On jets and luminosity function of GRBs associated with supernovae

Details On jets and luminosity function of GRBs associated with supernovae On jets and luminosity function of GRBs associated with supernovae

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..522..241c&link_type=abstract

COSMIC EXPLOSIONS: Tenth Astrophysics Conference. AIP Conference Proceedings, Volume 522, pp. 241-244 (2000).

Astronomy and Astrophysics

Astrophysics

1

Gamma-Ray Sources, Gamma-Ray Bursts, Supernovae, Radiation Mechanisms, Polarization

Scientific paper

If Gamma-ray Bursts (GRBs) are generally associated with supernovae, a relatively wide intrinsic luminosity function is implied. If it is assumed that the intrinsic luminosity function of GRBs is a power-law: φ(L)~L-β, data from the BATSE 4B catalog can be used to constrain slope index β and the dynamic range width Log Lmax/Lmin Using a K-S test comparison with the observational Log N-Log P, we find constraints on the GRB fireball model, GRB jets. We find the acceptable dynamic range for 102

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