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The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters

Gravitational-wave detectors are unveiling a population of binary black hole (BBH) mergers out to redshifts z ≈ 1, and are starting to constrain how the BBH population evolves with redshift. We present predictions for the redshift evolution of the BBH mass and spin distributions for systems originat...

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Bibliografske podrobnosti
Principais autores: Claire S. Ye, Maya Fishbach
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2024-01-01
Serija:The Astrophysical Journal
Teme:
Online dostop:https://doi.org/10.3847/1538-4357/ad3ba8
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