Practical guide to GW calculations: Difference between revisions

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__TOC__
Available as of VASP.5.X. For details on the implementation and use of the ''GW'' routines we recommend the papers by Shishkin ''et al.''<ref name="shishkin-PRB74"/><ref name="shishkin-PRB75"/><ref name="shishkin-PRL99"/> and Fuchs ''et al.''<ref name="fuchs-PRB76"/>  
Available as of VASP.5.X. For details on the implementation and use of the ''GW'' routines we recommend the papers by Shishkin ''et al.''<ref name="shishkin-PRB74"/><ref name="shishkin-PRB75"/><ref name="shishkin-PRL99"/> and Fuchs ''et al.''<ref name="fuchs-PRB76"/>  


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* [[GW recipes#scgw|GW and scGW calculations]]: selfconsistent ''GW'' ({{TAG|ALGO}}=GW or {{TAG|ALGO}}=scGW)
* [[GW recipes#scgw|GW and scGW calculations]]: selfconsistent ''GW'' ({{TAG|ALGO}}=GW or {{TAG|ALGO}}=scGW)
* [[DM calculations with GW routines]]: Determination of the frequency dependent dielectric matrix (DM) using the ''GW'' routines
* [[DM calculations with GW routines]]: Determination of the frequency dependent dielectric matrix (DM) using the ''GW'' routines
<span id="GWR>
== Large systems ==
As of version 6, an additional 'R' can be added to the GW {{TAG|ALGO}} tags, ''i.e.'' {{TAG|ALGO}}=G0W0R, GW0R, scGW0R, GWR or scGWR to select the cubic scaling GW algorithms as described by Liu ''et. al.''<ref name="liu"/>
</span>


== Related Tags and Sections ==
== Related Tags and Sections ==
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* {{TAG|LSELFENERGY}}: the frequency dependent self energy
* {{TAG|LSELFENERGY}}: the frequency dependent self energy
* {{TAG|LWAVE}}: selfconsistent ''GW''
* {{TAG|LWAVE}}: selfconsistent ''GW''
* {{TAG|NOMEGAPAR}}: frequency grid parallelization
* {{TAG|NTAUPAR}}: time grid parallelization


{{sc|GW calculations|Examples|Examples that use this tag}}
{{sc|GW calculations|Examples|Examples that use this tag}}
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<ref name="shishkin-PRL99">[http://link.aps.org/doi/10.1103/PhysRevLett.99.246403 M. Shishkin, M. Marsman, and G. Kresse, Phys. Rev. Lett. 99, 246403 (2007).]</ref>
<ref name="shishkin-PRL99">[http://link.aps.org/doi/10.1103/PhysRevLett.99.246403 M. Shishkin, M. Marsman, and G. Kresse, Phys. Rev. Lett. 99, 246403 (2007).]</ref>
<ref name="fuchs-PRB76">[http://link.aps.org/doi/10.1103/PhysRevB.76.115109 F. Fuchs, J. Furthmüller, F. Bechstedt, M. Shishkin, and G. Kresse, Phys. Rev. B 76, 115109 (2007).]</ref>
<ref name="fuchs-PRB76">[http://link.aps.org/doi/10.1103/PhysRevB.76.115109 F. Fuchs, J. Furthmüller, F. Bechstedt, M. Shishkin, and G. Kresse, Phys. Rev. B 76, 115109 (2007).]</ref>
<ref name="liu">[http://journals.aps.org/prb/abstract/10.1103/PhysRevB.94.165109 P. Liu, M. Kaltak, J. Klimes and G. Kresse, Phys. Rev. B 94, 165109 (2016).]</ref>
</references>
</references>
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Revision as of 13:48, 21 September 2017

Available as of VASP.5.X. For details on the implementation and use of the GW routines we recommend the papers by Shishkin et al.[1][2][3] and Fuchs et al.[4]

Recipes

Large systems

As of version 6, an additional 'R' can be added to the GW ALGO tags, i.e. ALGO=G0W0R, GW0R, scGW0R, GWR or scGWR to select the cubic scaling GW algorithms as described by Liu et. al.[5]

Related Tags and Sections

Examples that use this tag

References


Contents