Fig. 4.
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EOSs of β-stable neutrino-free matter at different temperature values ranging from T = 0 to 50 MeV. For T lower than Tlim = 7.21 MeV, we display the NS EOS containing the hot inner crust using the BCPM functional. At T > 7.21 MeV, the NS is composed of homogeneous dense matter, thus we illustrate the results of the bulk part of the hot BCPM functional.
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