The dynamics of binary neutron star mergers and GW170817

David Radice, Sebastiano Bernuzzi, Albino Perego

Research output: Contribution to journalReview articlepeer-review

2 Scopus citations

Abstract

With the first observation of a binary neutron star merger through gravitational waves and light, GW170817, compact binary mergers have now taken the center stage in nuclear astrophysics. They are thought to be one of the main astrophysical sites of production of r-process elements, and merger observations have become a fundamental tool to constrain the properties of matter. Here, we review our current understanding of the dynamics of neutron star mergers in general and of GW170817 in particular.We discuss the physical processes governing the inspiral, merger, and postmerger evolution, and we highlight the connections between these processes, the dynamics, and the multimessenger observables. Finally, we discuss open questions and issues in the field and the need to address them through a combination of better theoretical models and new observations.

Original languageEnglish (US)
Pages (from-to)95-119
Number of pages25
JournalAnnual Review of Nuclear and Particle Science
Volume70
DOIs
StatePublished - Oct 19 2020

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics

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