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Fig. 6.

image

Composition of dense matter for different physical regimes. Left (right) panel: composition of β-stable neutrino-free (trapped) nuclear matter, i.e., the particle fractions Yi = ni/n (with i = n, p, e, μ), in the case of an isoentropic EOS with S/A = 2. Right panel: we fix Yle = 0.33. The dashed lines in the left panel represent the composition of the T = 0 BL EOS (Bombaci & Logoteta 2018) which is reported for comparison. See text for further details.

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