Home > Publications database > GW calculations including spin-orbit coupling: Application to Hg chalcogenides > print |
001 | 16690 | ||
005 | 20230426083027.0 | ||
024 | 7 | _ | |a 10.1103/PhysRevB.84.085144 |2 DOI |
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084 | _ | _ | |2 WoS |a Physics, Condensed Matter |
100 | 1 | _ | |0 P:(DE-HGF)0 |a Sakuma, R. |b 0 |
245 | _ | _ | |a GW calculations including spin-orbit coupling: Application to Hg chalcogenides |
260 | _ | _ | |a College Park, Md. |b APS |c 2011 |
300 | _ | _ | |a 085144 |
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440 | _ | 0 | |0 4919 |a Physical Review B |v 84 |x 1098-0121 |y 8 |
500 | _ | _ | |3 POF3_Assignment on 2016-02-29 |
500 | _ | _ | |a Fruitful discussions with G. Bihlmayer are gratefully acknowledged. This work was supported by "Materials Design through Computics: Complex Correlation and Non-Equilibrium Dynamics,' A Grant in Aid for Scientific Research on Innovative Areas, and the Global Center-of-Excellence program (G-03) of MEXT Japan. We further acknowledge financial support from the Deutsche Forschungsgemeinschaft through the Priority Program 1145. Part of the calculations were performed at the Supercomputer Center of ISSP, Japan. |
520 | _ | _ | |a We present self-energy calculations for Hg chalcogenides (HgX, X = S, Se, and Te) with inverted band structures using an explicit spin-dependent formulation of the GW approximation. Spin-orbit coupling is fully taken into account in calculating the single-particle Green function G and the screened interaction W. We have found, apart from an upward shift of the occupied conductionlike Gamma(6) state by about 0.7 eV, an enhancement of spin-orbit splitting by about 0.1 eV, in good agreement with experiment. This renormalization originates mainly from spin-orbit induced changes in G rather than W, which is affected only little by spin-orbit coupling. |
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773 | 1 | 8 | |a 10.1103/physrevb.84.085144 |b American Physical Society (APS) |d 2011-08-30 |n 8 |p 085144 |3 journal-article |2 Crossref |t Physical Review B |v 84 |y 2011 |x 1098-0121 |
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856 | 7 | _ | |u http://dx.doi.org/10.1103/PhysRevB.84.085144 |
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