forked from lijiext/lammps
142 lines
5.9 KiB
Plaintext
142 lines
5.9 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 gle command :h3
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[Syntax:]
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fix ID id-group gle Ns Tstart Tstop seed Amatrix [noneq Cmatrix] [every stride] :pre
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ID, group-ID are documented in "fix"_fix.html command :ulb,l
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gle = style name of this fix command :l
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Ns = number of additional fictitious momenta :l
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Tstart, Tstop = temperature ramp during the run :l
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Amatrix = file to read the drift matrix A from :l
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seed = random number seed to use for generating noise (positive integer) :l
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zero or more keyword/value pairs may be appended :l
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keyword = {noneq} and/or {every}
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{noneq} Cmatrix = file to read the non-equilibrium covariance matrix from
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{every} stride = apply the GLE once every time steps. Reduces the accuracy
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of the integration of the GLE, but has *no effect* on the accuracy of equilibrium
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sampling. It might change sampling properties when used together with {noneq}.
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:ule
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[Examples:]
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fix 3 boundary gle 6 300 300 31415 smart.A
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fix 1 all gle 6 300 300 31415 qt-300k.A noneq qt-300k.C
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[Description:]
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Apply a Generalized Langevin Equation (GLE) thermostat as described
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in "(Ceriotti)"_#Ceriotti. The formalism allows one to obtain a number
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of different effects ranging from efficient sampling of all
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vibrational modes in the system to inexpensive (approximate)
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modelling of nuclear quantum effects. Contrary to
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"fix langevin"_fix_langevin.html, this fix performs both
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thermostatting and evolution of the Hamiltonian equations of motion, so it
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does not need to be used together with "fix nve"_fix_nve.html.
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Each degree of freedom in the thermostatted group is supplemented
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with Ns additional degrees of freedom s, and the equations of motion
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become
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dq/dt=p/m
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d(p,s)/dt=(F,0) - A(p,s) + B dW/dt
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where F is the physical force, A is the drift matrix (that generalizes
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the friction in Langevin dynamics), B is the diffusion term and dW/dt
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un-correlated Gaussian random forces. The A matrix couples the physical
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(q,p) dynamics with that of the additional degrees of freedom,
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and makes it possible to obtain effectively a history-dependent
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noise and friction kernel.
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The drift matrix should be given as an external file {Afile},
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as a (Ns+1 x Ns+1) matrix in inverse time units. Matrices that are
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optimal for a given application and the system of choice can be
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obtained from "(GLE4MD)"_#GLE4MD.
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Equilibrium sampling a temperature T is obtained by specifiying the
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target value as the {Tstart} and {Tstop} arguments, so that the diffusion
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matrix that gives canonical sampling for a given A is computed automatically.
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However, the GLE framework also allow for non-equilibrium sampling, that
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can be used for instance to model inexpensively zero-point energy
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effects "(Ceriotti2)"_#Ceriotti2. This is achieved specifying the
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{noneq} keyword followed by the name of the file that contains the
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static covariance matrix for the non-equilibrium dynamics.
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Since integrating GLE dynamics can be costly when used together with
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simple potentials, one can use the {every} optional keyword to
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apply the Langevin terms only once every several MD steps, in a
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multiple time-step fashion. This should be used with care when doing
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non-equilibrium sampling, but should have no effect on equilibrium
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averages when using canonical sampling.
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The random number {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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[Restart, fix_modify, output, run start/stop, minimize info:]
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The instantaneous values of the extended variables are written to
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"binary restart files"_restart.html. Because the state of the random
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number generator is not saved in restart files, this means you cannot
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do "exact" restarts with this fix, where the simulation continues on
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the same as if no restart had taken place. However, in a statistical
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sense, a restarted simulation should produce the same behavior.
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Note however that you should use a different seed each time you
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restart, otherwise the same sequence of random numbers will be used
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each time, which might lead to stochastic synchronization and
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subtle artefacts in the sampling.
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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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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.
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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".
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[Restrictions:]
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The GLE thermostat in its current implementation should not be used
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with rigid bodies, SHAKE or RATTLE. It is expected that all the
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thermostatted degrees of freedom are fully flexible, and the sampled
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ensemble will not be correct otherwise.
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This fix is part of the USER-MISC package. It is only enabled if LAMMPS
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was built with that package. See the "Making
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LAMMPS"_Section_start.html#start_3 section for more info.
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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, "fix_gld"_fix_gld.html
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:line
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:link(Ceriotti)
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[(Ceriotti)] Ceriotti, Bussi and Parrinello, J Chem Theory Comput 6,
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1170-80 (2010)
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:link(GLE4MD)
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[(GLE4MD)] "http://epfl-cosmo.github.io/gle4md/"_http://epfl-cosmo.github.io/gle4md/
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:link(Ceriotti2)
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[(Ceriotti2)] Ceriotti, Bussi and Parrinello, Phys Rev Lett 103,
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030603 (2009)
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