam/cd (o)</em></a></td>
<tr class="row-even"><td><a class="reference internal" href="pair_lj_soft.html"><em>coul/long/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_eam.html"><em>eam/cd (o)</em></a></td>
<td><a class="reference internal" href="pair_edip.html"><em>edip (o)</em></a></td>
<td><a class="reference internal" href="pair_eff.html"><em>eff/cut</em></a></td>
<td><a class="reference internal" href="pair_gauss.html"><em>gauss/cut</em></a></td>
</tr>
<tr class="row-odd"><td><a class="reference internal" href="pair_list.html"><em>list</em></a></td>
<tr class="row-odd"><td><a class="reference internal" href="pair_gauss.html"><em>gauss/cut</em></a></td>
<td><a class="reference internal" href="pair_mdf.html"><em>lennard/mdf</em></a></td>
<td><a class="reference internal" href="pair_list.html"><em>list</em></a></td>
<td><a class="reference internal" href="pair_charmm.html"><em>lj/charmm/coul/long/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>lj/cut/coul/cut/soft (o)</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_lj_soft.html"><em>lj/cut/coul/cut/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>lj/cut/coul/long/soft (o)</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_dipole.html"><em>lj/cut/dipole/sf (go)</em></a></td>
<td><a class="reference internal" href="pair_dipole.html"><em>lj/cut/dipole/sf (go)</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>lj/cut/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>lj/cut/tip4p/long/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_sdk.html"><em>lj/sdk (gko)</em></a></td>
</tr>
<tr class="row-odd"><td><a class="reference internal" href="pair_sdk.html"><em>lj/sdk/coul/long (go)</em></a></td>
<td><a class="reference internal" href="pair_sdk.html"><em>lj/sdk/coul/msm (o)</em></a></td>
<tr class="row-odd"><td><a class="reference internal" href="pair_lj_soft.html"><em>lj/cut/tip4p/long/soft (o)</em></a></td>
<td><a class="reference internal" href="pair_mdf.html"><em>lj/mdf</em></a></td>
<td><a class="reference internal" href="pair_sdk.html"><em>lj/sdk (gko)</em></a></td>
<td><a class="reference internal" href="pair_sdk.html"><em>lj/sdk/coul/long (go)</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_sdk.html"><em>lj/sdk/coul/msm (o)</em></a></td>
<td><a class="reference internal" href="pair_lj_sf.html"><em>lj/sf (o)</em></a></td>
<td><a class="reference internal" href="pair_meam_spline.html"><em>meam/spline</em></a></td>
<td><a class="reference internal" href="pair_meam_sw_spline.html"><em>meam/sw/spline</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_meam_sw_spline.html"><em>meam/sw/spline</em></a></td>
<td><a class="reference internal" href="pair_mgpt.html"><em>mgpt</em></a></td>
<tr class="row-odd"><td><a class="reference internal" href="pair_mgpt.html"><em>mgpt</em></a></td>
<td><a class="reference internal" href="pair_quip.html"><em>quip</em></a></td>
<td><a class="reference internal" href="pair_reax_c.html"><em>reax/c</em></a></td>
<td><a class="reference internal" href="pair_smd_hertz.html"><em>smd/hertz</em></a></td>
</tr>
<tr class="row-odd"><td><a class="reference internal" href="pair_smd_hertz.html"><em>smd/hertz</em></a></td>
<td><a class="reference internal" href="pair_smd_tlsph.html"><em>smd/tlsph</em></a></td>
<tr class="row-even"><td><a class="reference internal" href="pair_smd_tlsph.html"><em>smd/tlsph</em></a></td>
<td><a class="reference internal" href="pair_smd_triangulated_surface.html"><em>smd/triangulated/surface</em></a></td>
<td><a class="reference internal" href="pair_smd_ulsph.html"><em>smd/ulsph</em></a></td>
<td><a class="reference internal" href="pair_smtbq.html"><em>smtbq</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_smtbq.html"><em>smtbq</em></a></td>
<td><a class="reference internal" href="pair_sph_heatconduction.html"><em>sph/heatconduction</em></a></td>
<tr class="row-odd"><td><a class="reference internal" href="pair_sph_heatconduction.html"><em>sph/heatconduction</em></a></td>
<td><a class="reference internal" href="pair_sph_idealgas.html"><em>sph/idealgas</em></a></td>
<td><a class="reference internal" href="pair_sph_lj.html"><em>sph/lj</em></a></td>
<td><a class="reference internal" href="pair_sph_rhosum.html"><em>sph/rhosum</em></a></td>
</tr>
<tr class="row-odd"><td><a class="reference internal" href="pair_sph_rhosum.html"><em>sph/rhosum</em></a></td>
<td><a class="reference internal" href="pair_sph_taitwater.html"><em>sph/taitwater</em></a></td>
<tr class="row-even"><td><a class="reference internal" href="pair_sph_taitwater.html"><em>sph/taitwater</em></a></td>
<td><a class="reference internal" href="pair_sph_taitwater_morris.html"><em>sph/taitwater/morris</em></a></td>
<td><a class="reference internal" href="pair_srp.html"><em>srp</em></a></td>
<td><a class="reference internal" href="pair_tersoff.html"><em>tersoff/table (o)</em></a></td>
</tr>
<tr class="row-even"><td><a class="reference internal" href="pair_tersoff.html"><em>tersoff/table (o)</em></a></td>
<td><a class="reference internal" href="pair_thole.html"><em>thole</em></a></td>
<tr class="row-odd"><td><a class="reference internal" href="pair_thole.html"><em>thole</em></a></td>
<td><a class="reference internal" href="pair_lj_soft.html"><em>tip4p/long/soft (o)</em></a></td>
<td>&nbsp;</td>
<td>&nbsp;</td>
</tr>
</tbody>
</table>
@ -1406,12 +1411,14 @@ KOKKOS, o = USER-OMP, t = OPT.</p>
used if <a class="reference internal" href="Section_start.html#start-3"><span>LAMMPS is built with the appropriate package</span></a>.</p>
<table border="1" class="docutils">
<colgroup>
<col width="33%" />
<col width="36%" />
<col width="31%" />
<col width="24%" />
<col width="26%" />
<col width="27%" />
<col width="23%" />
</colgroup>
<tbody valign="top">
<tr class="row-odd"><td><a class="reference internal" href="improper_cossq.html"><em>cossq (o)</em></a></td>
<td><a class="reference internal" href="improper_distance.html"><em>distance</em></a></td>
<td><a class="reference internal" href="improper_fourier.html"><em>fourier (o)</em></a></td>
<td><a class="reference internal" href="improper_ring.html"><em>ring (o)</em></a></td>
</tr>

