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024 7 _ |a 10.1103/PhysRevB.84.085144
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041 _ _ |a eng
082 _ _ |a 530
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
336 7 _ |a Journal Article
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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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