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- W3104564161 abstract "Abstract Inasmuch as the hydrostatic structure of the interior of neutron stars uniquely depends on the equation of state (EOS), the inverse constraints on EOS from astrophysical observations have been an important method for revealing the properties of high density matter. Currently, most EOS for neutron star matter are given in tabular form, but these numerical tables can have quite different resolution. To guarantee both the accuracy and efficiency in computing the Tolman-Oppenheimer-Volkoff equations, a concise standard for generating EOS tables with suitable resolution is investigated. It is shown that EOS tables with 50 points logarithmic-uniformly distributed in the supra-nuclear density segment [ <?CDATA $ rho_{0}, 10 rho_{0} $?> ], where <?CDATA $ rho_{0} $?> is the nuclear saturation density, correspond to the interpolation induced errors of ~0.02% for the gravitational mass <?CDATA $ M $?> and ~0.2% for the tidal deformability <?CDATA $ Lambda $?> ." @default.
- W3104564161 created "2020-11-23" @default.
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- W3104564161 date "2019-05-01" @default.
- W3104564161 modified "2023-10-18" @default.
- W3104564161 title "Suitable resolution of EOS tables for neutron star investigations" @default.
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- W3104564161 doi "https://doi.org/10.1088/1674-1137/43/5/054108" @default.
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