A calorimetric test for Kerr black holes in gamma-ray bursts

被引：16

作者：

van Putten, MHPM ^{[1
]}

机构：

[1] MIT, Cambridge, MA 02139 USA

来源：

ASTROPHYSICAL JOURNAL | 2001年 / 562卷 / 01期

基金：

美国国家航空航天局;

关键词：

black hole physics; gamma rays : bursts; gamma rays : theory; gravitational waves;

D O I：

10.1086/338120

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Cosmological gamma-ray bursts are potentially associated with systems harboring a rotating black hole. Calorimetry on yet "unseen" emissions in gravitational waves from a surrounding torus may provide a measure for its rotational energy. We introduce a compactness parameter alpha = 2 pi integralf dE for the fluence E and frequency f in gravitational waves. For black hole-torus systems, alpha similar or equal to 2 pi Ef similar or equal to 0.005-0.05 may exceed the upper bound alpha = 0.005 for rapidly rotating neutron stars. A duration in gravitational radiation consistent with the redshift-corrected durations of the BATSE catalog defines an association with long gamma-ray bursts. This promises to be a new test for Kerr black holes as objects in nature.

引用

页码：L51 / L54

页数：4

共 44 条

[41] Calorimetry of gamma-ray bursts: Echoes in gravitational waves [J].