| Authors | M. Ghazanfari Mojarrad, N. S. Razavi and S. Vaezzade |
|---|---|
| Journal | Nucl. Phys. A |
| Page number | 51 |
| Volume number | 980 |
| Paper Type | Full Paper |
| Published At | 2018 |
| Journal Grade | ISI |
| Journal Type | Typographic |
| Journal Country | Netherlands |
| Journal Index | ISI |
Abstract
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).