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Gravitational waves and gamma-ray bursts

Published online by Cambridge University Press:  05 September 2012

Alessandra Corsi
Alessandra Corsi
Affiliation:
LIGO laboratory, California Institute of Technology MS 100-36, Pasadena, CA 91125 (USA) email: corsi@caltech.edu
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Abstract

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Gamma-Ray Bursts are likely associated with a catastrophic energy release in stellar mass objects. Electromagnetic observations provide important, but indirect information on the progenitor. On the other hand, gravitational waves emitted from the central source, carry direct information on its nature. In this context, I give an overview of the multi-messenger study of gamma-ray bursts that can be carried out by using electromagnetic and gravitational wave observations. I also underline the importance of joint electromagnetic and gravitational wave searches, in the absence of a gamma-ray trigger. Finally, I discuss how multi-messenger observations may probe alternative gamma-ray burst progenitor models, such as the magnetar scenario.

Keywords

gamma rays: burstsgravitational wavesstars: neutronsupernovae: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 142 - 149
Copyright
Copyright © International Astronomical Union 2012

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