期刊
ASTROPHYSICAL JOURNAL
卷 575, 期 2, 页码 L71-L74出版社
IOP PUBLISHING LTD
DOI: 10.1086/342781
关键词
black hole physics; gamma rays : bursts; gamma rays : theory; gravitational waves
A torus around a stellar-mass Kerr black hole can emit about 10% of the spin energy of a black hole in gravitational radiation, which is potentially associated with a gamma-ray burst (GRB). Wide tori may develop buckling modes by the Papaloizou-Pringle instability and gravitational radiation-reaction forces in the Burke-Thorne approximation. Gravitational-wave experiments may discover these emissions in a fraction of nearby supernovae. This provides a test for Kerr black holes and for GRB inner engines by a comparison with the deredshifted durations of long GRBs.
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