SMASS: Difference between revisions

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{{TAGDEF|SMASS|-3 {{!}} -2 {{!}} -1 {{!}} [real] ≥ 0|-3}}
{{TAGDEF|SMASS|-3 {{!}} -2 {{!}} -1 {{!}} [real] ≥ 0|-3}}


Description: {{TAG|SMASS}} controls the velocities during an ab-initio molecular dynamics run.
Description: {{TAG|SMASS}} controls the velocities during an ab-initio molecular-dynamics run.
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* {{TAG|SMASS}}=-3
* {{TAG|SMASS}}=-3
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:For {{TAG|SMASS}}≥0, a canonical ensemble is simulated using the algorithm of Nosé. The Nosé mass controls the frequency of the temperature oscillations during the simulation.{{cite|nose:jcp:1984}}{{cite|nose:ptp:1991}}{{cite|bylander:prb:1992}} For {{TAG|SMASS}}=0, a Nosé-mass corresponding to period of 40 time steps will be chosen. The Nosé-mass should be set such that the induced temperature fluctuation show approximately the same frequencies as the typical 'phonon'-frequencies for the specific system. For liquids something like 'phonon'-frequencies might be obtained from the spectrum of the velocity auto-correlation function. If the ionic frequencies differ by an order of magnitude from the frequencies of the induced temperature fluctuations, Nosé thermostat and ionic movement might decouple leading to a non canonical ensemble. The frequency of the approximate temperature fluctuations induced by the Nosé-thermostat is written to the {{FILE|OUTCAR}} file.
:For {{TAG|SMASS}}≥0, a canonical ensemble is simulated using the algorithm of Nosé. The Nosé mass controls the frequency of the temperature oscillations during the simulation.{{cite|nose:jcp:1984}}{{cite|nose:ptp:1991}}{{cite|bylander:prb:1992}} For {{TAG|SMASS}}=0, a Nosé-mass corresponding to period of 40 time steps will be chosen. The Nosé-mass should be set such that the induced temperature fluctuation show approximately the same frequencies as the typical 'phonon'-frequencies for the specific system. For liquids something like 'phonon'-frequencies might be obtained from the spectrum of the velocity auto-correlation function. If the ionic frequencies differ by an order of magnitude from the frequencies of the induced temperature fluctuations, Nosé thermostat and ionic movement might decouple leading to a non canonical ensemble. The frequency of the approximate temperature fluctuations induced by the Nosé-thermostat is written to the {{FILE|OUTCAR}} file.


== Related Tags and Sections ==
== Related tags and articles ==
{{TAG|IBRION}},
{{TAG|IBRION}},
{{TAG|POTIM}},
{{TAG|POTIM}},
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[[Category:INCAR]][[Category:Molecular Dynamics]][[Category:Thermostats]]
[[Category:INCAR tag]][[Category:Molecular dynamics]][[Category:Thermostats]]

Revision as of 14:30, 7 April 2022

SMASS = -3 | -2 | -1 | [real] ≥ 0
Default: SMASS = -3 

Description: SMASS controls the velocities during an ab-initio molecular-dynamics run.


For SMASS=-3 a micro canonical ensemble (NVE ensemble) is simulated (constant energy molecular dynamics). The calculated Hellmann-Feynman forces serve as an acceleration acting onto the ions. The total free energy (i.e. free electronic energy + Madelung energy of ions + kinetic energy of ions) is conserved. Mind: This option only works with MDALGO=0 (not with MDALGO=2) and is hence rather considered as obsolete. To calculate an NVE_ensemble we recommend the user to use MDALGO=1 and ANDERSEN_PROB=0.0.
For SMASS=-2 the initial velocities are kept constant. This allows to calculate the energy for a set of different linear dependent positions (for instance frozen phonons, or dimers with varying bond-length).
Mind: if SMASS=-2 the actual steps taken are POTIM×(velocities-read-from-the-POSCAR-file). To avoid ambiguities, set POTIM=1.
In this case the velocities are scaled each NBLOCK step (starting at the first step i.e. MOD(NSTEP,NBLOCK)=1) to the temperature: T=TEBEG+(TEEND-TEBEG)×NSTEP/NSW,
where NSTEP is the current step (starting from 1). This allows a continuous increase or decrease of the kinetic energy. In the intermediate period a micro-canonical ensemble is simulated.
For SMASS≥0, a canonical ensemble is simulated using the algorithm of Nosé. The Nosé mass controls the frequency of the temperature oscillations during the simulation.[1][2][3] For SMASS=0, a Nosé-mass corresponding to period of 40 time steps will be chosen. The Nosé-mass should be set such that the induced temperature fluctuation show approximately the same frequencies as the typical 'phonon'-frequencies for the specific system. For liquids something like 'phonon'-frequencies might be obtained from the spectrum of the velocity auto-correlation function. If the ionic frequencies differ by an order of magnitude from the frequencies of the induced temperature fluctuations, Nosé thermostat and ionic movement might decouple leading to a non canonical ensemble. The frequency of the approximate temperature fluctuations induced by the Nosé-thermostat is written to the OUTCAR file.

Related tags and articles

IBRION, POTIM, NBLOCK, TEBEG, TEEND

Examples that use this tag

References