forked from lijiext/lammps
341 lines
16 KiB
Plaintext
341 lines
16 KiB
Plaintext
"LAMMPS WWW Site"_lws - "LAMMPS Documentation"_ld - "LAMMPS Commands"_lc :c
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:link(lws,http://lammps.sandia.gov)
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:link(ld,Manual.html)
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:link(lc,Section_commands.html#comm)
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:line
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fix langevin command :h3
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fix langevin/kk command :h3
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[Syntax:]
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fix ID group-ID langevin Tstart Tstop damp seed keyword values ... :pre
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ID, group-ID are documented in "fix"_fix.html command :ulb,l
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langevin = style name of this fix command :l
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Tstart,Tstop = desired temperature at start/end of run (temperature units) :l
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Tstart can be a variable (see below) :l
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damp = damping parameter (time units) :l
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seed = random number seed to use for white noise (positive integer) :l
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zero or more keyword/value pairs may be appended :l
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keyword = {angmom} or {omega} or {scale} or {tally} or {zero} :l
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{angmom} value = {no} or scale
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{no} = do not thermostat rotational degrees of freedom via the angular momentum
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factor = do thermostat rotational degrees of freedom via the angular momentum and apply numeric factor as discussed below
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{gjf} value = {no} or {yes}
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{no} = use standard formulation
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{yes} = use Gronbech-Jensen/Farago formulation
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{omega} value = {no} or {yes}
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{no} = do not thermostat rotational degrees of freedom via the angular velocity
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{yes} = do thermostat rotational degrees of freedom via the angular velocity
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{scale} values = type ratio
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type = atom type (1-N)
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ratio = factor by which to scale the damping coefficient
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{tally} value = {no} or {yes}
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{no} = do not tally the energy added/subtracted to atoms
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{yes} = do tally the energy added/subtracted to atoms
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{zero} value = {no} or {yes}
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{no} = do not set total random force to zero
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{yes} = set total random force to zero :pre
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:ule
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[Examples:]
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fix 3 boundary langevin 1.0 1.0 1000.0 699483
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fix 1 all langevin 1.0 1.1 100.0 48279 scale 3 1.5
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fix 1 all langevin 1.0 1.1 100.0 48279 angmom 3.333 :pre
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[Description:]
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Apply a Langevin thermostat as described in "(Schneider)"_#Schneider
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to a group of atoms which models an interaction with a background
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implicit solvent. Used with "fix nve"_fix_nve.html, this command
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performs Brownian dynamics (BD), since the total force on each atom
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will have the form:
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F = Fc + Ff + Fr
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Ff = - (m / damp) v
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Fr is proportional to sqrt(Kb T m / (dt damp)) :pre
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Fc is the conservative force computed via the usual inter-particle
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interactions ("pair_style"_pair_style.html,
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"bond_style"_bond_style.html, etc).
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The Ff and Fr terms are added by this fix on a per-particle basis.
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See the "pair_style dpd/tstat"_pair_dpd.html command for a
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thermostatting option that adds similar terms on a pairwise basis to
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pairs of interacting particles.
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Ff is a frictional drag or viscous damping term proportional to the
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particle's velocity. The proportionality constant for each atom is
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computed as m/damp, where m is the mass of the particle and damp is
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the damping factor specified by the user.
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Fr is a force due to solvent atoms at a temperature T randomly bumping
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into the particle. As derived from the fluctuation/dissipation
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theorem, its magnitude as shown above is proportional to sqrt(Kb T m /
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dt damp), where Kb is the Boltzmann constant, T is the desired
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temperature, m is the mass of the particle, dt is the timestep size,
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and damp is the damping factor. Random numbers are used to randomize
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the direction and magnitude of this force as described in
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"(Dunweg)"_#Dunweg, where a uniform random number is used (instead of
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a Gaussian random number) for speed.
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Note that unless you use the {omega} or {angmom} keywords, the
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thermostat effect of this fix is applied to only the translational
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degrees of freedom for the particles, which is an important
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consideration for finite-size particles, which have rotational degrees
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of freedom, are being thermostatted. The translational degrees of
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freedom can also have a bias velocity removed from them before
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thermostatting takes place; see the description below.
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IMPORTANT NOTE: Unlike the "fix nvt"_fix_nh.html command which
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performs Nose/Hoover thermostatting AND time integration, this fix
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does NOT perform time integration. It only modifies forces to effect
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thermostatting. Thus you must use a separate time integration fix,
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like "fix nve"_fix_nve.html to actually update the velocities and
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positions of atoms using the modified forces. Likewise, this fix
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should not normally be used on atoms that also have their temperature
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controlled by another fix - e.g. by "fix nvt"_fix_nh.html or "fix
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temp/rescale"_fix_temp_rescale.html commands.
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See "this howto section"_Section_howto.html#howto_16 of the manual for
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a discussion of different ways to compute temperature and perform
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thermostatting.
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The desired temperature at each timestep is a ramped value during the
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run from {Tstart} to {Tstop}.
