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Volumn 79, Issue 19, 2009, Pages

Anisotropic vibrations in crystalline and amorphous InP

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EID: 66749147316     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.79.195203     Document Type: Article
Times cited : (42)

References (39)
  • 3
    • 0000807186 scopus 로고
    • 10.1103/PhysRevB.14.1514
    • G. Beni and P. M. Platzman, Phys. Rev. B 14, 1514 (1976). 10.1103/PhysRevB.14.1514
    • (1976) Phys. Rev. B , vol.14 , pp. 1514
    • Beni, G.1    Platzman, P.M.2
  • 6
    • 0000246324 scopus 로고
    • 10.1103/PhysRevB.48.585
    • A. I. Frenkel and J. J. Rehr, Phys. Rev. B 48, 585 (1993). 10.1103/PhysRevB.48.585
    • (1993) Phys. Rev. B , vol.48 , pp. 585
    • Frenkel, A.I.1    Rehr, J.J.2
  • 9
  • 12
    • 0000467436 scopus 로고
    • 10.1103/PhysRevB.51.12322
    • A. Filipponi and A. Di Cicco, Phys. Rev. B 51, 12322 (1995). 10.1103/PhysRevB.51.12322
    • (1995) Phys. Rev. B , vol.51 , pp. 12322
    • Filipponi, A.1    Di Cicco, A.2
  • 21
  • 24
    • 66749141317 scopus 로고    scopus 로고
    • note
    • Floating S02 and E0 for each measured temperature gave only a slight variation in the values significantly smaller than the experimental uncertainty, and showed no trend with temperature. Hence, the parameters were fixed to average values, similar to the analysis of Sanson in Ref., yielding S02 =1.00 and E0 =9.2 eV consistent with our previous measurements.
  • 25
    • 66749145973 scopus 로고    scopus 로고
    • note
    • Relating the relative increase Δ REXAFS / REXAFS of the first and second shells to each other or to the relative lattice expansion, (RC - R0) / R0, is far from trivial since REXAFS depends on the crystallographic distance RC and on the relative vibrations perpendicular to the line connecting absorber-backscatterer pair (REXAFS = RC + MSRD /2 R0). The relative lattice expansion, (RC - R0) / R0, is the same for all coordination shells. In contrast, the MSRD may be different for first and second NN shells due to a different correlation in the absorber-backscatter motion, as is indeed observed for MSRD = σ EXAFS 2 [see Fig. 5]. In fact, we have exploited this very difference between REXAFS and RC to obtain information about the MSRD for the first NN shell (see Figs. 6 7). Given the strong correlation between R EXAFS (2) and C3 (2), the large uncertainties of the values, and the dependence of the results on the fitting protocol, no such analysis or physical interpretation is attempted for the second shell.
  • 27
    • 0003060558 scopus 로고
    • 10.1088/0022-3719/12/13/011
    • W. Böhmer and P. Rabe, J. Phys. C 12, 2465 (1979). 10.1088/0022-3719/12/13/011
    • (1979) J. Phys. C , vol.12 , pp. 2465
    • Böhmer, W.1    Rabe, P.2
  • 35
    • 29144453140 scopus 로고
    • 10.1103/PhysRev.145.637
    • P. N. Keating, Phys. Rev. 145, 637 (1966). 10.1103/PhysRev.145.637
    • (1966) Phys. Rev. , vol.145 , pp. 637
    • Keating, P.N.1
  • 36
    • 35949027701 scopus 로고
    • 10.1103/PhysRevB.1.4005
    • R. M. Martin, Phys. Rev. B 1, 4005 (1970). 10.1103/PhysRevB.1.4005
    • (1970) Phys. Rev. B , vol.1 , pp. 4005
    • Martin, R.M.1
  • 37
    • 0004416046 scopus 로고
    • 10.1103/PhysRevB.32.3695
    • A.-B. Chen and A. Sher, Phys. Rev. B 32, 3695 (1985). 10.1103/PhysRevB.32.3695
    • (1985) Phys. Rev. B , vol.32 , pp. 3695
    • Chen, A.-B.1    Sher, A.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.