better explanations of vector outputs for compute temp commands

This commit is contained in:
Steve Plimpton
2024-08-21 12:46:45 -06:00
parent c299c94ebc
commit 7de2073e8e
16 changed files with 322 additions and 230 deletions

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@ -48,14 +48,18 @@ the group, :math:`N_\mathrm{fix DOFs}` is the number of degrees of
freedom removed by fix commands (see below), :math:`k_B` is the freedom removed by fix commands (see below), :math:`k_B` is the
Boltzmann constant, and :math:`T` is the resulting computed temperature. Boltzmann constant, and :math:`T` is the resulting computed temperature.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the computation of a pressure by this compute for use in the computation of a pressure tensor by the
tensor. The formula for the components of the tensor is the same as the :doc:`compute pressue <compute_pressure>` command. The formula for
above expression for :math:`E_\mathrm{kin}`, except that :math:`v_i^2` is the components of the tensor is the same as the above expression for
replaced by :math:`v_{i,x} v_{i,y}` for the :math:`xy` component, and so on. :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
The six components of the vector are ordered :math:`xx`, :math:`yy`, the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. :math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The number of atoms contributing to the temperature is assumed to be 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 constant for the duration of the run; use the *dynamic* option of the
:doc:`compute_modify <compute_modify>` command if this is not the case. :doc:`compute_modify <compute_modify>` command if this is not the case.
@ -94,16 +98,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global This compute calculates a global scalar (the temperature) and a global
vector of length six (KE tensor), which can be accessed by indices vector of length six (symmetric tensor), which can be accessed by
1--6. These values can be used by any command that uses global scalar indices 1--6. These values can be used by any command that uses
or vector values from a compute as input. See the :doc:`Howto output global scalar or vector values from a compute as input. See the
<Howto_output>` page for an overview of LAMMPS output options. :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -90,6 +90,19 @@ for the :math:`xy` component, and the appropriate elements of the moment of
inertia tensor are used. The six components of the vector are ordered inertia tensor are used. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
A symmetric tensor, stored as a six-element vector, is also calculated
by this compute for use in the computation of a pressure tensor by the
:doc:`compute pressue <compute_pressure>` command. The formula for
the components of the tensor is the same as the above expression for
:math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
the :math:`v_i^2` and :math:`\omega^2` are replaced by :math:`v_x v_y`
and :math:`\omega_x \omega_y` for the :math:`xy` component, and so on.
And the appropriate elements of the moment of inertia tensor are used.
Note that because it lacks the 1/2 factor, these tensor components are
twice those of the traditional kinetic energy tensor. The six
components of the vector are ordered :math:`xx`, :math:`yy`,
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
The number of atoms contributing to the temperature is assumed to be The number of atoms contributing to the temperature is assumed to be
constant for the duration of the run; use the *dynamic/dof* option of constant for the duration of the run; use the *dynamic/dof* option of
the :doc:`compute_modify <compute_modify>` command if this is not the the :doc:`compute_modify <compute_modify>` command if this is not the
@ -131,17 +144,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmertic tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. global scalar or vector values from a compute as input. See the
See the :doc:`Howto output <Howto_output>` page for an overview of LAMMPS :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
output options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -62,12 +62,17 @@ kinetic energy is computed as :math:`\frac12 I \omega^2`, where :math:`I`
