forked from lijiext/lammps
136 lines
5.6 KiB
HTML
136 lines
5.6 KiB
HTML
<HTML>
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<CENTER><A HREF = "http://lammps.sandia.gov">LAMMPS WWW Site</A> - <A HREF = "Manual.html">LAMMPS Documentation</A> - <A HREF = "Section_commands.html#comm">LAMMPS Commands</A>
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<HR>
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<H3>compute pressure command
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</H3>
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<H3>compute pressure/cuda command
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</H3>
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<P><B>Syntax:</B>
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</P>
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<PRE>compute ID group-ID pressure temp-ID keyword ...
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</PRE>
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<UL><LI>ID, group-ID are documented in <A HREF = "compute.html">compute</A> command
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<LI>pressure = style name of this compute command
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<LI>temp-ID = ID of compute that calculates temperature
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<LI>zero or more keywords may be appended
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<LI>keyword = <I>ke</I> or <I>pair</I> or <I>bond</I> or <I>angle</I> or <I>dihedral</I> or <I>improper</I> or <I>kspace</I> or <I>fix</I> or <I>virial</I>
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</UL>
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<P><B>Examples:</B>
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</P>
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<PRE>compute 1 all pressure myTemp
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compute 1 all pressure thermo_temp pair bond
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</PRE>
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<P><B>Description:</B>
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</P>
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<P>Define a computation that calculates the pressure of the entire system
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of atoms. The specified group must be "all". See the <A HREF = "compute_stress_atom.html">compute
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stress/atom</A> command if you want per-atom
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pressure (stress). These per-atom values could be summed for a group
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of atoms via the <A HREF = "compute_reduce.html">compute reduce</A> command.
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</P>
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<P>The pressure is computed by the formula
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</P>
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<CENTER><IMG SRC = "Eqs/pressure.jpg">
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</CENTER>
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<P>where N is the number of atoms in the system (see discussion of DOF
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below), Kb is the Boltzmann constant, T is the temperature, d is the
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dimensionality of the system (2 or 3 for 2d/3d), V is the system
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volume (or area in 2d), and the second term is the virial, computed
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within LAMMPS for all pairwise as well as 2-body, 3-body, and 4-body,
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and long-range interactions. <A HREF = "fix.html">Fixes</A> that impose constraints
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(e.g. the <A HREF = "fix_shake.html">fix shake</A> command) also contribute to the
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virial term.
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</P>
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<P>A symmetric pressure tensor, stored as a 6-element vector, is also
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calculated by this compute. The 6 components of the vector are
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ordered xx, yy, zz, xy, xz, yz. The equation for the I,J components
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(where I and J = x,y,z) is similar to the above formula, except that
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the first term uses components of the kinetic energy tensor and the
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second term uses components of the virial tensor:
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</P>
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<CENTER><IMG SRC = "Eqs/pressure_tensor.jpg">
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</CENTER>
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<P>If no extra keywords are listed, the entire equations above are
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calculated which include a kinetic energy (temperature) term and the
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virial as the sum of pair, bond, angle, dihedral, improper, kspace
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(long-range), and fix contributions to the force on each atom. If any
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extra keywords are listed, then only those components are summed to
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compute temperature or ke and/or the virial. The <I>virial</I> keyword
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means include all terms except the kinetic energy <I>ke</I>.
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</P>
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<P>The temperature and kinetic energy tensor is not calculated by this
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compute, but rather by the temperature compute specified with the
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command. Normally this compute should calculate the temperature of
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all atoms for consistency with the virial term, but any compute style
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that calculates temperature can be used, e.g. one that excludes frozen
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atoms or other degrees of freedom.
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</P>
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<P>Note that the N in the first formula above is really
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degrees-of-freedom divided by d = dimensionality, where the DOF value
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is calcluated by the temperature compute. See the various <A HREF = "compute.html">compute
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temperature</A> styles for details.
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</P>
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<P>A compute of this style with the ID of "thermo_press" is created when
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LAMMPS starts up, as if this command were in the input script:
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</P>
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<PRE>compute thermo_press all pressure thermo_temp
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</PRE>
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<P>where "thermo_temp" is the ID of a similarly defined compute of style
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"temp". See the "thermo_style" command for more details.
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</P>
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<HR>
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<P>Styles with a <I>cuda</I> suffix are functionally the same as the
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corresponding style without the suffix. They have been optimized to
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run faster, depending on your available hardware, as discussed in
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<A HREF = "Section_accelerate.html">this section</A> of the manual. The accelerated
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styles take the same arguments and should produce the same results,
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except for round-off and precision issues.
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</P>
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<P>These accelerated styles are part of the "user-cuda" package. They
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are only enabled if LAMMPS was built with that package. See the
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<A HREF = "Section_start.html#start_3">Making LAMMPS</A> section for more info.
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</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 HREF = "Section_start.html#start_6">-suffix command-line
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switch</A> when you invoke LAMMPS, or you can
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use the <A HREF = "suffix.html">suffix</A> command in your input script.
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</P>
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<P>See <A HREF = "Section_accelerate.html">this section</A> of the manual for more
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instructions on how to use the accelerated styles effectively.
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</P>
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<HR>
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<P><B>Output info:</B>
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</P>
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<P>This compute calculates a global scalar (the pressure) and a global
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vector of length 6 (pressure tensor), which can be accessed by indices
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1-6. These values can be used by any command that uses global scalar
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or vector values from a compute as input. See <A HREF = "Section_howto.html#howto_15">this
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section</A> for an overview of LAMMPS output
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options.
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</P>
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<P>The scalar and vector values calculated by this compute are
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"intensive". The scalar and vector values will be in pressure
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<A HREF = "units.html">units</A>.
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</P>
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<P><B>Restrictions:</B> none
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</P>
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<P><B>Related commands:</B>
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</P>
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<P><A HREF = "compute_temp.html">compute temp</A>, <A HREF = "compute_stress_atom.html">compute
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stress/atom</A>,
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<A HREF = "thermo_style.html">thermo_style</A>,
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</P>
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<P><B>Default:</B> none
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</P>
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</HTML>
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