메뉴 건너뛰기




Volumn 73, Issue 9, 2006, Pages

Resonance mode in B1g Raman scattering: A way to distinguish between spin-fluctuation and phonon-mediated d-wave superconductivity

Author keywords

[No Author keywords available]

Indexed keywords


EID: 33645289376     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.73.094512     Document Type: Article
Times cited : (30)

References (48)
  • 12
    • 12244279978 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.70.174505
    • A. V. Chubukov and M. R. Norman, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.70.174505 70, 174505 (2004).
    • (2004) Phys. Rev. B , vol.70 , pp. 174505
    • Chubukov, A.V.1    Norman, M.R.2
  • 13
    • 0000776907 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.61.14751
    • See, e.g., M. R. Norman, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.61.14751 61, 14751 (2000).
    • (2000) Phys. Rev. B , vol.61 , pp. 14751
    • Norman, M.R.1
  • 14
    • 29644444104 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.72.104519
    • G. Seibold and M. Grilli, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.72.104519 72, 104519 (2005).
    • (2005) Phys. Rev. B , vol.72 , pp. 104519
    • Seibold, G.1    Grilli, M.2
  • 15
    • 35949004738 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.46.14803
    • See, e.g., P. Monthoux, A. V. Balatsky, and D. Pines, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.46.14803 46, 14803 (1992);
    • (1992) Phys. Rev. B , vol.46 , pp. 14803
    • Monthoux, P.1    Balatsky, A.V.2    Pines, D.3
  • 16
    • 0001236360 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.54.14971
    • N. Bulut and D. J. Scalapino, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.54.14971 54, 14971 (1996);
    • (1996) Phys. Rev. B , vol.54 , pp. 14971
    • Bulut, N.1    Scalapino, D.J.2
  • 18
    • 0000703738 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.29.4976
    • M. V. Klein and S. B. Dierker, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.29.4976 29, 4976 (1984).
    • (1984) Phys. Rev. B , vol.29 , pp. 4976
    • Klein, M.V.1    Dierker, S.B.2
  • 20
    • 0034300226 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.85.3261
    • M. Eschrig and M. R. Norman, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.85.3261 85, 3261 (2000).
    • (2000) Phys. Rev. Lett. , vol.85 , pp. 3261
    • Eschrig, M.1    Norman, M.R.2
  • 21
    • 0009470180 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.41.8798
    • H. Monien and A. Zawadowski, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.41.8798 41, 8798 (1990).
    • (1990) Phys. Rev. B , vol.41 , pp. 8798
    • Monien, H.1    Zawadowski, A.2
  • 23
    • 0037152817 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.89.177004
    • see also R. Zeyher and A. Greco, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.89.177004 89, 177004 (2002).
    • (2002) Phys. Rev. Lett. , vol.89 , pp. 177004
    • Zeyher, R.1    Greco, A.2
  • 32
    • 4243817471 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.66.054516
    • K. C. Hewitt and J. C. Irwin, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.66.054516 66, 054516 (2002)
    • (2002) Phys. Rev. B , vol.66 , pp. 054516
    • Hewitt, K.C.1    Irwin, J.C.2
  • 33
    • 33645318081 scopus 로고    scopus 로고
    • especially Figs. 1 and 2 and Table II.
    • especially Figs. 1 and 2 and Table II.
  • 34
    • 0001696267 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.52.R9867
    • C. Kendziora and A. Rosenberg, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.52.R9867 52, R9867 (1995).
    • (1995) Phys. Rev. B , vol.52 , pp. 9867
    • Kendziora, C.1    Rosenberg, A.2
  • 35
  • 41
    • 0034229238 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.85.1112
    • S. Sugai and T. Hosokawa, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.85.1112 85, 1112 (2000)
    • (2000) Phys. Rev. Lett. , vol.85 , pp. 1112
    • Sugai, S.1    Hosokawa, T.2
  • 42
    • 33645286680 scopus 로고    scopus 로고
    • Fig. 2. The Tc =75 K result was not used because the gap feature was extremely weak.
    • Fig. 2. The Tc =75 K result was not used because the gap feature was extremely weak.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.