is the moment of inertia tensor for the aspherical particle and :math:`\omega` is the moment of inertia tensor for the aspherical particle and :math:`\omega`
is its angular velocity, which is computed from its angular momentum. is its angular velocity, which is computed from its angular momentum.
A kinetic energy tensor, stored as a 6-element vector, is also calculated by A symmetric tensor, stored as a six-element vector, is also calculated
this compute. The formula for the components of the tensor is the same as the by this compute for use in the computation of a pressure tensor by the
above formula, except that :math:`v^2` and :math:`\omega^2` are :doc:`compute pressue <compute_pressure>` command. The formula for
replaced by :math:`v_x v_y` and :math:`\omega_x \omega_y` for the the components of the tensor is the same as the above expression for
math:`xy` component, and the appropriate elements of the inertia tensor are :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
used. The six components of the vector are ordered :math:`xx`, :math:`yy`, the :math:`v_i^2` and :math:`\omega^2` are replaced by :math:`v_x v_y`
and :math:`\omega_x \omega_y` for the :math:`xy` component, and so on.
And the appropriate elements of the moment of inertia tensor are used.
Note that because it lacks the 1/2 factor, these tensor components are
twice those of the traditional kinetic energy tensor. The six
components of the vector are ordered :math:`xx`, :math:`yy`,
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
The number of atoms contributing to the temperature is assumed to be The number of atoms contributing to the temperature is assumed to be
@ -111,17 +116,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. global scalar or vector values from a compute as input. See the
See the :doc:`Howto output <Howto_output>` page for an overview of LAMMPS :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
output options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The scalar value is in temperature :doc:`units <units>`. The vector
The vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -85,12 +85,14 @@ By default, *adof* = 2 or 3 = dimensionality of system, as set via the
:doc:`dimension <dimension>` command, and *cdof* = 0.0. :doc:`dimension <dimension>` command, and *cdof* = 0.0.
This gives the usual formula for temperature. This gives the usual formula for temperature.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the computation of a pressure by this compute. The formula for the components of the tensor is the
tensor. The formula for the components of the tensor is the same as same as the above expression for :math:`E_\mathrm{kin}`, except that
the above formula, except that :math:`v^2` is replaced by the 1/2 factor is NOT included and the :math:`v_i^2` is replaced by
:math:`v_x v_y` for the :math:`xy` component, and so on. :math:`v_{i,x} v_{i,y}` for the :math:`xy` component, and so on. Note
The six components of the vector are ordered :math:`xx`, :math:`yy`, that because it lacks the 1/2 factor, these tensor components are
twice those of the traditional kinetic energy tensor. The six
components of the vector are ordered :math:`xx`, :math:`yy`,
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
Note that the number of atoms contributing to the temperature is Note that the number of atoms contributing to the temperature is
@ -227,10 +229,10 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. global scalar or vector values from a compute as input. See the
See the :doc:`Howto output <Howto_output>` page for an overview of LAMMPS :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
output options. output options.
This compute also optionally calculates a global array, if one or more This compute also optionally calculates a global array, if one or more
@ -245,9 +247,9 @@ page for an overview of LAMMPS output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". The array values are "intensive". vector values are "extensive". The array values are "intensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. The array values values are in energy :doc:`units <units>`. The array values will be
will be in temperature :doc:`units <units>` for the *temp* value, and in in temperature :doc:`units <units>` for the *temp* value, and in
energy :doc:`units <units>` for the *kecom* and *internal* values. energy :doc:`units <units>` for the *kecom* and *internal* values.
Restrictions Restrictions