View File

@ -563,7 +563,7 @@ g = GPU, i = USER-INTEL, k = KOKKOS, o = USER-OMP, t = OPT.
"rigid/small/npt"_fix_rigid.html,
"rigid/small/nve"_fix_rigid.html,
"rigid/small/nvt"_fix_rigid.html,
"setforce (c)"_fix_setforce.html,
"setforce (ck)"_fix_setforce.html,
"shake (c)"_fix_shake.html,
"spring"_fix_spring.html,
"spring/rg"_fix_spring_rg.html,
@ -898,6 +898,7 @@ if "LAMMPS is built with the appropriate
package"_Section_start.html#start_3.
"awpmd/cut"_pair_awpmd.html,
"buck/mdf"_pair_mdf.html,
"coul/cut/soft (o)"_pair_lj_soft.html,
"coul/diel (o)"_pair_coul_diel.html,
"coul/long/soft (o)"_pair_lj_soft.html,
@ -905,6 +906,7 @@ package"_Section_start.html#start_3.
"edip (o)"_pair_edip.html,
"eff/cut"_pair_eff.html,
"gauss/cut"_pair_gauss.html,
"lennard/mdf"_pair_mdf.html,
"list"_pair_list.html,
"lj/charmm/coul/long/soft (o)"_pair_charmm.html,
"lj/cut/coul/cut/soft (o)"_pair_lj_soft.html,
@ -912,6 +914,7 @@ package"_Section_start.html#start_3.
"lj/cut/dipole/sf (go)"_pair_dipole.html,
"lj/cut/soft (o)"_pair_lj_soft.html,
"lj/cut/tip4p/long/soft (o)"_pair_lj_soft.html,
"lj/mdf"_pair_mdf.html,
"lj/sdk (gko)"_pair_sdk.html,
"lj/sdk/coul/long (go)"_pair_sdk.html,
"lj/sdk/coul/msm (o)"_pair_sdk.html,
@ -1057,6 +1060,7 @@ used if "LAMMPS is built with the appropriate
package"_Section_start.html#start_3.
"cossq (o)"_improper_cossq.html,
"distance"_improper_distance.html,
"fourier (o)"_improper_fourier.html,
"ring (o)"_improper_ring.html :tb(c=4,ea=c)

