Abstract
The merger of binary neutron-star systems is among the scientifically richest events in the universe: it involves extremes of matter and gravity, copious emission of gravitational waves, complex microphysics, and electromagnetic pro- cesses that can lead to astrophysical signatures observable at the largest redshifts. We review here the recent progress in understanding the gravitational-wave signal emitted in this process, focussing in particular on its properties during the inspiral and then after the merger. 10.1
Original language | English |
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Title of host publication | The Physics and Astrophysics of Neutron Stars |
Publisher | Springer |
Pages | 575-635 |
Number of pages | 61 |
DOIs | |
Publication status | Published - 2018 |