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Volumn 192, Issue 2-3, 1982, Pages 565-574

Time dependence of the recombination luminescence from high-pressure argon, krypton and xenon excited by alpha particles

Author keywords

[No Author keywords available]

Indexed keywords

SCINTILLATION COUNTERS - RESEARCH;

EID: 0020091156     PISSN: 0029554X     EISSN: None     Source Type: Journal    
DOI: 10.1016/0029-554X(82)90874-6     Document Type: Article
Times cited : (53)

References (32)
  • 13
    • 84908745443 scopus 로고    scopus 로고
    • −0.5 for krypton and xenon, respectively, (J.N. Bardsley and M.A. Biondi, Adv. At. Mol. Phys. 6, 1970)2, it is safely considered that all the secondary electrons are thermalized and then recombine with molecular ions via eq. (3).
  • 17
    • 84908715153 scopus 로고    scopus 로고
    • M. Suzuki, to be published.
  • 23
    • 84908760558 scopus 로고    scopus 로고
    • M. Suzuki, J. Ruan(Gen) and S. Kubota, to be published.
  • 24
    • 84908715152 scopus 로고    scopus 로고
    • + states of lifetime τ are produced through the recombination process.
  • 25
    • 84908745442 scopus 로고    scopus 로고
    • f, measured decay curves are safely compared with I(t).
  • 31
    • 84908745441 scopus 로고    scopus 로고
    • Since energy loss due to inelastic scattering is a rapid process compared with the one due to elastic scattering, the thermalization time for secondary electrons is partically the same as that for sub-excitation electrons.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.