View File

@ -411,9 +411,16 @@ downloaded and looked at a few of them, their documentation was
incomplete and I had trouble with their installation. It&#8217;s not clear
if some of the packages are still being actively developed and
supported.</p>
<p>The one I recommend, since I have successfully used it with LAMMPS, is
Pypar. Pypar requires the ubiquitous <a class="reference external" href="http://numpy.scipy.org">Numpy package</a> be installed in your Python. After
launching python, type</p>
<p>The packages Pypar and mpi4py have both been successfully tested with
LAMMPS. Pypar is simpler and easy to set up and use, but supports
only a subset of MPI. Mpi4py is more MPI-feature complete, but also a
bit more complex to use. As of version 2.0.0, mpi4py is the only
python MPI wrapper that allows passing a custom MPI communicator to
the LAMMPS constructor, which means one can easily run one or more
LAMMPS instances on subsets of the total MPI ranks.</p>
<hr class="docutils" />
<p>Pypar requires the ubiquitous <a class="reference external" href="http://numpy.scipy.org">Numpy package</a>
be installed in your Python. After launching Python, type</p>
<div class="highlight-python"><div class="highlight"><pre><span class="kn">import</span> <span class="nn">numpy</span>
</pre></div>
</div>
@ -466,6 +473,51 @@ address, e.g. by moving other MPI installations so that Pypar finds
the right one.</p>
</div>
<hr class="docutils" />
<p>To install mpi4py (version mpi4py-2.0.0 as of Oct 2015), unpack it
and from its main directory, type</p>
<div class="highlight-python"><div class="highlight"><pre>python setup.py build
sudo python setup.py install
</pre></div>
</div>
<p>Again, the &#8220;sudo&#8221; is only needed if required to copy mpi4py files into
your Python distribution&#8217;s site-packages directory. To install with
user privilege into the user local directory type</p>
<div class="highlight-python"><div class="highlight"><pre>python setup.py install --user
</pre></div>
</div>
<p>If you have successully installed mpi4py, you should be able to run
Python and type</p>
<div class="highlight-python"><div class="highlight"><pre><span class="kn">from</span> <span class="nn">mpi4py</span> <span class="kn">import</span> <span class="n">MPI</span>
</pre></div>
</div>
<p>without error. You should also be able to run python in parallel
on a simple test script</p>
<div class="highlight-python"><div class="highlight"><pre>% mpirun -np 4 python test.py
</pre></div>
</div>
<p>where test.py contains the lines</p>
<div class="highlight-python"><div class="highlight"><pre>from mpi4py import MPI
comm = MPI.COMM_WORLD
print &quot;Proc %d out of %d procs&quot; % (comm.Get_rank(),comm.Get_size())
</pre></div>
</div>
<p>and see one line of output for each processor you run on.</p>
<div class="admonition warning">
<p class="first admonition-title">Warning</p>
<p class="last">To use mpi4py and LAMMPS in parallel from Python, you
must insure both are using the same version of MPI. If you only have
one MPI installed on your system, this is not an issue, but it can be
if you have multiple MPIs. Your LAMMPS build is explicit about which
MPI it is using, since you specify the details in your lo-level
src/MAKE/Makefile.foo file. Mpi4py uses the &#8220;mpicc&#8221; command to find
information about the MPI it uses to build against. And it tries to
load &#8220;libmpi.so&#8221; from the LD_LIBRARY_PATH. This may or may not find
the MPI library that LAMMPS is using. If you have problems running
both mpi4py and LAMMPS together, this is an issue you may need to
address, e.g. by moving other MPI installations so that mpi4py finds
the right one.</p>
</div>
<hr class="docutils" />
</div>
<div class="section" id="testing-the-python-lammps-interface">
<span id="py-6"></span><h2>11.6. Testing the Python-LAMMPS interface<a class="headerlink" href="#testing-the-python-lammps-interface" title="Permalink to this headline"></a></h2>
@ -517,8 +569,8 @@ typed something like:</p>
<div class="section" id="test-lammps-and-python-in-parallel">
<h3>11.6.2. <strong>Test LAMMPS and Python in parallel:</strong><a class="headerlink" href="#test-lammps-and-python-in-parallel" title="Permalink to this headline"></a></h3>
<p>To run LAMMPS in parallel, assuming you have installed the
<a class="reference external" href="http://datamining.anu.edu.au/~ole/pypar">Pypar</a> package as discussed
above, create a test.py file containing these lines:</p>
<a class="reference external" href="Pypar">Pypar</a> package as discussed above, create a test.py file
containing these lines:</p>
<div class="highlight-python"><div class="highlight"><pre>import pypar
from lammps import lammps
lmp = lammps()
@ -527,7 +579,20 @@ print &quot;Proc %d out of %d procs has&quot; % (pypar.rank(),pypar.size()),lmp
pypar.finalize()
</pre></div>
</div>
<p>You can then run it in parallel as:</p>
<p>To run LAMMPS in parallel, assuming you have installed the
<a class="reference external" href="mpi4py">mpi4py</a> package as discussed above, create a test.py file
containing these lines:</p>
<div class="highlight-python"><div class="highlight"><pre>from mpi4py import MPI
