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In this work we present the preliminary results of a complete equation ofstate (EoS) for core-collapse supernova simulations. We treat uniform mattermade of nucleons using the the quark-meson coupling (QMC) model. We show atable with a variety of thermodynamic quantities, which covers the protonfraction range $Y_{p}=0-0.65$ with the linear grid spacing $ \Delta Y_{p}=0.01$($66$ points) and the density range $\rho_{B}=10^{14}-10^{16}$g.cm$^{-3}$ withthe logarithmic grid spacing $\Delta log_{10}(\rho_{B}/[$g.cm$^{-3}])=0.1 $($21$ points). This preliminary study is performed at zero temperature and ourresults are compared with the widely used EoS already available in theliterature.

Preliminary EoS for core-collapse supernova simulations with the QMC model