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@ -44,12 +44,17 @@ where KE is the total kinetic energy of the group of atoms (sum of
simulation, :math:`N` is number of atoms in the group, :math:`k_B` is simulation, :math:`N` is number of atoms in the group, :math:`k_B` is
the Boltzmann constant, and :math:`T` is the absolute temperature. the Boltzmann constant, and :math:`T` is the absolute temperature.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the computation of a pressure by this compute for use in the computation of a pressure tensor by the
tensor. The formula for the components of the tensor is the same as :doc:`compute pressue <compute_pressure>` command. The formula for
the above formula, except that :math:`v^2` is replaced by :math:`v_x v_y` the components of the tensor is the same as the above expression for
for the :math:`xy` component, and so on. The six components of the vector are :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The number of atoms contributing to the temperature is assumed to be 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 constant for the duration of the run; use the *dynamic* option of the
@ -81,17 +86,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. See the global scalar or vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The scalar value is in temperature :doc:`units <units>`. The vector
The vector values will be in energy :doc:`units <units>`. values is in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -67,26 +67,31 @@ the velocity of each core or shell atom used in the KE calculation is
the velocity of the center-of-mass (COM) of the core/shell pair the the velocity of the center-of-mass (COM) of the core/shell pair the
atom is part of. atom is part of.
A kinetic energy tensor, stored as a six-element vector, is also calculated by A symmetric tensor, stored as a six-element vector, is also calculated
this compute for use in the computation of a pressure tensor. The formula for by this compute for use in the computation of a pressure tensor by the
the components of the tensor is the same as the above formula, except that :doc:`compute pressue <compute_pressure>` command. The formula for
:math:`v^2` is replaced by :math:`v_x v_y` for the :math:`xy` component, and so the components of the tensor is the same as the above expression for
on. The six components of the vector are ordered :math:`xx`, :math:`yy`, :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. In contrast to the temperature, the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
the velocity of each core or shell atom is taken individually. :math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The change this fix makes to core/shell atom velocities is essentially The change this fix makes to core/shell atom velocities is essentially
computing the temperature after a "bias" has been removed from the velocity of computing the temperature after a "bias" has been removed from the
the atoms. This "bias" is the velocity of the atom relative to the velocity of the atoms. This "bias" is the velocity of the atom
center-of-mass velocity of the core/shell pair. If this compute is used with a relative to the center-of-mass velocity of the core/shell pair. If
fix command that performs thermostatting then this bias will be subtracted from this compute is used with a fix command that performs thermostatting
each atom, thermostatting of the remaining center-of-mass velocity will be then this bias will be subtracted from each atom, thermostatting of
performed, and the bias will be added back in. This means the thermostatting the remaining center-of-mass velocity will be performed, and the bias
will effectively be performed on the core/shell pairs, instead of on the will be added back in. This means the thermostatting will effectively
individual core and shell atoms. Thermostatting fixes that work in this way be performed on the core/shell pairs, instead of on the individual
include :doc:`fix nvt <fix_nh>`, :doc:`fix temp/rescale <fix_temp_rescale>`, core and shell atoms. Thermostatting fixes that work in this way
:doc:`fix temp/berendsen <fix_temp_berendsen>`, and include :doc:`fix nvt <fix_nh>`, :doc:`fix temp/rescale
:doc:`fix langevin <fix_langevin>`. <fix_temp_rescale>`, :doc:`fix temp/berendsen <fix_temp_berendsen>`,
and :doc:`fix langevin <fix_langevin>`.
The internal energy of core/shell pairs can be calculated by the The internal energy of core/shell pairs can be calculated by the
:doc:`compute temp/chunk <compute_temp_chunk>` command, if chunks are defined :doc:`compute temp/chunk <compute_temp_chunk>` command, if chunks are defined
@ -97,15 +102,15 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmertric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. global scalar or vector values from a compute as input.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -73,12 +73,16 @@ simulation, :math:`N` is the number of atoms in the group, :math:`k_B`