from lammps import lammps
lmp = lammps()
lmp.file(&quot;in.lj&quot;)
me = MPI.COMM_WORLD.Get_rank()
nprocs = MPI.COMM_WORLD.Get_size()
print &quot;Proc %d out of %d procs has&quot; % (me,nprocs),lmp
MPI.Finalize()
</pre></div>
</div>
<p>You can either script in parallel as:</p>
<div class="highlight-python"><div class="highlight"><pre>% mpirun -np 4 python test.py
</pre></div>
</div>
@ -590,11 +655,12 @@ Python script, as follows:</p>
the files src/library.cpp and src/library.h you will see that they
correspond one-to-one with calls you can make to the LAMMPS library
from a C++ or C or Fortran program.</p>
<div class="highlight-python"><div class="highlight"><pre><span class="n">lmp</span> <span class="o">=</span> <span class="n">lammps</span><span class="p">()</span> <span class="c"># create a LAMMPS object using the default liblammps.so library</span>
<span class="n">lmp</span> <span class="o">=</span> <span class="n">lammps</span><span class="p">(</span><span class="n">ptr</span><span class="o">=</span><span class="n">lmpptr</span><span class="p">)</span> <span class="c"># ditto, but use lmpptr as previously created LAMMPS object</span>
<span class="n">lmp</span> <span class="o">=</span> <span class="n">lammps</span><span class="p">(</span><span class="s">&quot;g++&quot;</span><span class="p">)</span> <span class="c"># create a LAMMPS object using the liblammps_g++.so library</span>
<span class="n">lmp</span> <span class="o">=</span> <span class="n">lammps</span><span class="p">(</span><span class="s">&quot;&quot;</span><span class="p">,</span><span class="nb">list</span><span class="p">)</span> <span class="c"># ditto, with command-line args, e.g. list = [&quot;-echo&quot;,&quot;screen&quot;]</span>
<span class="n">lmp</span> <span class="o">=</span> <span class="n">lammps</span><span class="p">(</span><span class="s">&quot;g++&quot;</span><span class="p">,</span><span class="nb">list</span><span class="p">)</span>
<div class="highlight-python"><div class="highlight"><pre>lmp = lammps() # create a LAMMPS object using the default liblammps.so library
4 optional args are allowed: name, cmdargs, ptr, comm
lmp = lammps(ptr=lmpptr) # use lmpptr as previously created LAMMPS object
lmp = lammps(comm=split) # create a LAMMPS object with a custom communicator, requires mpi4py 2.0.0 or later
lmp = lammps(name=&quot;g++&quot;) # create a LAMMPS object using the liblammps_g++.so library
lmp = lammps(name=&quot;g++&quot;,cmdargs=list) # add LAMMPS command-line args, e.g. list = [&quot;-echo&quot;,&quot;screen&quot;]
</pre></div>
</div>
<div class="highlight-python"><div class="highlight"><pre><span class="n">lmp</span><span class="o">.</span><span class="n">close</span><span class="p">()</span> <span class="c"># destroy a LAMMPS object</span>
@ -706,8 +772,8 @@ argument.</p>
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. A pointer to a vector of
doubles or integers, or a pointer to an array of doubles (double <a href="#id2"><span class="problematic" id="id3">**</span></a>)
or integers (int <a href="#id4"><span class="problematic" id="id5">**</span></a>) is returned. You need to specify the appropriate
doubles or integers, or a pointer to an array of doubles (double <a href="#id3"><span class="problematic" id="id4">**</span></a>)
or integers (int <a href="#id5"><span class="problematic" id="id6">**</span></a>) is returned. You need to specify the appropriate
data type via the type argument.</p>
<p>For extract_compute() and extract_fix(), the global, per-atom, or
local data calulated by the compute or fix can be accessed. What is
@ -802,8 +868,8 @@ own scripts, send them to us and we can include them in the LAMMPS
distribution.</p>
<table border="1" class="docutils">
<colgroup>
<col width="27%" />
<col width="73%" />
<col width="56%" />
<col width="44%" />
</colgroup>
<tbody valign="top">
<tr class="row-odd"><td>trivial.py</td>
@ -813,19 +879,25 @@ distribution.</p>
<td>invoke various LAMMPS library interface routines</td>
</tr>
<tr class="row-odd"><td>simple.py</td>
<td>mimic operation of couple/simple/simple.cpp in Python</td>
<td>run in parallel</td>
</tr>
<tr class="row-even"><td>gui.py</td>
<td>GUI go/stop/temperature-slider to control LAMMPS</td>
<tr class="row-even"><td>similar to examples/COUPLE/simple/simple.cpp</td>
<td>split.py</td>
</tr>
<tr class="row-odd"><td>plot.py</td>
<td>real-time temeperature plot with GnuPlot via Pizza.py</td>
<tr class="row-odd"><td>same as simple.py but running in parallel on a subset of procs</td>
<td>gui.py</td>
</tr>
<tr class="row-even"><td>viz_tool.py</td>
<td>real-time viz via some viz package</td>
<tr class="row-even"><td>GUI go/stop/temperature-slider to control LAMMPS</td>
<td>plot.py</td>
</tr>
<tr class="row-odd"><td>vizplotgui_tool.py</td>
<td>combination of viz_tool.py and plot.py and gui.py</td>
<tr class="row-odd"><td>real-time temeperature plot with GnuPlot via Pizza.py</td>
<td>viz_tool.py</td>
</tr>
<tr class="row-even"><td>real-time viz via some viz package</td>
<td>vizplotgui_tool.py</td>
</tr>
<tr class="row-odd"><td>combination of viz_tool.py and plot.py and gui.py</td>
<td>&nbsp;</td>
</tr>
</tbody>
</table>

