SMASS: Difference between revisions
No edit summary |
|||
(17 intermediate revisions by 4 users not shown) | |||
Line 1: | Line 1: | ||
{{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. | ||
---- | ---- | ||
* {{TAG|SMASS}}=-3 | * {{TAG|SMASS}}=-3 | ||
:For {{TAG|SMASS}}=-3 a microcanonical 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. {{NB|tip|To calculate an [[NVE ensemble]] we instead recommend to use {{TAGO|MDALGO|1}} and {{TAGO|ANDERSEN_PROB|0.0}}.|:}} | |||
* {{TAG|SMASS}}=-2 | * {{TAG|SMASS}}=-2 | ||
:For {{TAG|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 lengths). | |||
:'''Mind''': if {{TAG|SMASS}}=-2 the actual steps taken are {{TAG|POTIM}}×(velocities-read-from-the-{{FILE|POSCAR}}-file). To avoid ambiguities, set {{TAG|POTIM}}=1. | |||
* {{TAG|SMASS}}=-1 | * {{TAG|SMASS}}=-1 | ||
:In this case the velocities are scaled each {{TAG|NBLOCK}} step (starting at the first step i.e. MOD(NSTEP,{{TAG|NBLOCK}})=1) to the temperature: T={{TAG|TEBEG}}+({{TAG|TEEND}}-{{TAG|TEBEG}})×NSTEP/{{TAG|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. | |||
* {{TAG|SMASS}}≥0 | * {{TAG|SMASS}}≥0 | ||
: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 articles == | |||
[[structure optimization]], | |||
{{TAG|IBRION}}, | |||
{{TAG|POTIM}}, | |||
{{TAG|NBLOCK}}, | |||
{{TAG|TEBEG}}, | |||
{{TAG|TEEND}} | |||
{{sc|SMASS|Examples|Examples that use this tag}} | |||
== References == | |||
<references/> | |||
<noinclude> | |||
---- | ---- | ||
[[Category:INCAR]][[Category: | [[Category:INCAR tag]][[Category:Molecular dynamics]][[Category:Thermostats]] |
Latest revision as of 11:50, 18 October 2024
SMASS = -3 | -2 | -1 | [real] ≥ 0
Default: SMASS = -3
Description: SMASS controls the velocities during an ab-initio molecular-dynamics run.
- SMASS=-3
- For SMASS=-3 a microcanonical 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.
Tip: To calculate an NVE ensemble we instead recommend to use MDALGO = 1
andANDERSEN_PROB = 0.0
.
- SMASS=-2
- 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 lengths).
- Mind: if SMASS=-2 the actual steps taken are POTIM×(velocities-read-from-the-POSCAR-file). To avoid ambiguities, set POTIM=1.
- SMASS=-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.
- SMASS≥0
- 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
structure optimization, IBRION, POTIM, NBLOCK, TEBEG, TEEND
References