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Volumn 60, Issue 8, 1999, Pages

Photon spectrum produced by the late decay of a cosmic neutrino background

Author keywords

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Indexed keywords


EID: 17144385157     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.60.083503     Document Type: Article
Times cited : (32)

References (27)
  • 5
    • 85037183162 scopus 로고    scopus 로고
    • G.G. Raffelt, Stars as Laboratories for Fundamental Physics (University of Chicago Press, Chicago, 1996)
    • Raffelt, G.G.1
  • 13
    • 85037177267 scopus 로고    scopus 로고
    • For a cosmic fluid with equation of state (Formula presented), with w constant, and no spatial curvature, one obtains Eq. (11) with (Formula presented). The relativistic condition (Formula presented) constrains n to be (Formula presented)
    • For a cosmic fluid with equation of state (Formula presented), with w constant, and no spatial curvature, one obtains Eq. (11) with (Formula presented). The relativistic condition (Formula presented) constrains n to be (Formula presented).
  • 26
    • 85037236886 scopus 로고    scopus 로고
    • Formula 361.54 in
    • Formula 361.54 in 14 contains a misprint when (Formula presented) is defined therein. The argument in the logarithm should read (Formula presented).
  • 27
    • 85037227220 scopus 로고    scopus 로고
    • Calculation of the asymptotic forms of (Formula presented) may be a bit tricky for the not initiated. Use of the infinite series expansion 436.01 in
    • Calculation of the asymptotic forms of (Formula presented) may be a bit tricky for the not initiated. Use of the infinite series expansion 436.01 in 14 is quite helpful.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.