is the Boltzmann constant, and :math:`T` is the temperature. Note that is the Boltzmann constant, and :math:`T` is the temperature. Note that
:math:`v` in the kinetic energy formula is the atom's velocity. :math:`v` in the kinetic energy formula is the atom's velocity.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the computation of a pressure by this compute for use in the computation of a pressure tensor by the
tensor. The formula for the components of the tensor is the same as :doc:`compute pressue <compute_pressure>` command. The formula for
the above formula, except that :math:`v^2` is replaced by :math:`v_x v_y` for the components of the tensor is the same as the above expression for
the :math:`xy` component, and so on. The six components of the vector are :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`. :math:`yz`.
The number of atoms contributing to the temperature is assumed to be The number of atoms contributing to the temperature is assumed to be
@ -128,17 +132,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. See the global scalar or vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The scalar value is in temperature :doc:`units <units>`. The vector
The vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -29,17 +29,20 @@ model, after subtracting out a streaming velocity induced by the
simulation box changing size and/or shape, for example in a simulation box changing size and/or shape, for example in a
non-equilibrium MD (NEMD) simulation. The size/shape change is non-equilibrium MD (NEMD) simulation. The size/shape change is
induced by use of the :doc:`fix deform <fix_deform>` command. A induced by use of the :doc:`fix deform <fix_deform>` command. A
compute of this style is created by the compute of this style is created by the :doc:`fix nvt/sllod/eff
:doc:`fix nvt/sllod/eff <fix_nvt_sllod_eff>` command to compute the thermal <fix_nvt_sllod_eff>` command to compute the thermal temperature of
temperature of atoms for thermostatting purposes. A compute of this atoms for thermostatting purposes. A compute of this style can also
style can also be used by any command that computes a temperature be used by any command that computes a temperature (e.g.,
(e.g., :doc:`thermo_modify <thermo_modify>`, :doc:`fix npt/eff <fix_nh_eff>`). :doc:`thermo_modify <thermo_modify>`, :doc:`fix npt/eff
<fix_nh_eff>`).
The calculation performed by this compute is exactly like that The calculation performed by this compute is exactly like that
described by the :doc:`compute temp/deform <compute_temp_deform>` described by the :doc:`compute temp/deform <compute_temp_deform>`
command, except that the formula for the temperature includes the command, except that the formulas for the temperature (scalar) and
radial electron velocity contributions, as discussed by the :doc:`compute temp/eff <compute_temp_eff>` command. Note that only the diagonal components of the symmetric tensor (vector) include the
translational degrees of freedom for each nuclei or electron are radial electron velocity contributions, as discussed by the
:doc:`compute temp/eff <compute_temp_eff>` command. Note that only
the translational degrees of freedom for each nuclei or electron are
affected by the streaming velocity adjustment. The radial velocity affected by the streaming velocity adjustment. The radial velocity
component of the electrons is not affected. component of the electrons is not affected.
@ -47,17 +50,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. See the global scalar or vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -44,12 +44,16 @@ constant, and :math:`T` = temperature. The calculation of KE excludes the
is 0. The dim parameter is adjusted to give the correct number of is 0. The dim parameter is adjusted to give the correct number of
degrees of freedom. degrees of freedom.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the calculation of a pressure by this compute for use in the computation of a pressure tensor by the
tensor. The formula for the components of the tensor is the same as :doc:`compute pressue <compute_pressure>` command. The formula for
the above formula, except that :math:`v^2` is replaced by :math:`v_x v_y` for the components of the tensor is the same as the above expression for
the :math:`xy` component, and so on. The six components of the vector are :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`. :math:`yz`.
The number of atoms contributing to the temperature is assumed to be The number of atoms contributing to the temperature is assumed to be
@ -88,17 +92,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. global scalar or vector values from a compute as input. See the
See the :doc:`Howto output <Howto_output>` page for an overview of LAMMPS :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
output options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

