Statistics
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..307c&link_type=abstract
Acta Astrophys. Sin., Vol. 16, No. 3, p. 307 - 313
Statistics
Gamma-Ray Bursts: Statistics, Gamma-Ray Bursts: Relativistic Beaming, Gamma-Ray Bursts: Cosmology
Scientific paper
Statistical properties of gamma-ray bursts are analyzed assuming that the bursts with non-thermal, rapidly varying spectra are from relativistic beaming if the bursts are cosmological. The model assumes that all of the bursts are standard candles with identical power-law spectra in their initial systems and the directions of beaming are random in the comoving system and the burst rate is assumed to be constant per unit comoving volume per unit comoving cosmological time in a Friedmann universe with Ω = 1 and Λ = 0. The calculated distribution of burst intensities is consistent with that found by the BATSE experiment for the weak events and by PVO for the strong events when the Lorentz factor of beaming is lower than 10 and the exponent of power-law is less than 1.
Che Hai-hong
Lu Fang-jun
Song Liming
Yu Wenfei
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