In this work we present the preliminary results of a complete equation of state (EoS) for core-collapse supernova simulations. We treat uniform matter made of nucleons using the the quark-meson coupling (QMC) model. We show a table with a variety of thermodynamic quantities, which covers the proton fraction range Yp=0−0.65 with the linear grid spacing ΔYp=0.01 (66 points) and the density range ρB=1014−1016g.cm−3 with the logarithmic grid spacing Δlog10(ρB/[g.cm−3])=0.1 (21 points). This preliminary study is performed at zero temperature and our results are compared with the widely used EoS already available in the literature.
@article{arxiv.1506.02641,
title = {Preliminary EoS for core-collapse supernova simulations with the QMC model},
author = {Guilherme Grams and Alexandre M. Santos and Débora P. Menezes},
journal= {arXiv preprint arXiv:1506.02641},
year = {2022}
}