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Volumn 90, Issue 2, 2003, Pages

Berciu and Bhatt Reply

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EID: 84861164486     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.90.029702     Document Type: Article
Times cited : (9)

References (7)
  • 1
    • 11844261853 scopus 로고    scopus 로고
    • C. Timm et al, preceding Comment, Phys. Rev. Lett. 90 029701 (2003).
    • (2003) Phys. Rev. Lett. , vol.90 , pp. 29701
    • Timm, C.1
  • 3
    • 0037179303 scopus 로고    scopus 로고
    • E.J. Singley et al, Phys. Rev. Lett.10.1103/PhysRevLett.87.097203 87, 097203 (2002).
    • (2002) Phys. Rev. Lett. , vol.87 , pp. 97203
    • Singley, E.J.1
  • 4
    • 0002184343 scopus 로고
    • One such possibility is using a Wigner-Seitz instead of a tight-binding scheme for the IB, as done in R.N. Bhatt and T.M. Rice, Phys. Rev. B10.1103/PhysRevB.23.1920 23, 1920 (1981).
    • (1981) Phys. Rev. B , vol.23 , pp. 1920
  • 5
    • 0037091434 scopus 로고    scopus 로고
    • A.L. Chudnovskiy et al, Phys. Rev. B10.1103/PhysRevB.65.165216 65, 165216 (2002).
    • (2002) Phys. Rev. B , vol.65 , pp. 165216
    • Chudnovskiy, A.L.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.