Many-body dispersion energy: Difference between revisions

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Details of the implementation of the MBD@rsSCS method in VASP are presented in reference {{cite|bucko:jpcm:16}}.
Details of the implementation of the MBD@rsSCS method in VASP are presented in reference {{cite|bucko:jpcm:16}}.
{{NB|mind|This method requires the use of {{TAG|POTCAR}} files from the PAW dataset version 52 or later.}}
{{NB|mind|
{{NB|mind|The input reference data for non-interacting atoms are available only for elements of the first six rows of the periodic table except of the lanthanides. If the system contains other elements, the user has to provide the free-atomic parameters for all atoms in the system via {{TAG|VDW_ALPHA}}, {{TAG|VDW_C6}} and {{TAG|VDW_R0}} (described by the {{TAG|Tkatchenko-Scheffler method}}) defined in the {{TAG|INCAR}} file.}}
*This method requires the use of {{TAG|POTCAR}} files from the PAW dataset version 52 or later.
{{NB|mind|The charge-density dependence of gradients is neglected.}}
*The input reference data for non-interacting atoms are available only for elements of the first six rows of the periodic table except of the lanthanides. If the system contains other elements, the user has to provide the free-atomic parameters for all atoms in the system via {{TAG|VDW_ALPHA}}, {{TAG|VDW_C6}} and {{TAG|VDW_R0}} (described by the {{TAG|Tkatchenko-Scheffler method}}) defined in the {{TAG|INCAR}} file.
{{NB|mind|This method is incompatible with the setting {{TAG|ADDGRID}}{{=}}''.TRUE.''.}}
*The charge-density dependence of gradients is neglected.
{{NB|mind|It is essential that a sufficiently dense FFT grid (controlled via {{TAG|NGXF}}, {{TAG|NGYF}} and {{TAG|NGZF}} ) is used in the {{TAG|Tkatchenko-Scheffler method}} calculation. We strongly recommend to use {{TAG|PREC}}{{=}}''Accurate'' for this type of calculations (in any case, avoid using {{TAG|PREC}}{{=}}''Low''}).}}
*This method is incompatible with the setting {{TAG|ADDGRID}}{{=}}''.TRUE.''.
{{NB|mind|The method sometimes has numerical problems if highly polarizable atoms are located at short distances. In such a case the calculation terminates with an error message ''Error(vdw\_tsscs\_range\_separated\_k): d\_lr(pp)<{{=}}0''. Note that this problem is not caused by a bug, but rather it is due to a limitation of the underlying physical model.}}
*It is essential that a sufficiently dense FFT grid (controlled via {{TAG|NGXF}}, {{TAG|NGYF}} and {{TAG|NGZF}} ) is used in the {{TAG|Tkatchenko-Scheffler method}} calculation. We strongly recommend to use {{TAG|PREC}}{{=}}''Accurate'' for this type of calculations (in any case, avoid using {{TAG|PREC}}{{=}}''Low'').
{{NB|mind|Analytical gradients of the energy are implemented (fore details see reference {{cite|bucko:jpcm:16}}) and hence the atomic and lattice relaxations can be performed.}}
*The method sometimes has numerical problems if highly polarizable atoms are located at short distances. In such a case the calculation terminates with an error message ''Error(vdw\_tsscs\_range\_separated\_k): d\_lr(pp)<{{=}}0''. Note that this problem is not caused by a bug, but rather it is due to a limitation of the underlying physical model.
{{NB|mind|Due to the long-range nature of dispersion interactions, the convergence of energy with respect to the number of k-points should be carefully examined.}}
*Analytical gradients of the energy are implemented (fore details see reference {{cite|bucko:jpcm:16}}) and hence the atomic and lattice relaxations can be performed.
{{NB|mind|A default value for the free-parameter of this method is available only for the PBE ({{TAG|VDW_SR}}{{=}}0.83), PBE0 ({{TAG|VDW_SR}}{{=}}0.85), HSE06 (({{TAG|VDW_SR}}{{=}}0.85)), B3LYP ({{TAG|VDW_SR}}{{=}}0.64), and SCAN ({{TAG|VDW_SR}}{{=}}1.12) functionals. If any other functional is used, the value of {{TAG|VDW_SR}} must be specified in the {{TAG|INCAR}} file.}}
*Due to the long-range nature of dispersion interactions, the convergence of energy with respect to the number of k-points should be carefully examined.
*A default value for the free-parameter of this method is available only for the PBE ({{TAG|VDW_SR}}{{=}}0.83), PBE0 ({{TAG|VDW_SR}}{{=}}0.85), HSE06 ({{TAG|VDW_SR}}{{=}}0.85), B3LYP ({{TAG|VDW_SR}}{{=}}0.64), and SCAN ({{TAG|VDW_SR}}{{=}}1.12) functionals. If any other functional is used, the value of {{TAG|VDW_SR}} must be specified in the {{TAG|INCAR}} file.}}
 
== Related tags and articles ==
== Related tags and articles ==
{{TAG|VDW_ALPHA}},
{{TAG|VDW_ALPHA}},
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[[The_VASP_Manual|Contents]]
 
[[Category:Exchange-correlation functionals]][[Category:van der Waals functionals]][[Category:Theory]]
[[Category:Exchange-correlation functionals]][[Category:van der Waals functionals]][[Category:Theory]]

