T high Yp lowGravitational mass

These are the results of my Bachelor thesis, on modelling properties of post-merger neutron star remnant along their radius.
The results are generated by solving the General Relativistic Tolmann Openheimer Volkoff equations for a multidimensional equation of state P=P(ρ,T, Ye) for the hadronic neutron star matter.
The parameter space is the Temperature profile along all densities, and the electron fraction profile along all densities.
In this animated plot we see the gravitational mass-vs radius profile along radius for increasing central density.