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@ -97,21 +97,27 @@ center-of-mass velocity across the group in directions where streaming velocity
is *not* subtracted. This can be altered using the *extra* option of the is *not* subtracted. This can be altered using the *extra* option of the
:doc:`compute_modify <compute_modify>` command. :doc:`compute_modify <compute_modify>` command.
If the *out* keyword is used with a *tensor* value, which is the default, If the *out* keyword is used with a *tensor* value, which is the
a kinetic energy tensor, stored as a six-element vector, is also calculated by default, then a symmetric tensor, stored as a six-element vector, is
this compute for use in the computation of a pressure tensor. The formula for also calculated by this compute for use in the computation of a
the components of the tensor is the same as the above formula, except that pressure tensor by the :doc:`compute pressue <compute_pressure>`
:math:`v^2` is replaced by :math:`v_x v_y` for the :math:`xy` component, and command. The formula for the components of the tensor is the same as
so on. The six components of the vector are ordered :math:`xx`, :math:`yy`, the above expression for :math:`E_\mathrm{kin}`, except that the 1/2
factor is NOT included and the :math:`v_i^2` is replaced by
:math:`v_{i,x} v_{i,y}` for the :math:`xy` component, and so on. Note
that because it lacks the 1/2 factor, these tensor components are
twice those of the traditional kinetic energy tensor. The six
components of the vector are ordered :math:`xx`, :math:`yy`,
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
If the *out* keyword is used with a *bin* value, the count of atoms and If the *out* keyword is used with a *bin* value, the count of atoms
computed temperature for each bin are stored for output, as an array of values, and computed temperature for each bin are stored for output, as an
as described below. The temperature of each bin is calculated as described array of values, as described below. The temperature of each bin is
above, where the bias velocity is subtracted and only the remaining thermal calculated as described above, where the bias velocity is subtracted
velocity of atoms in the bin contributes to the temperature. See the note and only the remaining thermal velocity of atoms in the bin
below for how the temperature is normalized by the degrees-of-freedom of atoms contributes to the temperature. See the note below for how the
in the bin. 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 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 constant for the duration of the run; use the *dynamic* option of the
@ -166,16 +172,17 @@ Output info
This compute calculates a global scalar (the temperature). Depending This compute calculates a global scalar (the temperature). Depending
on the setting of the *out* keyword, it also calculates a global on the setting of the *out* keyword, it also calculates a global
vector or array. For *out* = *tensor*, it calculates a vector of 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* length 6 (symmetric tensor), which can be accessed by indices 1--6.
= *bin* it calculates a global array which has 2 columns and :math:`N` rows, For *out* = *bin* it calculates a global array which has 2 columns and
where :math:`N` is the number of bins. The first column contains the number :math:`N` rows, where :math:`N` is the number of bins. The first
of atoms in that bin. The second contains the temperature of that column contains the number of atoms in that bin. The second contains
bin, calculated as described above. The ordering of rows in the array the temperature of that bin, calculated as described above. The
is as follows. Bins in :math:`x` vary fastest, then :math:`y`, then ordering of rows in the array is as follows. Bins in :math:`x` vary
:math:`z`. Thus for a :math:`10\times 10\times 10` 3d array of bins, there fastest, then :math:`y`, then :math:`z`. Thus for a :math:`10\times
will be 1000 rows. The bin with indices :math:`(i_x,i_y,i_z) = (2,3,4)` would 10\times 10` 3d array of bins, there will be 1000 rows. The bin with
map to row :math:`M = 10^2(i_z-1) + 10(i_y-1) + i_x = 322`, where the rows are indices :math:`(i_x,i_y,i_z) = (2,3,4)` would map to row :math:`M =
numbered from 1 to 1000 and the bin indices are numbered from 1 to 10 in each 10^2(i_z-1) + 10(i_y-1) + i_x = 322`, where the rows are numbered from
1 to 1000 and the bin indices are numbered from 1 to 10 in each
dimension. dimension.
These values can be used by any command that uses global scalar or These values can be used by any command that uses global scalar or
@ -186,9 +193,9 @@ options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". The array values are "intensive". vector values are "extensive". The array values are "intensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value us in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. The first column values are in energy :doc:`units <units>`. The first column of array
of array values are counts; the values in the second column will be in values are counts; the values in the second column will be in
temperature :doc:`units <units>`. temperature :doc:`units <units>`.
Restrictions Restrictions
@ -203,7 +210,10 @@ will be for most thermostats.
Related commands Related commands
"""""""""""""""" """"""""""""""""
:doc:`compute temp <compute_temp>`, :doc:`compute temp/ramp <compute_temp_ramp>`, :doc:`compute temp/deform <compute_temp_deform>`, :doc:`compute pressure <compute_pressure>` :doc:`compute temp <compute_temp>`, :doc:`compute temp/ramp
<compute_temp_ramp>`, :doc:`compute temp/deform
<compute_temp_deform>`, :doc:`compute pressure
<compute_pressure>`
Default Default
""""""" """""""

