Formation of double compact objects

V. Kalogera*, K. Belczynski, C. Kim, R. O'Shaughnessy, B. Willems

*Corresponding author for this work

Research output: Contribution to journalReview articlepeer-review

115 Scopus citations

Abstract

Current observations of double neutron stars provide us with a wealth of information that we can use to investigate their evolutionary history and the physical conditions of neutron star formation. Understanding this history and formation conditions further allow us to make theoretical predictions for the formation of other double compact objects with one or two black hole (BH) components and assess the detectability of such systems by ground-based gravitational-wave (GW) interferometers. In this paper we summarize our group's body of work in the past few years and we place our conclusions and current understanding in the framework of other work in this area of astrophysical research.

Original languageEnglish (US)
Pages (from-to)75-108
Number of pages34
JournalPhysics Reports
Volume442
Issue number1-6
DOIs
StatePublished - Apr 2007

Keywords

  • Binaries
  • Black holes
  • Gravitational waves
  • Neutron stars
  • Pulsars
  • Supernovae

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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