نویسندگان | M. Ghazanfari Mojarrad, N. S. Razavi and S. Vaezzade |
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نشریه | Nucl. Phys. A |
شماره صفحات | 51 |
شماره مجلد | 980 |
نوع مقاله | Full Paper |
تاریخ انتشار | 2018 |
رتبه نشریه | ISI |
نوع نشریه | چاپی |
کشور محل چاپ | هلند |
نمایه نشریه | ISI |
چکیده مقاله
An isentropic description of the equation of state (EOS) for β-stable nuclear matter (BSNM) is pre-sented in a semi-classical mean-field model. Within the Thomas–Fermi (TF) approximation, the Landau Fermi-liquid theory (LFT) is used in a self-consistent approach. Accordingly, isentropic thermodynamics of BSNM is investigated for the neutrino-free and neutrino-trapped cases. We find that the EOS for neutrino-trapped matter is stiffer than the one for neutrino-free matter. Our findings can set the stage for profound studies about the structure and composition of proto-neutron stars (PNSs).