Anisotropic neutron stars by gravitational decoupling

V. A. Torres-Sánchez, E. Contreras

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

48 Citas (Scopus)

Resumen

In this work we obtain an anisotropic neutron star solution by gravitational decoupling starting from a perfect fluid configuration which has been used to model the compact object PSR J0348+0432. Additionally, we consider the same solution to model the Binary Pulsar SAX J1808.4-3658 and X-ray Binaries Her X-1 and Cen X-3 ones. We study the acceptability conditions and obtain that the MGD-deformed solution obey the same physical requirements as its isotropic counterpart. Finally, we conclude that the most stable solutions, according to the adiabatic index and gravitational cracking criterion, are those with the smallest compactness parameters, namely SAX J1808.4-3658 and Her X-1.

Idioma originalInglés
Número de artículo829
PublicaciónEuropean Physical Journal C
Volumen79
N.º10
DOI
EstadoPublicada - 1 oct. 2019
Publicado de forma externa

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