Constraints on the Mass Accretion Rate of Neutrino-Cooled Disks in Gamma-Ray Bursts
arXiv:0712.4107 · doi:10.1086/527670
Abstract
We present a unified description of all the three known classes of optically thick accretion disks around black holes, namely Shakura-Sunyaev disks, slim disks, and neutrino-dominated accretion flows (NDAFs). It is found that NDAFs have both a maximal and a minimal possible mass accretion rate at their each radius. This may be suggestive of an interpretation for the origin of X-ray flares observed in gamma-ray bursts.
arXiv comment13 pages, 3 figures, accepted by ApJ
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