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{Tstart} can be specified as an equal-style or atom-style
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"variable"_variable.html. In this case, the {Tstop} setting is
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ignored. If the value is a variable, it should be specified as
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v_name, where name is the variable name. In this case, the variable
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will be evaluated each timestep, and its value used to determine the
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target temperature.
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Equal-style variables can specify formulas with various mathematical
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functions, and include "thermo_style"_thermo_style.html command
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keywords for the simulation box parameters and timestep and elapsed
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time. Thus it is easy to specify a time-dependent temperature.
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Atom-style variables can specify the same formulas as equal-style
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variables but can also include per-atom values, such as atom
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coordinates. Thus it is easy to specify a spatially-dependent
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temperature with optional time-dependence as well.
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Like other fixes that perform thermostatting, this fix can be used
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with "compute commands"_compute.html that remove a "bias" from the
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atom velocities. E.g. removing the center-of-mass velocity from a
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group of atoms or removing the x-component of velocity from the
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calculation. This is not done by default, but only if the
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"fix_modify"_fix_modify.html command is used to assign a temperature
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compute to this fix that includes such a bias term. See the doc pages
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for individual "compute commands"_compute.html to determine which ones
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include a bias. In this case, the thermostat works in the following
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manner: bias is removed from each atom, thermostatting is performed on
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the remaining thermal degrees of freedom, and the bias is added back
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in.
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The {damp} parameter is specified in time units and determines how
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rapidly the temperature is relaxed. For example, a value of 100.0
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means to relax the temperature in a timespan of (roughly) 100 time
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units (tau or fmsec or psec - see the "units"_units.html command).
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The damp factor can be thought of as inversely related to the
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viscosity of the solvent. I.e. a small relaxation time implies a
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hi-viscosity solvent and vice versa. See the discussion about gamma
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and viscosity in the documentation for the "fix
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viscous"_fix_viscous.html command for more details.
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The random # {seed} must be a positive integer. A Marsaglia random
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number generator is used. Each processor uses the input seed to
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generate its own unique seed and its own stream of random numbers.
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Thus the dynamics of the system will not be identical on two runs on
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different numbers of processors.
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:line
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The keyword/value option pairs are used in the following ways.
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The keyword {angmom} and {omega} keywords enable thermostatting of
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rotational degrees of freedom in addition to the usual translational
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degrees of freedom. This can only be done for finite-size particles.
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A simulation using atom_style sphere defines an omega for finite-size
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spheres. A simulation using atom_style ellipsoid defines a finite
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size and shape for aspherical particles and an angular momentum.
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The Langevin formulas for thermostatting the rotational degrees of
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freedom are the same as those above, where force is replaced by
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torque, m is replaced by the moment of inertia I, and v is replaced by
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omega (which is derived from the angular momentum in the case of
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aspherical particles).
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The rotational temperature of the particles can be monitored by the
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"compute temp/sphere"_compute_temp_sphere.html and "compute
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temp/asphere"_compute_temp_asphere.html commands with their rotate
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options.
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For the {omega} keyword there is also a scale factor of 10.0/3.0 that
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is applied as a multiplier on the Ff (damping) term in the equation
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above and of sqrt(10.0/3.0) as a multiplier on the Fr term. This does
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not affect the thermostatting behaviour of the Langevin formalism but
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insures that the randomized rotational diffusivity of spherical
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particles is correct.
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For the {angmom} keyword a similar scale factor is needed which is
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10.0/3.0 for spherical particles, but is anisotropic for aspherical
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particles (e.g. ellipsoids). Currently LAMMPS only applies an
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isotropic scale factor, and you can choose its magnitude as the
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specified value of the {angmom} keyword. If your aspherical particles
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are (nearly) spherical than a value of 10.0/3.0 = 3.333 is a good
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choice. If they are highly aspherical, a value of 1.0 is as good a
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choice as any, since the effects on rotational diffusivity of the
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particles will be incorrect regardless. Note that for any reasonable
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scale factor, the thermostatting effect of the {angmom} keyword on the
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rotational temperature of the aspherical particles should still be
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valid.
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The keyword {scale} allows the damp factor to be scaled up or down by
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the specified factor for atoms of that type. This can be useful when
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different atom types have different sizes or masses. It can be used
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multiple times to adjust damp for several atom types. Note that
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specifying a ratio of 2 increases the relaxation time which is
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equivalent to the solvent's viscosity acting on particles with 1/2 the
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diameter. This is the opposite effect of scale factors used by the
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"fix viscous"_fix_viscous.html command, since the damp factor in fix
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{langevin} is inversely related to the gamma factor in fix {viscous}.
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Also note that the damping factor in fix {langevin} includes the
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particle mass in Ff, unlike fix {viscous}. Thus the mass and size of
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different atom types should be accounted for in the choice of ratio
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values.
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The keyword {tally} enables the calculation of the cumulative energy
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added/subtracted to the atoms as they are thermostatted. Effectively
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it is the energy exchanged between the infinite thermal reservoir and
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the particles. As described below, this energy can then be printed
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out or added to the potential energy of the system to monitor energy
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conservation.
