期刊
ASTROPHYSICAL JOURNAL
卷 552, 期 1, 页码 L31-L34出版社
IOP PUBLISHING LTD
DOI: 10.1086/320253
关键词
black hole physics; gamma rays : bursts; gamma rays : theory
We analyze the temporal evolution of accretion onto rotating black holes subject to large-scale magnetic torques. Wind torques alone drive a disk toward collapse in a finite time similar to E-ff(k)/E-B, where t(ff) is the initial free-fall time and E-k/E-B is the ratio of kinetic energy to poloidal magnetic energy. Additional spin-up torques from a rapidly rotating black hole can arrest the disk's inflow. We associate short/long gamma-ray bursts with hyperaccretion/suspended-accretion onto slowly/rapidly spinning black holes. This model predicts afterglow emission from short bursts and may be tested by HETE-2.
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