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. © 2012 International Astronomical Union.

Corsi A., f.L.s.a.V.C., Cuoco, E. (2011). Gravitational waves and gamma-ray bursts [10.1017/S1743921312012835].

Gravitational waves and gamma-ray bursts

Cuoco E.
2011

Abstract

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. © 2012 International Astronomical Union.
2011
Proceedings of the International Astronomical Union
142
149
Corsi A., f.L.s.a.V.C., Cuoco, E. (2011). Gravitational waves and gamma-ray bursts [10.1017/S1743921312012835].
Corsi A., for LIGO scientific and Virgo Collaborations; Cuoco, E.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/998828
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