View File

@ -303,10 +303,18 @@ incomplete and I had trouble with their installation. It's not clear
if some of the packages are still being actively developed and
supported.
The one I recommend, since I have successfully used it with LAMMPS, is
Pypar. Pypar requires the ubiquitous "Numpy
package"_http://numpy.scipy.org be installed in your Python. After
launching python, type
The packages Pypar and mpi4py have both been successfully tested with
LAMMPS. Pypar is simpler and easy to set up and use, but supports
only a subset of MPI. Mpi4py is more MPI-feature complete, but also a
bit more complex to use. As of version 2.0.0, mpi4py is the only
python MPI wrapper that allows passing a custom MPI communicator to
the LAMMPS constructor, which means one can easily run one or more
LAMMPS instances on subsets of the total MPI ranks.
:line
Pypar requires the ubiquitous "Numpy package"_http://numpy.scipy.org
be installed in your Python. After launching Python, type
import numpy :pre
@ -361,6 +369,51 @@ the right one.
:line
To install mpi4py (version mpi4py-2.0.0 as of Oct 2015), unpack it
and from its main directory, type
python setup.py build
sudo python setup.py install :pre
Again, the "sudo" is only needed if required to copy mpi4py files into
your Python distribution's site-packages directory. To install with
user privilege into the user local directory type
python setup.py install --user :pre
If you have successully installed mpi4py, you should be able to run
Python and type
from mpi4py import MPI :pre
without error. You should also be able to run python in parallel
on a simple test script
% mpirun -np 4 python test.py :pre
where test.py contains the lines
from mpi4py import MPI
comm = MPI.COMM_WORLD
print "Proc %d out of %d procs" % (comm.Get_rank(),comm.Get_size()) :pre
and see one line of output for each processor you run on.
IMPORTANT NOTE: To use mpi4py and LAMMPS in parallel from Python, you
must insure both are using the same version of MPI. If you only have
one MPI installed on your system, this is not an issue, but it can be
if you have multiple MPIs. Your LAMMPS build is explicit about which
MPI it is using, since you specify the details in your lo-level
src/MAKE/Makefile.foo file. Mpi4py uses the "mpicc" command to find
information about the MPI it uses to build against. And it tries to
load "libmpi.so" from the LD_LIBRARY_PATH. This may or may not find
the MPI library that LAMMPS is using. If you have problems running
both mpi4py and LAMMPS together, this is an issue you may need to
address, e.g. by moving other MPI installations so that mpi4py finds
the right one.
:line
11.6 Testing the Python-LAMMPS interface :link(py_6),h4
To test if LAMMPS is callable from Python, launch Python interactively
@ -413,8 +466,8 @@ lmp_g++ -in in.lj :pre
[Test LAMMPS and Python in parallel:] :h5
To run LAMMPS in parallel, assuming you have installed the
"Pypar"_http://datamining.anu.edu.au/~ole/pypar package as discussed
above, create a test.py file containing these lines:
"Pypar"_Pypar package as discussed above, create a test.py file
containing these lines:
import pypar
from lammps import lammps
@ -423,7 +476,20 @@ lmp.file("in.lj")
print "Proc %d out of %d procs has" % (pypar.rank(),pypar.size()),lmp
pypar.finalize() :pre
You can then run it in parallel as:
To run LAMMPS in parallel, assuming you have installed the
"mpi4py"_mpi4py package as discussed above, create a test.py file
containing these lines:
from mpi4py import MPI
from lammps import lammps
lmp = lammps()
lmp.file("in.lj")
me = MPI.COMM_WORLD.Get_rank()
nprocs = MPI.COMM_WORLD.Get_size()
print "Proc %d out of %d procs has" % (me,nprocs),lmp
MPI.Finalize() :pre
You can either script in parallel as:
% mpirun -np 4 python test.py :pre
@ -491,10 +557,11 @@ correspond one-to-one with calls you can make to the LAMMPS library
from a C++ or C or Fortran program.
lmp = lammps() # create a LAMMPS object using the default liblammps.so library
lmp = lammps(ptr=lmpptr) # ditto, but use lmpptr as previously created LAMMPS object
lmp = lammps("g++") # create a LAMMPS object using the liblammps_g++.so library
lmp = lammps("",list) # ditto, with command-line args, e.g. list = \["-echo","screen"\]
lmp = lammps("g++",list) :pre
4 optional args are allowed: name, cmdargs, ptr, comm
lmp = lammps(ptr=lmpptr) # use lmpptr as previously created LAMMPS object
lmp = lammps(comm=split) # create a LAMMPS object with a custom communicator, requires mpi4py 2.0.0 or later
lmp = lammps(name="g++") # create a LAMMPS object using the liblammps_g++.so library
lmp = lammps(name="g++",cmdargs=list) # add LAMMPS command-line args, e.g. list = \["-echo","screen"\] :pre
lmp.close() # destroy a LAMMPS object :pre
@ -717,7 +784,8 @@ distribution.
trivial.py, read/run a LAMMPS input script thru Python,
demo.py, invoke various LAMMPS library interface routines,
simple.py, mimic operation of couple/simple/simple.cpp in Python,
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 temeperature plot with GnuPlot via Pizza.py,
viz_tool.py, real-time viz via some viz package,

Binary file not shown.

After

Width:  |  Height:  |  Size: 2.9 KiB

BIN
doc/_images/hexorder.jpg Normal file

Binary file not shown.

After

Width:  |  Height:  |  Size: 16 KiB

BIN
doc/_images/orientorder.jpg Normal file

Binary file not shown.

