Constraints from 3B & PVO on the Halo Beaming Model

Details Constraints from 3B & PVO on the Halo Beaming Model Constraints from 3B & PVO on the Halo Beaming Model

Aug 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..384..472l&link_type=abstract

Gamma-ray bursts: 3rd Huntsville symposium. AIP Conference Proceedings, Volume 384, pp. 472-476 (1996).

Computer Science

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

Scientific paper

We make detailed comparisons between the Halo Beaming Model (HBM) and data from the 3rd BATSE catalog, considering both the spatial and intensity distributions. The effects of a luminosity function are also discussed. In the context of this model, we find that the sampling depth of BATSE is ~160 kpc and the burst peak luminosity is ~1040 erg/s. The distinctive anisotropies predicted by HBM are inconsistent with the 3B data at the 2σ level, (i.e., HBM can not be ruled out at the 2σ level). Future observations will be capable of placing more stringent limits. We emphasize that GRB sources born in M31 are almost entirely undetectable by BATSE in this model. We briefly discuss the energy budgets for the bursters and the mechanism of spindown alignment.

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