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Volumn 110, Issue 8, 1999, Pages 3903-3912

Luminescence spectroscopy of matrix-isolated atomic cadmium

Author keywords

[No Author keywords available]

Indexed keywords

ABSORPTION SPECTROSCOPY; ARGON; ATOMS; CADMIUM; ELECTRON EMISSION; ELECTRON ENERGY LEVELS; ELECTRON RESONANCE; ELECTRON TRANSITIONS; KRYPTON; NEON; SYNCHROTRON RADIATION; XENON;

EID: 0033593717     PISSN: 00219606     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.478244     Document Type: Article
Times cited : (15)

References (29)
  • 8
    • 0040912911 scopus 로고
    • W. W. Duley, Proc. Phys. Soc. London 91, 976 (1967); Nature (London) 210, 264 (1966).
    • (1966) Nature (London) , vol.210 , pp. 264
  • 14
    • 85034561578 scopus 로고    scopus 로고
    • note
    • ZFIT program, Nonlinear Least Squares Analysis of Fluorescence Decay Data, M. Rehorek, H. Otto, W. Rettig, and A. Klock, and modified by P. Gürtler and M. Joppien, last update August 1995.
  • 17
    • 0000070078 scopus 로고
    • 1/2)/(1 - r)), in which r=exp(-θ) and p is the phonon number. Equation (1) is the first term in the expansion of the Wp function, and at low temperatures it approximates the latter very well. The line shape generated with the Wp function, using the S and ℏω terms extracted for the 329 nm emission band recorded at 4.3 K in the Cd/Xe system, was identical to that generated with Eq. (1). The advantage of using Eq. (1) over the Wp function is that it avoids use of the modified Bessel function Ip(x) appearing in the Wp expression, which makes fitting to this formula difficult and unreliable. For a more detailed discussion of these functions, see C. W. Struck and W. H. Fonger, Understanding Luminescence Spectra and Efficiency Using Wp and Related Functions (Springer-Verlag, Berlin, 1991). Chap. 4.
    • (1950) Rhys. Proc. R. Soc. London, Ser. A , vol.204 A , pp. 406
    • Huang, K.1    Rhys, A.2
  • 18
    • 0004114934 scopus 로고
    • Springer-Verlag, Berlin, Chap. 4
    • 1/2)/(1 - r)), in which r=exp(-θ) and p is the phonon number. Equation (1) is the first term in the expansion of the Wp function, and at low temperatures it approximates the latter very well. The line shape generated with the Wp function, using the S and ℏω terms extracted for the 329 nm emission band recorded at 4.3 K in the Cd/Xe system, was identical to that generated with Eq. (1). The advantage of using Eq. (1) over the Wp function is that it avoids use of the modified Bessel function Ip(x) appearing in the Wp expression, which makes fitting to this formula difficult and unreliable. For a more detailed discussion of these functions, see C. W. Struck and W. H. Fonger, Understanding Luminescence Spectra and Efficiency Using Wp and Related Functions (Springer-Verlag, Berlin, 1991). Chap. 4.
    • (1991) Understanding Luminescence Spectra and Efficiency Using Wp and Related Functions
    • Struck, C.W.1    Fonger, W.H.2
  • 20
    • 85034543387 scopus 로고    scopus 로고
    • note
    • m.
  • 23
    • 25744472063 scopus 로고    scopus 로고
    • unpublished results
    • The index of refraction of Ar at 233 nm is 1.32 at 6 K. Those of Kr at 241 and 262 nm are 1.428 and 1,418, respectively (P. Gürtler, unpublished results, 1996).
    • (1996)
    • Gürtler, P.1
  • 27
    • 0346821780 scopus 로고    scopus 로고
    • unpublished results
    • -1 intervenes between the two minima. B. Healy and J. G. McCaffrey, unpublished results, 1998.
    • (1998)
    • Healy, B.1    McCaffrey, J.G.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.