Gravitational Waves and GRBs from Tidal Disruption of Stars in the Center of Galaxies

Details Gravitational Waves and GRBs from Tidal Disruption of Stars in the Center of Galaxies Gravitational Waves and GRBs from Tidal Disruption of Stars in the Center of Galaxies

2004-04-12

arxiv.org/abs/gr-qc/0404049v4

Published on GRB 2003 Conference Proceedings by American Institute for Physics (AIP)

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, 2 figures talk at Gamma Ray Burst Symposium - Santa Fe, New Mexico (USA) September 8-12, 2003. There were added four

Scientific paper

10.1063/1.1810826

Recent measurements of the Chandra satellite have shown that a supermassive black hole of $M = 2.6 \times 10^{6} M_{\odot}$ is located in the Galactic Center; it seems probable that, from other observations, this fact is common in the majority of galaxies. On the other hand, GRB explosions are typical phenomenon linked to the galactic dynamics. In the present paper we discuss the possibility that GRBs are tidal disruption of stars by supermassive black holes located in the center of galaxies. This conjecture can be tested by a gravitational wave detector of the class of AURIGA.

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