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Emergence of Microphysical Bulk Viscosity in Binary Neutron Star Postmerger Dynamics

In nuclear matter in isolated neutron stars, the flavor content (e.g., proton fraction) is subject to weak interactions, establishing flavor ( β -)equilibrium. However, there can be deviations from this equilibrium during the merger of two neutron stars. We study the resulting out-of-equilibrium dyn...

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Principais autores: Elias R. Most, Alexander Haber, Steven P. Harris, Ziyuan Zhang, Mark G. Alford, Jorge Noronha
Format: Artigo
Sprog:Inglês
Udgivet: IOP Publishing 2024-01-01
Serier:The Astrophysical Journal Letters
Fag:
Neutron stars
Nuclear astrophysics
Nuclear physics
Gravitational waves
Online adgang:https://doi.org/10.3847/2041-8213/ad454f
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