View File

@ -63,12 +63,17 @@ command (e.g., :math:`\AA` for units = real or metal). A
velocity in lattice spacings per unit time). The :doc:`lattice <lattice>` velocity in lattice spacings per unit time). The :doc:`lattice <lattice>`
command must have been previously used to define the lattice spacing. command must have been previously used to define the lattice spacing.
A kinetic energy tensor, stored as a six-element vector, is also calculated by A symmetric tensor, stored as a six-element vector, is also calculated
this compute for use in the computation of a pressure tensor. The formula for by this compute for use in the computation of a pressure tensor by the
the components of the tensor is the same as the above formula, except that :doc:`compute pressue <compute_pressure>` command. The formula for
:math:`v^2` is replaced by :math:`v_x v_y` for the :math:`xy` component, and the components of the tensor is the same as the above expression for
so on. The six components of the vector are ordered :math:`xx`, :math:`yy`, :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The number of atoms contributing to the temperature is assumed to be constant 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 for the duration of the run; use the *dynamic* option of the
@ -100,17 +105,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. See the global scalar or vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""
@ -119,7 +124,10 @@ Restrictions
Related commands Related commands
"""""""""""""""" """"""""""""""""
:doc:`compute temp <compute_temp>`, :doc:`compute temp/profie <compute_temp_profile>`, :doc:`compute temp/deform <compute_temp_deform>`, :doc:`compute pressure <compute_pressure>` :doc:`compute temp <compute_temp>`, :doc:`compute temp/profie
<compute_temp_profile>`, :doc:`compute temp/deform
<compute_temp_deform>`, :doc:`compute pressure
<compute_pressure>`
Default Default
""""""" """""""

View File

@ -49,12 +49,17 @@ where KE = is the total kinetic energy of the group of atoms (sum of
:math:`N` is the number of atoms in both the group and region, :math:`k_B` is :math:`N` is the number of atoms in both the group and region, :math:`k_B` is
the Boltzmann constant, and :math:`T` temperature. the Boltzmann constant, and :math:`T` temperature.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the computation of a pressure by this compute for use in the computation of a pressure tensor by the
tensor. The formula for the components of the tensor is the same as :doc:`compute pressue <compute_pressure>` command. The formula for
the above formula, except that :math:`v^2` is replaced by :math:`v_x v_y` the components of the tensor is the same as the above expression for
for the :math:`xy` component, and so on. The six components of the vector are :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The number of atoms contributing to the temperature is calculated each The number of atoms contributing to the temperature is calculated each
time the temperature is evaluated since it is assumed atoms can time the temperature is evaluated since it is assumed atoms can
@ -78,12 +83,13 @@ will operate only on atoms that are currently in the geometric region.
Unlike other compute styles that calculate temperature, this compute Unlike other compute styles that calculate temperature, this compute
does not subtract out degrees-of-freedom due to fixes that constrain does not subtract out degrees-of-freedom due to fixes that constrain
motion, such as :doc:`fix shake <fix_shake>` and :doc:`fix rigid <fix_rigid>`. This is because those degrees of freedom motion, such as :doc:`fix shake <fix_shake>` and :doc:`fix rigid
(e.g., a constrained bond) could apply to sets of atoms that straddle <fix_rigid>`. This is because those degrees of freedom (e.g., a
the region boundary, and hence the concept is somewhat ill-defined. constrained bond) could apply to sets of atoms that straddle the
If needed the number of subtracted degrees of freedom can be set region boundary, and hence the concept is somewhat ill-defined. If
explicitly using the *extra* option of the needed the number of subtracted degrees of freedom can be set
:doc:`compute_modify <compute_modify>` command. explicitly using the *extra* option of the :doc:`compute_modify
<compute_modify>` command.
See the :doc:`Howto thermostat <Howto_thermostat>` page for a See the :doc:`Howto thermostat <Howto_thermostat>` page for a
discussion of different ways to compute temperature and perform discussion of different ways to compute temperature and perform
@ -93,17 +99,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. See the global scalar or vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The scalar value is in temperature :doc:`units <units>`. The vector
The vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

