# compute temp/profile command

## Syntax

```
compute ID group-ID temp/profile xflag yflag zflag binstyle args
```

ID, group-ID are documented in compute command

temp/profile = style name of this compute command

xflag,yflag,zflag = 0/1 for whether to exclude/include this dimension

binstyle =

*x*or*y*or*z*or*xy*or*yz*or*xz*or*xyz**x*arg = Nx*y*arg = Ny*z*arg = Nz*xy*args = Nx Ny*yz*args = Ny Nz*xz*args = Nx Nz*xyz*args = Nx Ny Nz Nx,Ny,Nz = number of velocity bins in x,y,z dimensionszero or more keyword/value pairs may be appended

keyword =

*out**out*value =*tensor*or*bin*

## Examples

```
compute myTemp flow temp/profile 1 1 1 x 10
compute myTemp flow temp/profile 1 1 1 x 10 out bin
compute myTemp flow temp/profile 0 1 1 xyz 20 20 20
```

## Description

Define a computation that calculates the temperature of a group of atoms, after subtracting out a spatially-averaged center-of-mass velocity field, before computing the kinetic energy. This can be useful for thermostatting a collection of atoms undergoing a complex flow, e.g. via a profile-unbiased thermostat (PUT) as described in (Evans). A compute of this style can be used by any command that computes a temperature, e.g. thermo_modify, fix temp/rescale, fix npt, etc.

The *xflag*, *yflag*, *zflag* settings determine which components of
average velocity are subtracted out.

The *binstyle* setting and its *Nx*, *Ny*, *Nz* arguments determine
how bins are setup to perform spatial averaging. “Bins” can be 1d
slabs, 2d pencils, or 3d bricks depending on which *binstyle* is used.
The simulation box is partitioned conceptually into *Nx* by *Ny* by
*Nz* bins. Depending on the *binstyle*, you may only specify one or
two of these values; the others are effectively set to 1 (no binning
in that dimension). For non-orthogonal (triclinic) simulation boxes,
the bins are “tilted” slabs or pencils or bricks that are parallel to
the tilted faces of the box. See the region prism
command for a discussion of the geometry of tilted boxes in LAMMPS.

When a temperature is computed, the center-of-mass velocity for the set of atoms that are both in the compute group and in the same spatial bin is calculated. This bias velocity is then subtracted from the velocities of individual atoms in the bin to yield a thermal velocity for each atom. Note that if there is only one atom in the bin, its thermal velocity will thus be 0.0.

After the spatially-averaged velocity field has been subtracted from each atom, the temperature is calculated by the formula KE = (dim*N - dim*Nx*Ny*Nz) k T/2, where KE = total kinetic energy of the group of atoms (sum of 1/2 m v^2), dim = 2 or 3 = dimensionality of the simulation, N = number of atoms in the group, k = Boltzmann constant, and T = temperature. The dim*Nx*Ny*Nz term are degrees of freedom subtracted to adjust for the removal of the center-of-mass velocity in each of Nx*Ny*Nz bins, as discussed in the (Evans) paper.

If the *out* keyword is used with a *tensor* value, which is the
default, a kinetic energy tensor, stored as a 6-element vector, is
also calculated by this compute for use in the computation of a
pressure tensor. The formula for the components of the tensor is the
same as the above formula, except that v^2 is replaced by vx*vy for
the xy component, etc. The 6 components of the vector are ordered xx,
yy, zz, xy, xz, yz.

If the *out* keyword is used with a *bin* value, the count of atoms
and computed temperature for each bin are stored for output, as an
array of values, as described below. The temperature of each bin is
calculated as described above, where the bias velocity is subtracted
and only the remaining thermal velocity of atoms in the bin
contributes to the temperature. See the note below for how the
temperature is normalized by the degrees-of-freedom of atoms in the
bin.

The number of atoms contributing to the temperature is assumed to be
constant for the duration of the run; use the *dynamic* option of the
compute_modify command if this is not the case.

The removal of the spatially-averaged velocity field by this fix is essentially computing the temperature after a “bias” has been removed from the velocity of the atoms. If this compute is used with a fix command that performs thermostatting then this bias will be subtracted from each atom, thermostatting of the remaining thermal velocity will be performed, and the bias will be added back in. Thermostatting fixes that work in this way include fix nvt, fix temp/rescale, fix temp/berendsen, and fix langevin.

This compute subtracts out degrees-of-freedom due to fixes that
constrain molecular motion, such as fix shake and
fix rigid. 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
*extra* option of the compute_modify command.

Note

When using the *out* keyword with a value of *bin*, the
calculated temperature for each bin does not include the
degrees-of-freedom adjustment described in the preceding paragraph,
for fixes that constrain molecular motion. It does include the
adjustment due to the *extra* option, which is applied to each bin.

See the Howto thermostat doc page for a discussion of different ways to compute temperature and perform thermostatting. Using this compute in conjunction with a thermostatting fix, as explained there, will effectively implement a profile-unbiased thermostat (PUT), as described in (Evans).

## Output info

This compute calculates a global scalar (the temperature). Depending
on the setting of the *out* keyword, it also calculates a global
vector or array. For *out* = *tensor*, it calculates a vector of
length 6 (KE tensor), which can be accessed by indices 1-6. For *out*
= *bin* it calculates a global array which has 2 columns and N rows,
where N is the number of bins. The first column contains the number
of atoms in that bin. The second contains the temperature of that
bin, calculated as described above. The ordering of rows in the array
is as follows. Bins in x vary fastest, then y, then z. Thus for a
10x10x10 3d array of bins, there will be 1000 rows. The bin with
indices ix,iy,iz = 2,3,4 would map to row M = (iz-1)*10*10 + (iy-1)*10
+ ix = 322, where the rows are numbered from 1 to 1000 and the bin
indices are numbered from 1 to 10 in each dimension.

These values can be used by any command that uses global scalar or vector or array values from a compute as input. See the Howto output doc page for an overview of LAMMPS output options.

The scalar value calculated by this compute is “intensive”. The vector values are “extensive”. The array values are “intensive”.

The scalar value will be in temperature units. The vector values will be in energy units. The first column of array values are counts; the values in the second column will be in temperature units.

## Restrictions

You should not use too large a velocity-binning grid, especially in 3d. In the current implementation, the binned velocity averages are summed across all processors, so this will be inefficient if the grid is too large, and the operation is performed every timestep, as it will be for most thermostats.

## Default

The option default is out = tensor.

**(Evans)** Evans and Morriss, Phys Rev Lett, 56, 2172-2175 (1986).