GRO: Black hole models for gamma ray bursts

Details GRO: Black hole models for gamma ray bursts GRO: Black hole models for gamma ray bursts

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cuny.reptq....s&link_type=abstract

Annual Report, 15 Jul. 1992 - 14 Jul. 1993 Columbia Univ., New York, NY. Astrophysics Lab.

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Applications

Applications Programs (Computers), Astronomical Models, Black Holes (Astronomy), Cosmology, Gamma Ray Bursts, Monte Carlo Method, Dark Matter, Dynamic Characteristics, Halos, Mathematical Models

Scientific paper

This grant deals with the production of gamma-ray bursts (GRB's) close to horizons of black holes (BH's), mainly via accretion of small chunks of matter onto extreme Kerr BH's. In the past year, we laid the ground work for actual calculations close to Kerr BH's. Because of technical reasons, actual work has only started very recently. Following the detailed list of research subprojects as per our original proposal, we have performed research in the following areas: spectrum calculation; burst dynamics; tidal capture and primordial cloud collapse; halo density profile; and capture of other objects.

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