After

Width:  |  Height:  |  Size: 34 KiB

View File

@ -159,15 +159,17 @@ and the reference (bond) vector r_ij:</p>
angle.</p>
<p>The torque on the dipole can be obtained by differentiating the
potential using the &#8216;chain rule&#8217; as in appendix C.3 of
<a class="reference internal" href="pair_gayberne.html#allen"><span>(Allen)</span></a>:</p>
<a class="reference internal" href="#allen"><span>(Allen)</span></a>:</p>
<img alt="_images/angle_dipole_torque.jpg" class="align-center" src="_images/angle_dipole_torque.jpg" />
<p>Example: if gamma0 is set to 0 degrees, the torque generated by
the potential will tend to align the dipole along the reference
direction defined by the (bond) vector r_ij (in other words, mu_j is
restrained to point towards atom &#8216;i&#8217;).</p>
<p>Note that the angle dipole potential does not give rise to any force,
because it does not depend on the distance between i and j (it only
depends on the angle between mu_j and r_ij).</p>
<p>The dipolar torque T_j must be counterbalanced in order to conserve
the local angular momentum. This is achieved via an additional force
couple generating a torque equivalent to the opposite of T_j:</p>
<img alt="_images/angle_dipole_couple.jpg" class="align-center" src="_images/angle_dipole_couple.jpg" />
<p>where F_i and F_j are applied on atoms i and j, respectively.</p>
<p>The following coefficients must be defined for each angle type via the
<a class="reference internal" href="angle_coeff.html"><em>angle_coeff</em></a> command as in the example above, or in
the data file or restart files read by the <a class="reference internal" href="read_data.html"><em>read_data</em></a>

View File

@ -50,9 +50,13 @@ the potential will tend to align the dipole along the reference
direction defined by the (bond) vector r_ij (in other words, mu_j is
restrained to point towards atom 'i').
Note that the angle dipole potential does not give rise to any force,
because it does not depend on the distance between i and j (it only
depends on the angle between mu_j and r_ij).
The dipolar torque T_j must be counterbalanced in order to conserve
the local angular momentum. This is achieved via an additional force
couple generating a torque equivalent to the opposite of T_j:
:c,image(Eqs/angle_dipole_couple.jpg)
where F_i and F_j are applied on atoms i and j, respectively.
The following coefficients must be defined for each angle type via the
"angle_coeff"_angle_coeff.html command as in the example above, or in

View File

@ -145,8 +145,7 @@
<div class="section" id="description">
<h2>Description<a class="headerlink" href="#description" title="Permalink to this headline"></a></h2>
<p>Define a computation that calculates the temperatures of core-Drude
pairs. This compute is designed to be used with the thermalized Drude
oscillator model. This compute is designed to be used with the
pairs. This compute is designed to be used with the
<a class="reference internal" href="tutorial_drude.html"><em>thermalized Drude oscillator model</em></a>. Polarizable
models in LAMMPS are described in <a class="reference internal" href="Section_howto.html#howto-25"><span>this Section</span></a>.</p>
<p>Drude oscillators consist of a core particle and a Drude particle
@ -189,7 +188,7 @@ assumed to be constant for the duration of the run unless the
</div>
<div class="section" id="related-commands">
<h2>Related commands<a class="headerlink" href="#related-commands" title="Permalink to this headline"></a></h2>
<p><a class="reference internal" href="fix_drude.html"><em>fix drude</em></a>, <a class="reference internal" href="fix_langevin_drude.html"><em>fix langevin_drude</em></a>, <a class="reference internal" href="fix_drude_transform.html"><em>fix drude/transform</em></a>, <a class="reference internal" href="pair_thole.html"><em>pair_style thole</em></a>, <a class="reference internal" href="compute_temp.html"><em>compute temp</em></a></p>
<p><a class="reference internal" href="fix_drude.html"><em>fix drude</em></a>, <a class="reference internal" href="fix_langevin_drude.html"><em>fix langevin/drude</em></a>, <a class="reference internal" href="fix_drude_transform.html"><em>fix drude/transform</em></a>, <a class="reference internal" href="pair_thole.html"><em>pair_style thole</em></a>, <a class="reference internal" href="compute_temp.html"><em>compute temp</em></a></p>
<p><strong>Default:</strong> none</p>
</div>
</div>

View File

@ -22,8 +22,7 @@ compute TDRUDE all temp/drude :pre
[Description:]
Define a computation that calculates the temperatures of core-Drude
pairs. This compute is designed to be used with the thermalized Drude
oscillator model. This compute is designed to be used with the
pairs. This compute is designed to be used with the
"thermalized Drude oscillator model"_tutorial_drude.html. Polarizable
models in LAMMPS are described in "this
Section"_Section_howto.html#howto_25.
@ -75,7 +74,7 @@ assumed to be constant for the duration of the run unless the
[Related commands:]
"fix drude"_fix_drude.html, "fix
langevin_drude"_fix_langevin_drude.html, "fix
langevin/drude"_fix_langevin_drude.html, "fix
drude/transform"_fix_drude_transform.html, "pair_style
thole"_pair_thole.html, "compute temp"_compute_temp.html

View File

@ -1,30 +0,0 @@
This is TeX, Version 3.14159 (Web2C 7.4.5) (format=latex 2008.11.14) 27 AUG 2011 15:16
**pair_sph_tait
(/usr/share/texmf/tex/latex/tools/.tex
LaTeX2e <2001/06/01>
Babel <v3.7h> and hyphenation patterns for american, french, german, ngerman, n
ohyphenation, loaded.
File ignored)
*
(Please type a command or say `\end')
*x
! LaTeX Error: Missing \begin{document}.
See the LaTeX manual or LaTeX Companion for explanation.
Type H <return> for immediate help.
...
<*> x
? x
Here is how much of TeX's memory you used:
6 strings out of 95847
257 string characters out of 1195947
44507 words of memory out of 1000001
3034 multiletter control sequences out of 10000+50000
3640 words of font info for 14 fonts, out of 500000 for 1000
14 hyphenation exceptions out of 1000
5i,0n,4p,93b,14s stack positions out of 1500i,500n,5000p,200000b,5000s
No pages of output.

