PIRSA:13040081

Video URL

https://pirsa.org/13040081

Shake, Rattle and Explode: Short GRBs and the Electromagnetic Counterparts of Gravitational Wave Sources

Berger, E. (2013). Shake, Rattle and Explode: Short GRBs and the Electromagnetic Counterparts of Gravitational Wave Sources. Perimeter Institute for Theoretical Physics. https://pirsa.org/13040081

Berger, Edo. Shake, Rattle and Explode: Short GRBs and the Electromagnetic Counterparts of Gravitational Wave Sources. Perimeter Institute for Theoretical Physics, Apr. 02, 2013, https://pirsa.org/13040081 

          @misc{ scivideos_PIRSA:13040081,
            doi = {10.48660/13040081},
            url = {https://pirsa.org/13040081},
            author = {Berger, Edo},
            keywords = {Cosmology, Strong Gravity},
            language = {en},
            title = {Shake, Rattle and Explode: Short GRBs and the Electromagnetic Counterparts of Gravitational Wave Sources},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2013},
            month = {apr},
            note = {PIRSA:13040081 see, \url{https://scivideos.org/pirsa/13040081}}
          }

Edo Berger Harvard University

Talk numberPIRSA:13040081
DOI10.48660/13040081
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

The bimodality of gamma-ray burst (GRB) durations points to distinct progenitor classes for the long- and short-duration GRBs. While the progenitors of long-duration GRBs are now known to be massive stars, the progenitors of short-duration GRBs remain unidentified. In this talk I will discuss the discovery of short GRB afterglow and their host galaxies, detailed studies of their environments from parsec to galactic scales, and studies of their energetics and beaming. Taken together, these observations point to the coalescence of NS-NS/NS-BH binaries as the most likely progenitors. With the upcoming Advanced LIGO/VIRGO gravitational wave detectors it is therefore possible that short GRBs will be the first detected sources, and I will discuss various approaches to making this connection between gravitational wave and electromagnetic sources.