<p>Define a computation that calculates the temperature of a group of
nuclei and electrons in the <a class="reference internal" href="pair_eff.html"><span class="doc">electron force field</span></a>
model, within a geometric region using the electron force field. A
compute of this style can be used by commands that compute a
temperature, e.g. <a class="reference internal" href="thermo_modify.html"><span class="doc">thermo_modify</span></a>.</p>
<p>The operation of this compute is exactly like that described by the
<a class="reference internal" href="compute_temp_region.html"><span class="doc">compute temp/region</span></a> command, except that
the formula for the temperature itself includes the radial electron
velocity contributions, as discussed by the <a class="reference internal" href="compute_temp_eff.html"><span class="doc">compute temp/eff</span></a> command.</p>
<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 class="std std-ref">this section</span></a> for an overview of LAMMPS output
options.</p>
<p>The scalar value calculated by this compute is “intensive”. The
vector values are “extensive”.</p>
<p>The scalar value will be in temperature <a class="reference internal" href="units.html"><span class="doc">units</span></a>. The
vector values will be in energy <a class="reference internal" href="units.html"><span class="doc">units</span></a>.</p>
</div>
<div class="section" id="restrictions">
<h2>Restrictions</h2>
<p>This compute is part of the USER-EFF 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 class="std std-ref">Making LAMMPS</span></a> section for more info.</p>
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