Analysis of gamma-ray burst duration distribution using mixtures of skewed distributions
arXiv:1506.07801 · doi:10.1093/mnras/stw429
Abstract
Two classes of GRBs have been confidently identified thus far and are prescribed to different physical scenarios -- NS-NS or NS-BH mergers, and collapse of massive stars, for short and long GRBs, respectively. A third, intermediate in duration class, was suggested to be present in previous catalogs, such as BATSE and , based on statistical tests regarding a mixture of two or three log-normal distributions of . However, this might possibly not be an adequate model. This paper investigates whether the distributions of from BATSE, , and are described better by a mixture of skewed distributions rather than standard Gaussians. Mixtures of standard normal, skew-normal, sinh-arcsinh and alpha-skew-normal distributions are fitted using a maximum likelihood method. The preferred model is chosen based on the Akaike information criterion. It is found that mixtures of two skew-normal or two sinh-arcsinh distributions are more likely to describe the observed duration distribution of than a mixture of three standard Gaussians, and that mixtures of two sinh-arcsinh or two skew-normal distributions are models competing with the conventional three-Gaussian in the case of BATSE and . Based on statistical reasoning, existence of a third (intermediate) class of GRBs in data is rejected, and it is shown that other phenomenological models may describe the observed , BATSE, and duration distributions at least as well as a mixture of standard normal distributions.
9 pages, 7 figures, 3 tables; matches the version accepted by MNRAS. arXiv admin note: text overlap with arXiv:1602.02363
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