View File

@ -32,32 +32,33 @@ temperature (e.g., :doc:`thermo_modify <thermo_modify>`).
The operation of this compute is exactly like that described by the The operation of this compute is exactly like that described by the
:doc:`compute temp/region <compute_temp_region>` command, except that :doc:`compute temp/region <compute_temp_region>` command, except that
the formula for the temperature itself includes the radial electron the formulas for the temperature (scalar) and diagonal components of
velocity contributions, as discussed by the the symmetric tensor (vector) include the radial electron velocity
:doc:`compute temp/eff <compute_temp_eff>` command. contributions, as discussed by the :doc:`compute temp/eff
<compute_temp_eff>` command.
Output info Output info
""""""""""" """"""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. See the global scalar or vector values from a compute as input. See the
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""
This compute is part of the EFF package. It is only enabled if This compute is part of the EFF package. It is only enabled if LAMMPS
LAMMPS was built with that package. was built with that package. See the :doc:`Build package
See the :doc:`Build package <Build_package>` page for more info. <Build_package>` page for more info.
Related commands Related commands
"""""""""""""""" """"""""""""""""

View File

@ -43,12 +43,17 @@ where KE is the total kinetic energy of the group of atoms (sum of
:math:`N` is the number of atoms in the group, :math:`k_B` is the Boltzmann :math:`N` is the number of atoms in the group, :math:`k_B` is the Boltzmann
constant, and :math:`T` is the absolute temperature. constant, and :math:`T` is the absolute temperature.
A kinetic energy tensor, stored as a six-element vector, is also calculated by A symmetric tensor, stored as a six-element vector, is also calculated
this compute for use in the computation of a pressure tensor. The formula for by this compute for use in the computation of a pressure tensor by the
the components of the tensor is the same as the above formula, except that :doc:`compute pressue <compute_pressure>` command. The formula for
:math:`v^2` is replaced by :math:`v_x v_y` for the :math:`xy` component, and the components of the tensor is the same as the above expression for
so on. The six components of the vector are ordered :math:`xx`, :math:`yy`, :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The number of atoms contributing to the temperature is assumed to be 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 constant for the duration of the run; use the *dynamic* option of the
@ -80,17 +85,16 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1-6. These values can be used by any command that uses global
vector values from a compute as input. See the scalar or vector values from a compute as input. See the :doc:`Howto
:doc:`Howto output <Howto_output>` page for an overview of LAMMPS output output <Howto_output>` page for an overview of LAMMPS output options.
options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

View File

@ -77,6 +77,18 @@ tensor is the same as the above formulas, except that :math:`v^2` and
vector are ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, vector are ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`,
:math:`xz`, :math:`yz`. :math:`xz`, :math:`yz`.
A symmetric tensor, stored as a six-element vector, is also calculated
by this compute for use in the computation of a pressure tensor by the
:doc:`compute pressue <compute_pressure>` command. The formula for
the components of the tensor is the same as the above expression for
:math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
the :math:`v_i^2` and :math:`\omega^2` are replaced by :math:`v_x v_y`
and :math:`\omega_x \omega_y` for the :math:`xy` component, and so on.
Note that because it lacks the 1/2 factor, these tensor components are
twice those of the traditional kinetic energy tensor. The six
components of the vector are ordered :math:`xx`, :math:`yy`,
:math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`.
The number of atoms contributing to the temperature is assumed to be 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 constant for the duration of the run; use the *dynamic* option of the
:doc:`compute_modify <compute_modify>` command if this is not the case. :doc:`compute_modify <compute_modify>` command if this is not the case.
@ -117,17 +129,17 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global 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. vector of length 6 (symmetric tensor), which can be accessed by
These values can be used by any command that uses global scalar or indices 1--6. These values can be used by any command that uses
vector values from a compute as input. global scalar or vector values from a compute as input. See the
See the :doc:`Howto output <Howto_output>` page for an overview of LAMMPS :doc:`Howto output <Howto_output>` page for an overview of LAMMPS
output options. output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
vector values are "extensive". vector values are "extensive".
The scalar value will be in temperature :doc:`units <units>`. The The scalar value is in temperature :doc:`units <units>`. The vector
vector values will be in energy :doc:`units <units>`. values are in energy :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""

