git-svn-id: svn://svn.icms.temple.edu/lammps-ro/trunk@3495 f3b2605a-c512-4ea7-a41b-209d697bcdaa
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@ -56,10 +56,11 @@ inertia for a sphere and w is the particle's angular velocity.
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as spheres, not disks, meaning their moment of inertia will be the
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same as in 3d.
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</P>
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<P>A 6-component kinetic energy tensor is also calculated by this
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compute. The formula for the components of the tensor is the same as
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the above formulas, except that v^2 and w^2 are replaced by vx*vy and
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wx*wy for the xy component.
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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. The formula for the components of the
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tensor is the same as the above formulas, except that v^2 and w^2 are
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replaced by vx*vy and wx*wy for the xy component. The 6 components of
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the vector are ordered xx, yy, zz, xy, xz, yz.
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</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 <I>dynamic</I> option of the
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@ -88,6 +89,13 @@ thermostatting.
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</P>
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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 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 HREF = "Section_howto.html#4_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 value calculated by this compute is "intensive", meaning it
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is independent of the number of atoms in the simulation. The vector
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values are "extensive", meaning they scale with the number of atoms in
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