GW Calculations on post-transition-metal oxides
DC Field | Value | Language |
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dc.contributor.author | Youngho Kang | - |
dc.contributor.author | Gijae Kang | - |
dc.contributor.author | Ho-Hyun Nahm | - |
dc.contributor.author | Seong-Ho Cho | - |
dc.contributor.author | Young Soo Park | - |
dc.contributor.author | Seungwu Han | - |
dc.date.available | 2015-04-20T06:00:17Z | - |
dc.date.created | 2014-08-11 | - |
dc.date.issued | 2014-04 | - |
dc.identifier.issn | 2469-9950 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/1052 | - |
dc.description.abstract | In order to establish the reliable GW scheme that can be consistently applied to post-transition-metal oxides (post-TMOs), we carry out comprehensive GW calculations on electronic structures of ZnO, Ga2O3, In2O3, and SnO2, the four representative post-TMOs. Various levels of self-consistency (G0W0, GW0, and QPGW0) and different starting functionals (GGA, GGA + U, and hybrid functional) are tested and their influence on the resulting electronic structure is closely analyzed. It is found that the GW0 scheme with GGA + U as the initial functional turns out to give the best agreement with experiment, implying that describing the position of metal-d level precisely in the ground state plays a critical role for the accurate dielectric property and quasiparticle band gap. Nevertheless, the computation on ZnO still suffers from the shallow Zn-d level and we propose a modified approach (GW0+Ud) that additionally considers an effective Hubbard U term during GW0 iterations and thereby significantly improves the band gap. It is also shown that a GGA + U-based GW0(+Ud) scheme produces an accurate energy gap of crystalline InGaZnO4, implying that this can serve as a standard scheme that can be applied to general structures of post-TMOs. © 2014 American Physical Society. | - |
dc.description.uri | 1 | - |
dc.language | 영어 | - |
dc.publisher | AMER PHYSICAL SOC | - |
dc.title | GW Calculations on post-transition-metal oxides | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.wosid | 000335320800003 | - |
dc.identifier.scopusid | 2-s2.0-84899714695 | - |
dc.identifier.rimsid | 227 | ko |
dc.date.tcdate | 2018-10-01 | - |
dc.contributor.affiliatedAuthor | Ho-Hyun Nahm | - |
dc.identifier.doi | 10.1103/PhysRevB.89.165130 | - |
dc.identifier.bibliographicCitation | PHYSICAL REVIEW B, v.89, no.16, pp.165130 | - |
dc.citation.title | PHYSICAL REVIEW B | - |
dc.citation.volume | 89 | - |
dc.citation.number | 16 | - |
dc.citation.startPage | 165130 | - |
dc.date.scptcdate | 2018-10-01 | - |
dc.description.wostc | 9 | - |
dc.description.scptc | 9 | - |
dc.description.journalClass | 1 | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |