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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Published in | Chinese physics C Vol. 47; no. 1; p. 14103 |
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Main Authors | , , , , |
Format | Journal Article |
Language | English |
Published |
01.01.2023
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Online Access | Get full text |
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