Dependence of the tidal deformability of neutron stars on the nuclear equation of state

Within the Bayesian framework, using an explicitly isospin-dependent parametric equation of state (EOS) for the core of neutron stars (NSs), we studied how the NS EOS behaves when we confront it with the tidal deformabilities of canonical NSs with different error and different lower boundaries, and...

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Bibliographic Details
Published inChinese physics C Vol. 47; no. 1; p. 14103
Main Authors Xie 谢, Wen-Jie 文杰, Chen 陈, Jian-Ling 建玲, Ma 马, Zi-Wei 紫微, Guo 郭, Jun-Hua 俊华, Zhu 祝, Long 龙
Format Journal Article
LanguageEnglish
Published 01.01.2023
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