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• W2098778873 abstract "Methods are developed for constructing spectral representations of cold (barotropic) neutron-star equations of state. These representations are faithful in the sense that every physical equation of state has a representation of this type and conversely every such representation satisfies the minimal thermodynamic stability criteria required of any physical equation of state. These spectral representations are also efficient, in the sense that only a few spectral coefficients are generally required to represent neutron-star equations of state quiet accurately. This accuracy and efficiency is illustrated by constructing spectral fits to a large collection of ``realistic'' neutron-star equations of state." @default.
• W2098778873 created "2016-06-24" @default.
• W2098778873 creator A5060564143 @default.
• W2098778873 date "2010-11-18" @default.
• W2098778873 modified "2023-10-06" @default.
• W2098778873 title "Spectral representations of neutron-star equations of state" @default.
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• W2098778873 doi "https://doi.org/10.1103/physrevd.82.103011" @default.
• W2098778873 hasPublicationYear "2010" @default.
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