Capozziello 2010 检验双星并合产生短暴

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Title:		Short Gamma Ray Bursts as possible electromagnetic counterpart of coalescing binary systems
Authors:		Capozziello, S.; De Laurentis, M.; De Martino, I.; Formisano, M.
Publication:		eprint arXiv:1004.4818
Publication Date:		04/2010
Origin:		ARXIV
Keywords:		Astrophysics - Cosmology and Extragalactic Astrophysics, General Relativity and Quantum Cosmology, High Energy Physics - Theory
Comment:		4 pages, 1 figure
Bibliographic Code:		2010arXiv1004.4818C

Abstract

Coalescing binary systems, consisting of two collapsed objects, are among the most promising sources of high frequency gravitational waves signals detectable, in principle, by ground-based interferometers. Binary systems of Neutron Star or Black Hole/Neutron Star mergers should also give rise to short Gamma Ray Bursts, a subclass of Gamma Ray Bursts. Short-hard-Gamma Ray Bursts might thus provide a powerful way to infer the merger rate of two-collapsed object binaries. Under the hypothesis that most short Gamma Ray Bursts originate from binaries of Neutron Star or Black Hole/Neutron Star mergers, we outline here the possibility to associate short Gamma Ray Bursts as electromagnetic counterpart of coalescing binary systems.

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