Search of Gravitational Waves from GRBs Inner Engine with the AURIGA Detector

Details Search of Gravitational Waves from GRBs Inner Engine with the AURIGA Detector Search of Gravitational Waves from GRBs Inner Engine with the AURIGA Detector

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..312..478c&link_type=abstract

Third Rome Workshop on Gamma-Ray Bursts in the Afterglow Era ASP Conference Series, Volume 312, Proceedings of the conference he

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The origin of GRBs could be explained by identifying their inner engines with NS-BH coalescences, which form, at the end of their evolution, a matter torus surrounding a BH. Once the torus has been formed, a strong emission of gravitational waves, which lasts for several seconds, occurs. The predicted gw signal is a linear chirp with slowly varying frequency in the kHz range. We simulate both the noise of the gw detector AURIGA using its predicted sensitivity (10-22

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