View File

@ -86,12 +86,17 @@ where KE is the total kinetic energy of the group of atoms (sum of
:math:`N` is the number of atoms in the group, :math:`k_B` is the Boltzmann :math:`N` is the number of atoms in the group, :math:`k_B` is the Boltzmann
constant, and :math:`T` is the absolute temperature. constant, and :math:`T` is the absolute temperature.
A kinetic energy tensor, stored as a six-element vector, is also A symmetric tensor, stored as a six-element vector, is also calculated
calculated by this compute for use in the computation of a pressure by this compute for use in the computation of a pressure tensor by the
tensor. The formula for the components of the tensor is the same as :doc:`compute pressue <compute_pressure>` command. The formula for
the above formula, except that :math:`v^2` is replaced by :math:`v_x v_y` for the components of the tensor is the same as the above expression for
the :math:`xy` component, and so on. The six components of the vector are :math:`E_\mathrm{kin}`, except that the 1/2 factor is NOT included and
ordered :math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`, :math:`yz`. the :math:`v_i^2` is replaced by :math:`v_{i,x} v_{i,y}` for the
:math:`xy` component, and so on. Note that because it lacks the 1/2
factor, these tensor components are twice those of the traditional
kinetic energy tensor. The six components of the vector are ordered
:math:`xx`, :math:`yy`, :math:`zz`, :math:`xy`, :math:`xz`,
:math:`yz`.
The number of atoms contributing to the temperature is assumed to be 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 constant for the duration of the run; use the *dynamic* option of the
@ -126,21 +131,21 @@ Output info
""""""""""" """""""""""
This compute calculates a global scalar (the temperature) and a global This compute calculates a global scalar (the temperature) and a global
vector of length 7, which can be accessed by indices 1--7. vector of length 7, which can be accessed by indices 1--7. The first
The first six elements of the vector are the KE tensor, six elements of the vector are those of the symmetric tensor discussed
and the seventh is the cosine-shaped velocity amplitude :math:`V`, above. The seventh is the cosine-shaped velocity amplitude :math:`V`,
which can be used to calculate the reciprocal viscosity, as shown in the example. which can be used to calculate the reciprocal viscosity, as shown in
These values can be used by any command that uses global scalar or the example. These values can be used by any command that uses global
vector values from a compute as input. scalar or vector values from a compute as input. See the :doc:`Howto
See the :doc:`Howto output <Howto_output>` page for an overview of LAMMPS output options. output <Howto_output>` page for an overview of LAMMPS output options.
The scalar value calculated by this compute is "intensive". The The scalar value calculated by this compute is "intensive". The
first six elements of vector values are "extensive", first six elements of vector values are "extensive",
and the seventh element of vector values is "intensive". and the seventh element of vector values is "intensive".
The scalar value will be in temperature :doc:`units <units>`. The scalar value is in temperature :doc:`units <units>`. The first
The first six elements of vector values will be in energy :doc:`units <units>`. six elements of vector values are in energy :doc:`units <units>`. The
The seventh element of vector value will be in velocity :doc:`units <units>`. seventh element of vector value us in velocity :doc:`units <units>`.
Restrictions Restrictions
"""""""""""" """"""""""""