Latest revision as of 12:02, 20 May 2024

The many-body dispersion energy method (MBD@rsSCS) of Tkatchenko et al.[1][2] is based on the random-phase expression for the correlation energy

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): E_{c}=\int _{{0}}^{{\infty }}{\frac {d\omega }{2\pi }}{\mathrm {Tr}}\left\{{\mathrm {ln}}(1-v\chi _{0}(i\omega ))+v\chi _{0}(i\omega )\right\}

whereby the response function Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): \chi _{0} is approximated by a sum of atomic contributions represented by quantum harmonic oscillators. The expression for the dispersion energy used in the VASP k-space implementation of the MBD@rsSCS method (see reference [3] for details) is as follows:

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): E_{{{\mathrm {disp}}}}=-\int _{{{\mathrm {FBZ}}}}{\frac {d{{\mathbf {k}}}}{v_{{{\mathrm {FBZ}}}}}}\int _{0}^{{\infty }}{{\frac {d\omega }{2\pi }}}\,{{\mathrm {Tr}}}\left\{{\mathrm {ln}}\left({{\mathbf {1}}}-{{\mathbf {A}}}_{{LR}}^{{(0)}}(\omega ){{\mathbf {T}}}_{{LR}}({{\mathbf {k}}})\right)\right\}

where Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): {{\mathbf {A}}}_{{LR}} is the frequency-dependent polarizability matrix and Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): {\mathbf {T}}_{{LR}} is the long-range interaction tensor, which describes the interaction of the screened polarizabilities embedded in the system in a given geometrical arrangement. The components of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): {\mathbf {A}}_{{LR}} are obtained using an atoms-in-molecule approach as employed in the pairwise Tkatchenko-Scheffler method (see references [2][3] for details). The input reference data for non-interacting atoms can be optionally defined via the parameters VDW_ALPHA, VDW_C6, and VDW_R0 (described by the Tkatchenko-Scheffler method). This method has one free parameter (Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): \beta ) that must be adjusted for each exchange-correlation functional. The default value of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): \beta =0.83 corresponds to the PBE functional (GGA=PE). If another functional is used, the value of Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): \beta must be specified via VDW_SR in the INCAR file. The MBD@rsSCS method is invoked by setting IVDW=202. Optionally, the following parameters can be user-defined (the given values are the default ones):

  • VDW_SR=0.83 : scaling parameter Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): \beta
  • LVDWEXPANSION=.FALSE. : writes the two- to six-body contributions to the MBD dispersion energy in the OUTCAR (LVDWEXPANSION=.TRUE.)
  • LSCSGRAD=.TRUE. : compute gradients (or not)
  • VDW_ALPHA, VDW_C6, VDW_R0 : atomic reference (see also Tkatchenko-Scheffler method)
  • ITIM=-1: if set to +1, apply eigenvalue remapping to avoid unphysical cases where the eigenvalues of the matrix

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://www.vasp.at/wiki/restbase/vasp.at/v1/":): {\displaystyle \left(1-\mathbf{A}^{(0)}_{LR}(\omega) {\mathbf{T}}_{LR}({\mathbf{k}})\right) } are non-positive, see reference[4] for details

Details of the implementation of the MBD@rsSCS method in VASP are presented in reference [3].

Mind:
  • This method requires the use of POTCAR files from the PAW dataset version 52 or later.
  • The input reference data for non-interacting atoms are available only for elements of the first six rows of the periodic table except of the lanthanides. If the system contains other elements, the user has to provide the free-atomic parameters for all atoms in the system via VDW_ALPHA, VDW_C6 and VDW_R0 (described by the Tkatchenko-Scheffler method) defined in the INCAR file.
  • The charge-density dependence of gradients is neglected.
  • This method is incompatible with the setting ADDGRID=.TRUE..
  • It is essential that a sufficiently dense FFT grid (controlled via NGXF, NGYF and NGZF ) is used in the Tkatchenko-Scheffler method calculation. We strongly recommend to use PREC=Accurate for this type of calculations (in any case, avoid using PREC=Low).
  • The method sometimes has numerical problems if highly polarizable atoms are located at short distances. In such a case the calculation terminates with an error message Error(vdw\_tsscs\_range\_separated\_k): d\_lr(pp)<=0. Note that this problem is not caused by a bug, but rather it is due to a limitation of the underlying physical model.
  • Analytical gradients of the energy are implemented (fore details see reference [3]) and hence the atomic and lattice relaxations can be performed.
  • Due to the long-range nature of dispersion interactions, the convergence of energy with respect to the number of k-points should be carefully examined.
  • A default value for the free-parameter of this method is available only for the PBE (VDW_SR=0.83), PBE0 (VDW_SR=0.85), HSE06 (VDW_SR=0.85), B3LYP (VDW_SR=0.64), and SCAN (VDW_SR=1.12) functionals. If any other functional is used, the value of VDW_SR must be specified in the INCAR file.

Related tags and articles

VDW_ALPHA, VDW_C6, VDW_R0, VDW_SR, LVDWEXPANSION, LSCSGRAD, IVDW, Tkatchenko-Scheffler method, Self-consistent screening in Tkatchenko-Scheffler method, Tkatchenko-Scheffler method with iterative Hirshfeld partitioning, Many-body dispersion energy with fractionally ionic model for polarizability

References