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Original paper

Rates of compact object coalescences

Volume: 25, Issue: 1
Published: Feb 17, 2022
Abstract
Gravitational-wave detections are enabling measurements of the rate of coalescences of binaries composed of two compact objects—neutron stars and/or black holes. The coalescence rate of binaries containing neutron stars is further constrained by electromagnetic observations, including Galactic radio binary pulsars and short gamma-ray bursts. Meanwhile, increasingly sophisticated models of compact objects merging through a variety of evolutionary...
Paper Details
Title
Rates of compact object coalescences
Published Date
Feb 17, 2022
Volume
25
Issue
1
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