메뉴 건너뛰기




Volumn 74, Issue 19, 2006, Pages

Charge modulations versus strain waves in resonant x-ray scattering

Author keywords

[No Author keywords available]

Indexed keywords


EID: 33751175206     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.74.195113     Document Type: Article
Times cited : (25)

References (29)
  • 1
    • 33645821085 scopus 로고
    • PHRVAO 0031-899X 10.1103/PhysRev.46.1002
    • E. Wigner, Phys. Rev. PHRVAO 0031-899X 10.1103/PhysRev.46.1002 46, 1002 (1934).
    • (1934) Phys. Rev. , vol.46 , pp. 1002
    • Wigner, E.1
  • 3
    • 33751179766 scopus 로고    scopus 로고
    • In this manuscript the term "Wigner crystal" (WC) will refer to any charge density wave that is driven principally by many-body interactions rather than a Peierls distortion, a density wave in the dilute electron gas driven by long-ranged Coulomb repulsion being just one example.
    • In this manuscript the term "Wigner crystal" (WC) will refer to any charge density wave that is driven principally by many-body interactions rather than a Peierls distortion, a density wave in the dilute electron gas driven by long-ranged Coulomb repulsion being just one example.
  • 10
    • 0000822613 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.62.1033
    • C. W. M. Castleton and M. Altarelli, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.62.1033 62, 1033 (2000).
    • (2000) Phys. Rev. B , vol.62 , pp. 1033
    • Castleton, C.W.M.1    Altarelli, M.2
  • 12
    • 3242718670 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.92.056403
    • S. S. Dhesi, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.92. 056403 92, 056403 (2004).
    • (2004) Phys. Rev. Lett. , vol.92 , pp. 056403
    • Dhesi, S.S.1
  • 14
    • 84860641033 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.92.237204
    • K. J. Thomas, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.92. 237204 92, 237204 (2004).
    • (2004) Phys. Rev. Lett. , vol.92 , pp. 237204
    • Thomas, K.J.1
  • 15
    • 28944440597 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.95.156402
    • C. Schüßler-Langeheine, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.95.156402 95, 156402 (2005).
    • (2005) Phys. Rev. Lett. , vol.95 , pp. 156402
    • Schüßler-Langeheine, C.1
  • 20
    • 36149024213 scopus 로고
    • PHRVAO 0031-899X 10.1103/PhysRev.94.1593
    • L. G. Parratt and C. F. Hempstead, Phys. Rev. PHRVAO 0031-899X 10.1103/PhysRev.94.1593 94, 1593 (1954).
    • (1954) Phys. Rev. , vol.94 , pp. 1593
    • Parratt, L.G.1    Hempstead, C.F.2
  • 21
    • 0026095584 scopus 로고
    • SCIEAS 0036-8075
    • W. A. Hendrickson, Science SCIEAS 0036-8075 254, 51 (1991).
    • (1991) Science , vol.254 , pp. 51
    • Hendrickson, W.A.1
  • 22
    • 33751165609 scopus 로고    scopus 로고
    • v is defined with respect to a reference valence state of the atom. This reference is arbitrary, since the transformation v→v+Δv may be accomodated by the redefinition fR → fR +Δv fD.
    • v is defined with respect to a reference valence state of the atom. This reference is arbitrary, since the transformation v→v+Δv may be accomodated by the redefinition fR → fR +Δv fD.
  • 23
    • 33751190168 scopus 로고    scopus 로고
    • For the sake of illustration it is assumed that N is an integer, i.e., the CDW is commensurate. However, the method also works for an incommensurate CDW.
    • For the sake of illustration it is assumed that N is an integer, i.e., the CDW is commensurate. However, the method also works for an incommensurate CDW.
  • 24
    • 0001089729 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.37.1779
    • M. Blume and D. Gibbs, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.37. 1779 37, 1779 (1988).
    • (1988) Phys. Rev. B , vol.37 , pp. 1779
    • Blume, M.1    Gibbs, D.2
  • 25
    • 33744591933 scopus 로고
    • RMPHAT 0034-6861 10.1103/RevModPhys.36.681
    • B. W. Battermann and H. Cole, Rev. Mod. Phys. RMPHAT 0034-6861 10.1103/RevModPhys.36.681 36, 681 (1964).
    • (1964) Rev. Mod. Phys. , vol.36 , pp. 681
    • Battermann, B.W.1    Cole, H.2
  • 28


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.