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Volumn 54, Issue 12, 1996, Pages 8446-8451

Photoemission spectral weight distribution

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Indexed keywords


EID: 0000795919     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.54.8446     Document Type: Article
Times cited : (78)

References (21)
  • 16
    • 43949153492 scopus 로고
    • the present paper, we have used the Ti 3d and O 2p partial DOS of (Formula presented), because a band-structure calculation has not been done for (Formula presented) to the authors' knowledge. Due to the orthorhombic distortion, the Ti 3d ((Formula presented)) bandwidth of (Formula presented) should be smaller than that of (Formula presented), meaning that the band DOS at (Formula presented), (Formula presented)(0), used in the present analysis has been underestimated and therefore that the quasiparticle weight z derived here gives an upper bound
    • K. Takegahara, J. Electron. Spectrosc. Relat. Phenom. 66, 303 (1994). In the present paper, we have used the Ti 3d and O 2p partial DOS of (Formula presented), because a band-structure calculation has not been done for (Formula presented) to the authors' knowledge. Due to the orthorhombic distortion, the Ti 3d ((Formula presented)) bandwidth of (Formula presented) should be smaller than that of (Formula presented), meaning that the band DOS at (Formula presented), (Formula presented)(0), used in the present analysis has been underestimated and therefore that the quasiparticle weight z derived here gives an upper bound.
    • (1994) J. Electron. Spectrosc. Relat. Phenom. , vol.66 , pp. 303
    • Takegahara, K.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.