BINARY BLACK HOLES IN DENSE STAR CLUSTERS: EXPLORING THE THEORETICAL UNCERTAINTIES

Recent N-body simulations predict that large numbers of stellar black holes (BHs) could at present remain bound to globular clusters (GCs), and merging BH–BH binaries are produced dynamically in significant numbers. We systematically vary "standard" assumptions made by numerical simulation...

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Detalhes bibliográficos
Principais autores: Chatterjee, Sourav, Rasio, Frederic A., Rodriguez, Carl
Outros Autores: Massachusetts Institute of Technology. Department of Physics
Formato: Artigo
Idioma:en_US
Publicado em: IOP Publishing 2017
Acesso em linha:http://hdl.handle.net/1721.1/109564