Figure 1: Neutron-star EOS for non-rotational configurations: BPS (triangles), Haensel & Pichon (1994) (HP94, stars), SLy (dots), OPAL at T=10^{6}, 10^{7}, and 10^{8} K (dashed lines), the fit (14) (solid line) and the fit modified at low (dotted line). | |
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Figure 2: Comparison of the data and fits for SLy and FPS EOSs for non-rotational configurations. Upper panel: rarefied tabular data (symbols) and the fit (14) (lines); lower panel: relative difference between the data and fit. Filled dots and solid line: SLy; open circles and dot-dashed line: FPS (triangles and stars on the upper panel are BPS and HP94 data at g cm^{-3}). | |
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Figure 3: Dependence of on n. Upper panel: rarefied data (symbols) and the fit (15) (lines); lower panel: relative difference between the data and fit. Filled dots and solid line: SLy; open circles and dot-dashed line: FPS. | |
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Figure 4: SLy and FPS EOS for rotational configurations. Upper panel: rarefied data to be fitted, calculated according to Eq. (14) (symbols) and the fit (17) (lines); lower panel: relative difference between the data and fit. Filled dots and solid line: SLy; open circles and dot-dashed line: FPS. | |
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Figure 5: Adiabatic index for SLy and FPS EOSs. Solid line: analytical approximation (SLy); dotted line: precise values (SLy); dot-dashed line: analytical approximation (FPS). | |
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