메뉴 건너뛰기




Volumn 91, Issue 20, 2015, Pages

Pressure dependence of the charge-density-wave and superconducting states in GdTe3, TbTe3, and DyTe3 pressure dependence of the charge-density- ⋯ Zocco, Hamlin, Grube, Chu, Kuo, Fisher, and Maple

Author keywords

[No Author keywords available]

Indexed keywords


EID: 84929603655     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.91.205114     Document Type: Article
Times cited : (109)

References (49)
  • 3
    • 0001726741 scopus 로고
    • PRBMDO 1098-0121
    • C. A. Balseiro and L. M. Falicov, Phys. Rev. B 20, 4457 (1979). PRBMDO 1098-0121 10.1103/PhysRevB.20.4457
    • (1979) Phys. Rev. B , vol.20 , pp. 4457
    • Balseiro, C.A.1    Falicov, L.M.2
  • 13
  • 24
    • 43049105742 scopus 로고    scopus 로고
    • PRBMDO 1098-0121
    • M. D. Johannes and I. I. Mazin, Phys. Rev. B 77, 165135 (2008). PRBMDO 1098-0121 10.1103/PhysRevB.77.165135
    • (2008) Phys. Rev. B , vol.77 , pp. 165135
    • Johannes, M.D.1    Mazin, I.I.2
  • 28
    • 33749081260 scopus 로고    scopus 로고
    • PRBMDO 1098-0121
    • N. Ru and I. R. Fisher, Phys. Rev. B 73, 033101 (2006). PRBMDO 1098-0121 10.1103/PhysRevB.73.033101
    • (2006) Phys. Rev. B , vol.73 , pp. 033101
    • Ru, N.1    Fisher, I.R.2
  • 30
  • 32
    • 48449104214 scopus 로고    scopus 로고
    • PRBMDO 1098-0121
    • N. Ru, J.-H. Chu, and I. R. Fisher, Phys. Rev. B 78, 012410 (2008). PRBMDO 1098-0121 10.1103/PhysRevB.78.012410
    • (2008) Phys. Rev. B , vol.78 , pp. 012410
    • Ru, N.1    Chu, J.-H.2    Fisher, I.R.3
  • 33
    • 84929586434 scopus 로고    scopus 로고
    • Due to difficulties arising from tuning small magnetic fields of the order of 1 Oe, the highest (Equation presented) occurred at fields other than zero, even after oscillating the magnet to zero field, possibly due to an intrinsic offset of the magnet power supply or to remnant fields in the magnet. The values of magnetic field shown in Fig. 2 were corrected by appropriate values of the order of 17 Oe (within an error of (Equation presented)).
    • Due to difficulties arising from tuning small magnetic fields of the order of 1 Oe, the highest (Equation presented) occurred at fields other than zero, even after oscillating the magnet to zero field, possibly due to an intrinsic offset of the magnet power supply or to remnant fields in the magnet. The values of magnetic field shown in Fig. 2 were corrected by appropriate values of the order of 17 Oe (within an error of (Equation presented)).
  • 34
    • 36049060613 scopus 로고
    • PHRVAO 0031-899X
    • E. Helfand and N. R. Werthamer, Phys. Rev. 147, 288 (1966). PHRVAO 0031-899X 10.1103/PhysRev.147.288
    • (1966) Phys. Rev. , vol.147 , pp. 288
    • Helfand, E.1    Werthamer, N.R.2
  • 36
    • 78649711802 scopus 로고    scopus 로고
    • PRBMDO 1098-0121
    • A. Gurevich, Phys. Rev. B 82, 184504 (2010). PRBMDO 1098-0121 10.1103/PhysRevB.82.184504
    • (2010) Phys. Rev. B , vol.82 , pp. 184504
    • Gurevich, A.1
  • 38
    • 0342974886 scopus 로고
    • PHLTAM 0031-9163
    • B. T. Matthias and J. L. Olsen, Phys. Lett. 13, 202 (1964). PHLTAM 0031-9163 10.1016/0031-9163(64)90447-0
    • (1964) Phys. Lett. , vol.13 , pp. 202
    • Matthias, B.T.1    Olsen, J.L.2
  • 41
    • 6144250711 scopus 로고
    • PRLTAO 0031-9007
    • F. P. Bundy and K. J. Dunn, Phys. Rev. Lett. 44, 1623 (1980). PRLTAO 0031-9007 10.1103/PhysRevLett.44.1623
    • (1980) Phys. Rev. Lett. , vol.44 , pp. 1623
    • Bundy, F.P.1    Dunn, K.J.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.