Homec4science
Diffusion lammps (lammm-master-deprecated) Browse

lammps/doc/compute_temp_asphere.html
c6213f36d34clammm-master-deprecated

Last Change
Raw File

compute_temp_asphere.html
View Options

<!DOCTYPE html>
<!--[if IE 8]><html class="no-js lt-ie9" lang="en" > <![endif]-->
<!--[if gt IE 8]><!--> <html class="no-js" lang="en" > <!--<![endif]-->
<head>
<meta charset="utf-8">
<meta name="viewport" content="width=device-width, initial-scale=1.0">
<title>compute temp/asphere command &mdash; LAMMPS 15 May 2015 version documentation</title>
<link rel="stylesheet" href="_static/css/theme.css" type="text/css" />
<link rel="stylesheet" href="_static/sphinxcontrib-images/LightBox2/lightbox2/css/lightbox.css" type="text/css" />
<link rel="top" title="LAMMPS 15 May 2015 version documentation" href="index.html"/>
<script src="_static/js/modernizr.min.js"></script>
</head>
<body class="wy-body-for-nav" role="document">
<div class="wy-grid-for-nav">
<nav data-toggle="wy-nav-shift" class="wy-nav-side">
<div class="wy-side-nav-search">
<a href="Manual.html" class="icon icon-home"> LAMMPS
</a>
<div role="search">
<form id="rtd-search-form" class="wy-form" action="search.html" method="get">
<input type="text" name="q" placeholder="Search docs" />
<input type="hidden" name="check_keywords" value="yes" />
<input type="hidden" name="area" value="default" />
</form>
</div>
</div>
<div class="wy-menu wy-menu-vertical" data-spy="affix" role="navigation" aria-label="main navigation">
<ul>
<li class="toctree-l1"><a class="reference internal" href="Section_intro.html">1. Introduction</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_start.html">2. Getting Started</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_commands.html">3. Commands</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_packages.html">4. Packages</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_accelerate.html">5. Accelerating LAMMPS performance</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_howto.html">6. How-to discussions</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_example.html">7. Example problems</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_perf.html">8. Performance &amp; scalability</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_tools.html">9. Additional tools</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_modify.html">10. Modifying &amp; extending LAMMPS</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_python.html">11. Python interface to LAMMPS</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_errors.html">12. Errors</a></li>
<li class="toctree-l1"><a class="reference internal" href="Section_history.html">13. Future and history</a></li>
</ul>
</div>
&nbsp;
</nav>
<section data-toggle="wy-nav-shift" class="wy-nav-content-wrap">
<nav class="wy-nav-top" role="navigation" aria-label="top navigation">
<i data-toggle="wy-nav-top" class="fa fa-bars"></i>
<a href="Manual.html">LAMMPS</a>
</nav>
<div class="wy-nav-content">
<div class="rst-content">
<div role="navigation" aria-label="breadcrumbs navigation">
<ul class="wy-breadcrumbs">
<li><a href="Manual.html">Docs</a> &raquo;</li>
<li>compute temp/asphere command</li>
<li class="wy-breadcrumbs-aside">
<a href="http://lammps.sandia.gov">Homepage</a>
<a href="Section_commands.html#comm">Commands</a>
</li>
</ul>
<hr/>
</div>
<div role="main" class="document" itemscope="itemscope" itemtype="http://schema.org/Article">
<div itemprop="articleBody">
<div class="section" id="compute-temp-asphere-command">
<span id="index-0"></span><h1>compute temp/asphere command<a class="headerlink" href="#compute-temp-asphere-command" title="Permalink to this headline"></a></h1>
<div class="section" id="syntax">
<h2>Syntax<a class="headerlink" href="#syntax" title="Permalink to this headline"></a></h2>
<div class="highlight-python"><div class="highlight"><pre>compute ID group-ID temp/asphere keyword value ...