Binary file not shown.

Before

Width:  |  Height:  |  Size: 3.8 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K (\theta - \theta_0)^2 + K_{UB} (r - r_{UB})^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 16 KiB

View File

@ -1,12 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
\begin{eqnarray*}
E & = & E_a + E_{bb} + E_{ba} \\
E_a & = & K_2 (\theta - \theta_0)^2 + K_3 (\theta - \theta_0)^3 + K_4 (\theta - \theta_0)^4 \\
E_{bb} & = & M (r_{ij} - r_1) (r_{jk} - r_2) \\
E_{ba} & = & N_1 (r_{ij} - r_1) (\theta - \theta_0) + N_2 (r_{jk} - r_2) (\theta - \theta_0)
\end{eqnarray*}
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.3 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K [1 + \cos(\theta)]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.5 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K [1 - \cos(\theta - \theta_0)]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 3.3 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
E=C\left[ 1-B(-1)^ncos\left( n\theta\right) \right]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 3.8 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
E=-\frac{Umin}{2} \left[ 1+Cos(\theta-\theta_0) \right]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 7.7 KiB

View File

@ -1,13 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
E=-U_{min}
\frac{e^{-a U(\theta,\theta_0)}-1}{e^a-1}
\quad\mbox{with}\quad
U(\theta,\theta_0)
=-0.5 \left(1+\cos(\theta-\theta_0) \right)
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 3.2 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K [\cos(\theta) - \cos(\theta_0)]^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.6 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
\cos\gamma = \frac{\vec{\mu_j}\bullet\vec{r_{ij}}}{\mu_j\,r_{ij}}
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.6 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K (\cos\gamma - \cos\gamma_0)^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 5.0 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
\vec{T_j} = \frac{2K(\cos\gamma - \cos\gamma_0)}{\mu_j\,r_{ij}}\,
\vec{r_{ij}} \times \vec{\mu_j}
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 4.5 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K [C_0 + C_1 \cos ( \theta) + C_2 \cos( 2 \theta) ]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.7 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K [ 1.0 + c \cos ( n \theta) ]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.0 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K (\theta - \theta_0)^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 5.1 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K_2 (\theta - \theta_0)^2 + K_3 (\theta - \theta_0)^3 + K_4 (\theta - \theta_0)^4
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 5.0 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K_2 (r - r_0)^2 + K_3 (r - r_0)^3 + K_4 (r - r_0)^4
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 8.1 KiB

View File

@ -1,11 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = -0.5 K R_0^2 \ln \left[ 1 - \left(\frac{r}{R_0}\right)^2\right] +
4 \epsilon \left[ \left(\frac{\sigma}{r}\right)^{12} -
\left(\frac{\sigma}{r}\right)^6 \right] + \epsilon
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 11 KiB

View File

@ -1,13 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = -0.5 K R_0^2
\ln \left[1 -\left( \frac{\left(r - \Delta\right)}{R_0}\right)^2 \right] +
4 \epsilon \left[ \left(\frac{\sigma}{\left(r -
\Delta\right)}\right)^{12} - \left(\frac{\sigma}{\left(r -
\Delta\right)}\right)^6 \right] + \epsilon
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 1.8 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K (r - r_0)^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 5.0 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = \frac{Umin}{(r_0-r_c)^2} \left[ (r-r_0)^2-(r_c-r_0)^2 \right]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 5.1 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = \frac{Umin}{(r_0-r_c)^2} \left[ (r-r_0)^2-(r_c-r_0)^2 \right]
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.5 KiB

View File

@ -1,10 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
% E = D \left[ 1 - \exp \left( -\alpha (r - r_0) \right) \right]^2
E = D \left[ 1 - e^{-\alpha (r - r_0)} \right]^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 3.5 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = \frac{\epsilon (r - r_0)^2}{ [ \lambda^2 - (r - r_0)^2 ]}
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 9.3 KiB

View File

@ -1,11 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
E = K (r - R_c)^ 2 (r - R_c - B_1) (r - R_c - B_2) + U_0 +
4 \epsilon \left[ \left(\frac{\sigma}{r}\right)^{12} -
\left(\frac{\sigma}{r}\right)^6 \right] + \epsilon
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 11 KiB

