Type I gamma-ray bursts: Constraints from Monte Carlo simulations

Details Type I gamma-ray bursts: Constraints from Monte Carlo simulations Type I gamma-ray bursts: Constraints from Monte Carlo simulations

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1133..118v&link_type=abstract

GAMMA-RAY BURST: Sixth Huntsville Symposium. AIP Conference Proceedings, Volume 1133, pp. 118-120 (2009).

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Gamma-Ray Sources, Gamma-Ray Bursts, Applications Of Monte Carlo Methods, X-Ray Sources, X-Ray Bursts

Scientific paper

In this analysis we attempt to constrain various facets of the theoretical framework that gives rise to Type I (compact merger) gamma-ray bursts (GRBs) utilizing Monte Carlo simulations. We are interested in testing, specifically, the luminosity function, rate, merger timescale distribution, and host galaxy type and offset of Type I GRBs with one comprehensive Monte Carlo code. The results from these simulations can then be compared to current observations, with consistency being tested from various constraints including the 1D luminosity and redshift distribution, 2D L-z distribution, Swift and BATSE logN(>P)-logP distribution, and host galaxy type and offset data.

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