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The keyword {zero} can be used to eliminate drift due to the
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thermostat. Because the random forces on different atoms are
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independent, they do not sum exactly to zero. As a result, this fix
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applies a small random force to the entire system, and the
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center-of-mass of the system undergoes a slow random walk. If the
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keyword {zero} is set to {yes}, the total random force is set exactly
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to zero by subtracting off an equal part of it from each atom in the
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group. As a result, the center-of-mass of a system with zero initial
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momentum will not drift over time.
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The keyword {gjf} can be used to run the "Gronbech-Jensen/Farago
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"_#Gronbech-Jensen time-discretization of the Langevin model. As
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described in the papers cited below, the purpose of this method is to
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enable longer timesteps to be used (up to the numerical stability
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limit of the integrator), while still producing the correct Boltzmann
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distribution of atom positions. It is implemented within LAMMPS, by
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changing how the the random force is applied so that it is composed of
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the average of two random forces representing half-contributions from
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the previous and current time intervals.
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In common with all methods based on Verlet integration, the
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discretized velocities generated by this method in conjunction with
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velocity-Verlet time integration are not exactly conjugate to the
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positions. As a result the temperature (computed from the discretized
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velocities) will be systematically lower than the target temperature,
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by a small amount which grows with the timestep. Nonetheless, the
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distribution of atom positions will still be consistent with the
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target temperature.
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As an example of using the {gjf} keyword, for molecules containing C-H
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bonds, configurational properties generated with dt = 2.5 fs and tdamp
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= 100 fs are indistinguishable from dt = 0.5 fs. Because the velocity
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distribution systematically decreases with increasing timestep, the
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method should not be used to generate properties that depend on the
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velocity distribution, such as the velocity autocorrelation function
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(VACF). In this example, the velocity distribution at dt = 2.5fs
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generates an average temperature of 220 K, instead of 300 K.
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:line
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Styles with a {cuda}, {gpu}, {intel}, {kk}, {omp}, or {opt} suffix are
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functionally the same as the corresponding style without the suffix.
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They have been optimized to run faster, depending on your available
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hardware, as discussed in "Section_accelerate"_Section_accelerate.html
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of the manual. The accelerated styles take the same arguments and
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should produce the same results, except for round-off and precision
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issues.
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These accelerated styles are part of the USER-CUDA, GPU, USER-INTEL,
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KOKKOS, USER-OMP and OPT packages, respectively. They are only
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enabled if LAMMPS was built with those packages. See the "Making
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LAMMPS"_Section_start.html#start_3 section for more info.
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You can specify the accelerated styles explicitly in your input script
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by including their suffix, or you can use the "-suffix command-line
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switch"_Section_start.html#start_7 when you invoke LAMMPS, or you can
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use the "suffix"_suffix.html command in your input script.
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See "Section_accelerate"_Section_accelerate.html of the manual for
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more instructions on how to use the accelerated styles effectively.
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:line
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[Restart, fix_modify, output, run start/stop, minimize info:]
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No information about this fix is written to "binary restart
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files"_restart.html. Because the state of the random number generator
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is not saved in restart files, this means you cannot do "exact"
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restarts with this fix, where the simulation continues on the same as
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if no restart had taken place. However, in a statistical sense, a
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restarted simulation should produce the same behavior.
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The "fix_modify"_fix_modify.html {temp} option is supported by this
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fix. You can use it to assign a temperature "compute"_compute.html
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you have defined to this fix which will be used in its thermostatting
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procedure, as described above. For consistency, the group used by
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this fix and by the compute should be the same.
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The "fix_modify"_fix_modify.html {energy} option is supported by this
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fix to add the energy change induced by Langevin thermostatting to the
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system's potential energy as part of "thermodynamic
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output"_thermo_style.html. Note that use of this option requires
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setting the {tally} keyword to {yes}.
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This fix computes a global scalar which can be accessed by various
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"output commands"_Section_howto.html#howto_15. The scalar is the
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cummulative energy change due to this fix. The scalar value
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calculated by this fix is "extensive". Note that calculation of this
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quantity requires setting the {tally} keyword to {yes}.
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This fix can ramp its target temperature over multiple runs, using the
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{start} and {stop} keywords of the "run"_run.html command. See the
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"run"_run.html command for details of how to do this.
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This fix is not invoked during "energy minimization"_minimize.html.
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[Restrictions:] none
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[Related commands:]
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"fix nvt"_fix_nh.html, "fix temp/rescale"_fix_temp_rescale.html, "fix
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viscous"_fix_viscous.html, "fix nvt"_fix_nh.html, "pair_style
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dpd/tstat"_pair_dpd.html
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[Default:]
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The option defaults are angmom = no, omega = no, scale = 1.0 for all
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types, tally = no, zero = no, gjf = no.
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:line
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:link(Dunweg)
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[(Dunweg)] Dunweg and Paul, Int J of Modern Physics C, 2, 817-27 (1991).
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:link(Schneider)
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[(Schneider)] Schneider and Stoll, Phys Rev B, 17, 1302 (1978).
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:link(Gronbech-Jensen)
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[(Gronbech-Jensen)] Gronbech-Jensen and Farago, Mol Phys, 111, 983
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(2013); Gronbech-Jensen, Hayre, and Farago, Comp Phys Comm,
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185, 524 (2014)
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