View File

@ -1,14 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
\begin{eqnarray*}
a &=& {\rm lx} \\
b^2 &=& {\rm ly}^2 + {\rm xy}^2 \\
c^2 &=& {\rm lz}^2 + {\rm xz}^2 + {\rm yz}^2 \\
\cos{\alpha} &=& \frac{{\rm xy}*{\rm xz} + {\rm ly}*{\rm yz}}{b*c} \\
\cos{\beta} &=& \frac{\rm xz}{c} \\
\cos{\gamma} &=& \frac{\rm xy}{b} \\
\end{eqnarray*}
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 10 KiB

View File

@ -1,14 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
\begin{eqnarray*}
{\rm lx} &=& a \\
{\rm xy} &=& b \cos{\gamma} \\
{\rm xz} &=& c \cos{\beta}\\
{\rm ly}^2 &=& b^2 - {\rm xy}^2 \\
{\rm yz} &=& \frac{b*c \cos{\alpha} - {\rm xy}*{\rm xz}}{\rm ly} \\
{\rm lz}^2 &=& c^2 - {\rm xz}^2 - {\rm yz}^2 \\
\end{eqnarray*}
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 4.0 KiB

View File

@ -1,9 +0,0 @@
\documentclass[12pt]{article}
\begin{document}
$$
CS = \sum_{i = 1}^{N/2} | \vec{R}_i + \vec{R}_{i+N/2} |^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 13 KiB

View File

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

Binary file not shown.

Before

Width:  |  Height:  |  Size: 2.5 KiB

View File

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

Binary file not shown.

Before

Width:  |  Height:  |  Size: 18 KiB

View File

@ -1,7 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\[ \left< \frac{1}{1 + \exp\left[\left(U_1 - U_0 - \Delta_0^1A \right) /kT \right]} \right>_0 = \left< \frac{1}{1 + \exp\left[\left(U_0 - U_1 + \Delta_0^1A \right) /kT \right]} \right>_1 \]
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 15 KiB

View File

@ -1,10 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\[ \Delta_0^1 A = \int_{\lambda=0}^{\lambda=1} \left( \frac{\partial
A(\lambda)}{\partial\lambda} \right)_\lambda \mathrm{d}\lambda
\approx \sum_{i=0}^{n-1} w_i \frac{A(\lambda_{i} + \delta) -
A(\lambda_i)}{\delta} \]
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 18 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\[ \Delta_0^1 A = \sum_{i=0}^{n-1} \Delta_{\lambda_i}^{\lambda_{i+1}} A =
- kT \sum_{i=0}^{n-1} \ln \left< \exp \left( - \frac{U(\lambda_{i+1}) -
U(\lambda_i)}{kT} \right) \right>_{\lambda_i} \]
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 10 KiB

View File

@ -1,10 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\begin{eqnarray*}
\lambda = 0 \quad\Rightarrow\quad U = U_{\mathrm{bg}} + U_0 \\
\lambda = 1 \quad\Rightarrow\quad U = U_{\mathrm{bg}} + U_1
\end{eqnarray*}
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 18 KiB

View File

@ -1,10 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\[ \Delta_0^1 A = \int_{\lambda=0}^{\lambda=1} \left< \frac{\partial
U(\lambda)}{\partial\lambda} \right>_\lambda \mathrm{d}\lambda
\approx \sum_{i=0}^{n-1} w_i \left< \frac{U(\lambda_{i} + \delta) -
U(\lambda_i)}{\delta} \right>_{\lambda_i} \]
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 9.1 KiB

View File

@ -1,7 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\[ U(\lambda) = U_{\mathrm{bg}} + U_1(\lambda) + U_0(\lambda) \]
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 15 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
\[ \Delta_0^1 A = - kT \sum_{i=0}^{n-1} \ln \frac{\left< V \exp \left( -
\frac{U(\lambda_{i+1}) - U(\lambda_i)}{kT} \right)
\right>_{\lambda_i}}{\left< V \right>_{\lambda_i}} \]
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 3.6 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
{R_g}^2 = \frac{1}{M} \sum_i m_i (r_i - r_{cm})^2
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 7.1 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
NGP(t) = 3<(r(t)-r(0))^4>/(5<(r(t)-r(0))^2>^2) - 1
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 1.4 KiB

View File

@ -1,10 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
I=\frac{F^{*}F}{N}
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 4.8 KiB

View File

@ -1,9 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
F(\mathbf{k})=\sum_{j=1}^{N}f_j(\theta)exp(2\pi i \mathbf{k}\cdot \mathbf{r}_j)
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 6.9 KiB

View File

@ -1,10 +0,0 @@
\documentstyle[12pt]{article}
\begin{document}
$$
f_j\left ( \frac{sin(\theta)}{\lambda} \right )=\sum_{i}^{5}
a_i exp\left ( -b_i \frac{sin^{2}(\theta)}{\lambda^{2}} \right )
$$
\end{document}

Binary file not shown.

Before

Width:  |  Height:  |  Size: 19 KiB

View File

@ -1,11 +0,0 @@
\documentclass[24pt]{article}
\pagestyle{empty}
\begin{document}
\begin{eqnarray*}
\theta_0 = {\tt rfac0} \frac{r-r_{min0}}{R_{ii'}-r_{min0}} \pi
\end{eqnarray*}
\end{document}

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