期刊
PHYSICAL REVIEW D
卷 82, 期 10, 页码 -出版社
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.82.103011
关键词
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资金
- Sherman Fairchild Foundation
- NSF [PHY-0601459]
- NASA [NNX09AF97G]
- NASA [118467, NNX09AF97G] Funding Source: Federal RePORTER
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.
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