Determining the population properties of spinning black holes

There are at least two formation scenarios consistent with the first gravitational-wave observations of binary black hole mergers. In field models, black hole binaries are formed from stellar binaries that may undergo common envelope evolution. In dynamic models, black hole binaries are formed throu...

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Veröffentlicht in:	Physical review. D 2017-07, Vol.96 (2), Article 023012
Hauptverfasser:	Talbot, Colm, Thrane, Eric
Format:	Artikel
Sprache:	eng
Schlagworte:	Angular momentum Astronomical models Binary stars Black holes Coding Constraint modelling Dynamic models Globular clusters Gravitational waves Misalignment Properties (attributes) Stellar evolution
Online-Zugang:	Volltext
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