Constraining the Equation of State of Hybrid Stars Using Recent Information from Multidisciplinary Physics

Constraining the Equation of State of Hybrid Stars Using Recent Information from Multidisciplinary Physics

At the ultrahigh densities existing in the core of neutron stars (NSs), it is expected that a phase transition from baryonic to deconfined quark matter may occur. Such a phase transition would affect the underlying equation of state (EoS) as well as the observable astrophysical properties of NSs. Co...

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Bibliographic Details
Main Authors: Swarnim Shirke, Suprovo Ghosh, Debarati Chatterjee
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Neutron stars
Neutron star cores
Gravitational waves
High energy astrophysics
Particle astrophysics
Online Access:https://doi.org/10.3847/1538-4357/acac31

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