</pre></div>
</div>
<ul class="simple">
<li>ID, group-ID are documented in <a class="reference internal" href="compute.html"><em>compute</em></a> command</li>
<li>temp/asphere = style name of this compute command</li>
<li>zero or more keyword/value pairs may be appended</li>
<li>keyword = <em>bias</em> or <em>dof</em></li>
</ul>
<pre class="literal-block">
<em>bias</em> value = bias-ID
bias-ID = ID of a temperature compute that removes a velocity bias
<em>dof</em> value = <em>all</em> or <em>rotate</em>
all = compute temperature of translational and rotational degrees of freedom
rotate = compute temperature of just rotational degrees of freedom
</pre>
</div>
<div class="section" id="examples">
<h2>Examples<a class="headerlink" href="#examples" title="Permalink to this headline"></a></h2>
<div class="highlight-python"><div class="highlight"><pre>compute 1 all temp/asphere
compute myTemp mobile temp/asphere bias tempCOM
compute myTemp mobile temp/asphere dof rotate
</pre></div>
</div>
</div>
<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 temperature of a group of
aspherical particles, including a contribution from both their
translational and rotational kinetic energy. This differs from the
usual <a class="reference internal" href="compute_temp.html"><em>compute temp</em></a> command, which assumes point
particles with only translational kinetic energy.</p>
<p>Only finite-size particles (aspherical or spherical) can be included
in the group. For 3d finite-size particles, each has 6 degrees of
freedom (3 translational, 3 rotational). For 2d finite-size
particles, each has 3 degrees of freedom (2 translational, 1
rotational).</p>
<div class="admonition warning">
<p class="first admonition-title">Warning</p>
<p class="last">This choice for degrees of freedom (dof) assumes that
all finite-size aspherical or spherical particles in your model will
freely rotate, sampling all their rotational dof. It is possible to
use a combination of interaction potentials and fixes that induce no
torque or otherwise constrain some of all of your particles so that
this is not the case. Then there are less dof and you should use the
<a class="reference internal" href="compute_modify.html"><em>compute_modify extra</em></a> command to adjust the dof
accordingly.</p>
</div>
<p>For example, an aspherical particle with all three of its shape
parameters the same is a sphere. If it does not rotate, then it
should have 3 dof instead of 6 in 3d (or 2 instead of 3 in 2d). A
uniaxial aspherical particle has two of its three shape parameters the
same. If it does not rotate around the axis perpendicular to its
circular cross section, then it should have 5 dof instead of 6 in 3d.
The latter is the case for uniaxial ellipsoids in a <a class="reference internal" href="pair_gayberne.html"><em>GayBerne model</em></a> since there is no induced torque around the
optical axis. It will also be the case for biaxial ellipsoids when
exactly two of the semiaxes have the same length and the corresponding
relative well depths are equal.</p>
<p>The translational kinetic energy is computed the same as is described
by the <a class="reference internal" href="compute_temp.html"><em>compute temp</em></a> command. The rotational
kinetic energy is computed as 1/2 I w^2, where I is the inertia tensor
for the aspherical particle and w is its angular velocity, which is
computed from its angular momentum.</p>
<div class="admonition warning">
<p class="first admonition-title">Warning</p>
<p class="last">For <a class="reference internal" href="dimension.html"><em>2d models</em></a>, particles are treated
as ellipsoids, not ellipses, meaning their moments of inertia will be
the same as in 3d.</p>
</div>
<p>A kinetic energy tensor, stored as a 6-element vector, is also
calculated by this compute. The formula for the components of the
tensor is the same as the above formula, except that v^2 and w^2 are
replaced by vx*vy and wx*wy for the xy component, and the appropriate
elements of the inertia tensor are used. The 6 components of the
vector are ordered xx, yy, zz, xy, xz, yz.</p>
<p>The number of atoms contributing to the temperature is assumed to be
constant for the duration of the run; use the <em>dynamic</em> option of the
<a class="reference internal" href="compute_modify.html"><em>compute_modify</em></a> command if this is not the case.</p>
<p>This compute subtracts out translational degrees-of-freedom due to
