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Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers

The detection of gravitational waves has brought to light a population of binary black holes that merge within a Hubble time. Multiple formation channels can contribute to this population, making it difficult to definitively associate particular population features with underlying stellar physics. B...

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Detalles Bibliográficos
Principais autores: Sharan Banagiri, Thomas A. Callister, Christian Adamcewicz, Zoheyr Doctor, Vicky Kalogera
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/adf4c6
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