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Volumn 71, Issue 4, 2005, Pages

Observable form of pulses emitted from relativistic collapsing objects

Author keywords

[No Author keywords available]

Indexed keywords

ACCURACY; ANALYTIC METHOD; ARTICLE; COSMOS; DENSITY; GRAVITY; NEUTRINO; PHASE TRANSITION; RADIATION; X RAY ANALYSIS;

EID: 84927768425     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.71.044002     Document Type: Article
Times cited : (10)

References (22)
  • 5
    • 0013466667 scopus 로고
    • P. Meszaros and H. Riffert, Astrophys. J. 327, 712 (1988); H. Riffert and P. Meszaros, Astrophys. J. 325, 207 (1988).
    • (1988) Astrophys. J. , vol.327 , pp. 712
    • Meszaros, P.1    Riffert, H.2
  • 6
    • 0000908478 scopus 로고
    • P. Meszaros and H. Riffert, Astrophys. J. 327, 712 (1988); H. Riffert and P. Meszaros, Astrophys. J. 325, 207 (1988).
    • (1988) Astrophys. J. , vol.325 , pp. 207
    • Riffert, H.1    Meszaros, P.2
  • 14
    • 84927744506 scopus 로고    scopus 로고
    • T. Schaefer, hep-ph/0304281
    • T. Schaefer, hep-ph/0304281.
  • 18
    • 84927744505 scopus 로고    scopus 로고
    • note
    • In the presence of both, forward and backward rays, the integral over the impact parameter l is understood as a sum of two integrals, one over l ∈ [0, lmax] for the forward radiation and another over l ∈ [l T, lmax] for the backward radiation. Thus the integral (68) stands for F(o) = 2π/r02[∫ 0lmax ldlI+(o) + ∫lTlmax ldlI-(o)]. A(16) We shall use this convention for the other similar integrals.


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