fixes that constrain molecular motion, such as <a class="reference internal" href="fix_shake.html"><em>fix shake</em></a> and <a class="reference internal" href="fix_rigid.html"><em>fix rigid</em></a>. This means the
temperature of groups of atoms that include these constraints will be
computed correctly. If needed, the subtracted degrees-of-freedom can
be altered using the <em>extra</em> option of the
<a class="reference internal" href="compute_modify.html"><em>compute_modify</em></a> command.</p>
<p>See <a class="reference internal" href="Section_howto.html#howto-16"><span>this howto section</span></a> of the manual for
a discussion of different ways to compute temperature and perform
thermostatting.</p>
<hr class="docutils" />
<p>The keyword/value option pairs are used in the following ways.</p>
<p>For the <em>bias</em> keyword, <em>bias-ID</em> refers to the ID of a temperature
compute that removes a &#8220;bias&#8221; velocity from each atom. This allows
compute temp/sphere to compute its thermal temperature after the
translational kinetic energy components have been altered in a
prescribed way, e.g. to remove a flow velocity profile. Thermostats
that use this compute will work with this bias term. See the doc
pages for individual computes that calculate a temperature and the doc
pages for fixes that perform thermostatting for more details.</p>
<p>For the <em>dof</em> keyword, a setting of <em>all</em> calculates a temperature
that includes both translational and rotational degrees of freedom. A
setting of <em>rotate</em> calculates a temperature that includes only
rotational degrees of freedom.</p>
<hr class="docutils" />
<p><strong>Output info:</strong></p>
<p>This compute calculates a global scalar (the temperature) and a global
vector of length 6 (KE tensor), which can be accessed by indices 1-6.
These values can be used by any command that uses global scalar or
vector values from a compute as input. See <a class="reference internal" href="Section_howto.html#howto-15"><span>this section</span></a> for an overview of LAMMPS output
options.</p>
<p>The scalar value calculated by this compute is &#8220;intensive&#8221;. The
vector values are &#8220;extensive&#8221;.</p>
<p>The scalar value will be in temperature <a class="reference internal" href="units.html"><em>units</em></a>. The
vector values will be in energy <a class="reference internal" href="units.html"><em>units</em></a>.</p>
</div>
<div class="section" id="restrictions">
<h2>Restrictions<a class="headerlink" href="#restrictions" title="Permalink to this headline"></a></h2>
<p>This compute is part of the ASPHERE package. It is only enabled if
LAMMPS was built with that package. See the <a class="reference internal" href="Section_start.html#start-3"><span>Making LAMMPS</span></a> section for more info.</p>
<p>This compute requires that atoms store angular momementum and a
quaternion as defined by the <a class="reference internal" href="atom_style.html"><em>atom_style ellipsoid</em></a>
command.</p>
<p>All particles in the group must be finite-size. They cannot be point
particles, but they can be aspherical or spherical as defined by their
shape attribute.</p>
</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="compute_temp.html"><em>compute temp</em></a></p>
<p><strong>Default:</strong> none</p>
</div>
</div>
</div>
</div>
<footer>
<hr/>
<div role="contentinfo">
<p>
&copy; Copyright .
</p>
</div>
Built with <a href="http://sphinx-doc.org/">Sphinx</a> using a <a href="https://github.com/snide/sphinx_rtd_theme">theme</a> provided by <a href="https://readthedocs.org">Read the Docs</a>.
</footer>
</div>
</div>
</section>
</div>
<script type="text/javascript">
var DOCUMENTATION_OPTIONS = {
URL_ROOT:'./',
VERSION:'15 May 2015 version',
COLLAPSE_INDEX:false,
FILE_SUFFIX:'.html',
HAS_SOURCE: true
};
</script>
<script type="text/javascript" src="_static/jquery.js"></script>
<script type="text/javascript" src="_static/underscore.js"></script>
<script type="text/javascript" src="_static/doctools.js"></script>
<script type="text/javascript" src="_static/sphinxcontrib-images/LightBox2/lightbox2/js/jquery-1.11.0.min.js"></script>
<script type="text/javascript" src="_static/sphinxcontrib-images/LightBox2/lightbox2/js/lightbox.min.js"></script>
<script type="text/javascript" src="_static/sphinxcontrib-images/LightBox2/lightbox2-customize/jquery-noconflict.js"></script>
<script type="text/javascript" src="_static/js/theme.js"></script>
<script type="text/javascript">
jQuery(function () {
SphinxRtdTheme.StickyNav.enable();
});
</script>
</body>
</html>
c4science · Help