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Compact Object Mergers in the Gravitational Wave Era

Rosalba Perna

Stony Brook University

The observation of gravitational waves has opened a new, unexplored window onto the Universe. Among the sources of gravitational wave transients,compact objects such as neutron stars (NSs) and black holes (BHs) play the most important role. In this talk, I will focus on the expected gravitational wave signal when two compact objects (NS-NS and NS-BH) in a binary merge. These events are believed to be accompanied by a strong electromagnetic signature in gamma-rays, followed by longer-wavelength radiation. I will discuss what can be learned from the complementary observations of the electromagnetic and the gravitational wave signals during these events.

Date: Mardi, le 12 janvier 2021
Heure: 15:30
Lieu: Université McGill

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