Cost of Inferred Nuclear Parameters toward the f-mode Dynamical Tide in Binary Neutron Stars

Gravitational-wave (GW) observations from neutron stars (NSs) in a binary system provide an excellent scenario to constrain the nuclear parameters. The investigation of Pratten et al. has shown that the ignorance of f -mode dynamical tidal correction in the GW waveform model of the binary NS system...

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Autores principales:	Bikram Keshari Pradhan, Tathagata Ghosh, Dhruv Pathak, Debarati Chatterjee
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2024-01-01
Colección:	The Astrophysical Journal
Materias:	Neutron star cores Neutron stars Gravitational waves Stellar oscillations Nuclear physics Gravitational wave astronomy
Acceso en línea:	https://doi.org/10.3847/1538-4357/ad31a8
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