Binary Neutron Star Mergers
We review the current status of studies of the coalescence of binary neutron star systems. We begin with a discussion of the formation channels of merging binaries and we discuss the most recent theoretical predictions for merger rates. Next, we turn to the quasi-equilibrium formalisms that are used...
Main Authors: | Joshua A. Faber, Frederic A. Rasio |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2012-07-01
|
Series: | Living Reviews in Relativity |
Subjects: | |
Online Access: | http://www.livingreviews.org/lrr-2012-8 |
Similar Items
-
Post-merger Gravitational-wave Signal from Neutron-star Binaries: A New Look at an Old Problem
by: Konrad Topolski, et al.
Published: (2023-01-01) -
Wide Binaries with White Dwarf or Neutron Star Companions Discovered from Gaia DR3 and LAMOST
by: Xinlin Zhao, et al.
Published: (2024-01-01) -
Neutron Star Binaries Produced by Binary-Driven Hypernovae, Their Mergers, and the Link between Long and Short GRBs
by: Laura M. Becerra, et al.
Published: (2023-07-01) -
Thermal Effects in Binary Neutron Star Mergers
by: Jacob Fields, et al.
Published: (2023-01-01) -
Event Rate of Fast Radio Bursts from Binary Neutron Star Mergers
by: Zhi-Lin Chen, et al.
Published: (2023-01-01)