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<li class="toctree-l1"><a class="reference internal" href="Section_intro.html">1. Introduction</a></li>
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<li class="toctree-l1"><a class="reference internal" href="Section_accelerate.html">5. Accelerating LAMMPS performance</a></li>
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<li class="toctree-l1"><a class="reference internal" href="Section_errors.html">12. Errors</a></li>
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<li>compute temp/partial command</li>
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<div class="section" id="compute-temp-partial-command">
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<span id="index-0"></span><h1>compute temp/partial command</h1>
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<div class="section" id="syntax">
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<h2>Syntax</h2>
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<div class="highlight-default"><div class="highlight"><pre><span></span><span class="n">compute</span> <span class="n">ID</span> <span class="n">group</span><span class="o">-</span><span class="n">ID</span> <span class="n">temp</span><span class="o">/</span><span class="n">partial</span> <span class="n">xflag</span> <span class="n">yflag</span> <span class="n">zflag</span>
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</pre></div>
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</div>
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<ul class="simple">
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<li>ID, group-ID are documented in <a class="reference internal" href="compute.html"><span class="doc">compute</span></a> command</li>
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<li>temp/partial = style name of this compute command</li>
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<li>xflag,yflag,zflag = 0/1 for whether to exclude/include this dimension</li>
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</ul>
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</div>
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<div class="section" id="examples">
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<h2>Examples</h2>
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<div class="highlight-default"><div class="highlight"><pre><span></span><span class="n">compute</span> <span class="n">newT</span> <span class="n">flow</span> <span class="n">temp</span><span class="o">/</span><span class="n">partial</span> <span class="mi">1</span> <span class="mi">1</span> <span class="mi">0</span>
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</pre></div>
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</div>
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</div>
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<div class="section" id="description">
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<h2>Description</h2>
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<p>Define a computation that calculates the temperature of a group of
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atoms, after excluding one or more velocity components. A compute of
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this style can be used by any command that computes a temperature,
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e.g. <a class="reference internal" href="thermo_modify.html"><span class="doc">thermo_modify</span></a>, <a class="reference internal" href="fix_temp_rescale.html"><span class="doc">fix temp/rescale</span></a>, <a class="reference internal" href="fix_nh.html"><span class="doc">fix npt</span></a>, etc.</p>
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<p>The temperature is calculated by the formula KE = dim/2 N k T, where
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KE = total kinetic energy of the group of atoms (sum of 1/2 m v^2),
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dim = dimensionality of the simulation, N = number of atoms in the
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group, k = Boltzmann constant, and T = temperature. The calculation
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of KE excludes the x, y, or z dimensions if xflag, yflag, or zflag =
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0. The dim parameter is adjusted to give the correct number of
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degrees of freedom.</p>
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<p>A kinetic energy tensor, stored as a 6-element vector, is also
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calculated by this compute for use in the calculation of a pressure
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tensor. The formula for the components of the tensor is the same as
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the above formula, except that v^2 is replaced by vx*vy for the xy
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component, etc. The 6 components of the vector are ordered xx, yy,
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zz, xy, xz, yz.</p>
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<p>The number of atoms contributing to the temperature is assumed to be
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constant for the duration of the run; use the <em>dynamic</em> option of the
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<a class="reference internal" href="compute_modify.html"><span class="doc">compute_modify</span></a> command if this is not the case.</p>
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<p>The removal of velocity components by this fix is essentially
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computing the temperature after a “bias” has been removed from the
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velocity of the atoms. If this compute is used with a fix command
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that performs thermostatting then this bias will be subtracted from
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each atom, thermostatting of the remaining thermal velocity will be
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performed, and the bias will be added back in. Thermostatting fixes
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that work in this way include <a class="reference internal" href="fix_nh.html"><span class="doc">fix nvt</span></a>, <a class="reference internal" href="fix_temp_rescale.html"><span class="doc">fix temp/rescale</span></a>, <a class="reference internal" href="fix_temp_berendsen.html"><span class="doc">fix temp/berendsen</span></a>, and <a class="reference internal" href="fix_langevin.html"><span class="doc">fix langevin</span></a>.</p>
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<p>This compute subtracts out degrees-of-freedom due to fixes that
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constrain molecular motion, such as <a class="reference internal" href="fix_shake.html"><span class="doc">fix shake</span></a> and
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<a class="reference internal" href="fix_rigid.html"><span class="doc">fix rigid</span></a>. This means the temperature of groups of
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atoms that include these constraints will be computed correctly. If
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needed, the subtracted degrees-of-freedom can be altered using the
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<em>extra</em> option of the <a class="reference internal" href="compute_modify.html"><span class="doc">compute_modify</span></a> command.</p>
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<p>See <a class="reference internal" href="Section_howto.html#howto-16"><span class="std std-ref">this howto section</span></a> of the manual for
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a discussion of different ways to compute temperature and perform
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thermostatting.</p>
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<hr class="docutils" />
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<p>Styles with a <em>gpu</em>, <em>intel</em>, <em>kk</em>, <em>omp</em>, or <em>opt</em> suffix are
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functionally the same as the corresponding style without the suffix.
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They have been optimized to run faster, depending on your available
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hardware, as discussed in <a class="reference internal" href="Section_accelerate.html"><span class="doc">Section_accelerate</span></a>
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of the manual. The accelerated styles take the same arguments and
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should produce the same results, except for round-off and precision
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issues.</p>
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<p>These accelerated styles are part of the GPU, USER-INTEL, KOKKOS,
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USER-OMP and OPT packages, respectively. They are only enabled if
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LAMMPS was built with those packages. See the <a class="reference internal" href="Section_start.html#start-3"><span class="std std-ref">Making LAMMPS</span></a> section for more info.</p>
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<p>You can specify the accelerated styles explicitly in your input script
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by including their suffix, or you can use the <a class="reference internal" href="Section_start.html#start-7"><span class="std std-ref">-suffix command-line switch</span></a> when you invoke LAMMPS, or you can
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use the <a class="reference internal" href="suffix.html"><span class="doc">suffix</span></a> command in your input script.</p>
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<p>See <a class="reference internal" href="Section_accelerate.html"><span class="doc">Section_accelerate</span></a> of the manual for
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more instructions on how to use the accelerated styles effectively.</p>
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<hr class="docutils" />
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<p><strong>Output info:</strong></p>
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<p>This compute calculates a global scalar (the temperature) and a global
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vector of length 6 (KE tensor), which can be accessed by indices 1-6.
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These values can be used by any command that uses global scalar or
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vector values from a compute as input. See <a class="reference internal" href="Section_howto.html#howto-15"><span class="std std-ref">this section</span></a> for an overview of LAMMPS output
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options.</p>
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<p>The scalar value calculated by this compute is “intensive”. The
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vector values are “extensive”.</p>
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<p>The scalar value will be in temperature <a class="reference internal" href="units.html"><span class="doc">units</span></a>. The
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vector values will be in energy <a class="reference internal" href="units.html"><span class="doc">units</span></a>.</p>
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</div>
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<div class="section" id="restrictions">
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<h2>Restrictions</h2>
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<blockquote>
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<div>none</div></blockquote>
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</div>
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<div class="section" id="related-commands">
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<h2>Related commands</h2>
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<p><a class="reference internal" href="compute_temp.html"><span class="doc">compute temp</span></a>, <a class="reference internal" href="compute_temp_region.html"><span class="doc">compute temp/region</span></a>, <a class="reference internal" href="compute_pressure.html"><span class="doc">compute pressure</span></a></p>
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<p><strong>Default:</strong> none</p>
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