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GRB jet beaming angle statistics

GRB jet beaming angle statistics
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摘要 Existing theory and models suggest that a Type I (merger) GRB should have a larger jet beaming angle than a Type II (collapsar) GRB, but so far no statistical evidence is available to support this suggestion. In this paper, we obtain a sample of 37 beaming angles and calculate the probability that this is true. A correction is also devised to account for the scarcity of Type I GRBs in our sample. The probability is calculated to be 83% without the correction and 71% with it. Existing theory and models suggest that a Type I (merger) GRB should have a larger jet beaming angle than a Type II (collapsar) GRB, but so far no statistical evidence is available to support this suggestion. In this paper, we obtain a sample of 37 beaming angles and calculate the probability that this is true. A correction is also devised to account for the scarcity of Type I GRBs in our sample. The probability is calculated to be 83% without the correction and 71% with it.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2010年第2期142-150,共9页 天文和天体物理学研究(英文版)
基金 supported by the National Natural Science Foundation of China (Grant No. 10873009) the National Basic Research Program of China (973 program, No. 2007CB815404)
关键词 gamma rays: bursts -- ISM: jets and outflows -- methods: statistical gamma rays: bursts -- ISM: jets and outflows -- methods: statistical
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参考文献22

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