Magnetization for -equilibrium matter [panels (a) and (c)] and isochemical potential quark matter [panels (b) and (d)]. Densities of interest for each scenario are considered. In (a) and (b) the magnetization is shown as a function of and in (c) and (d) as a function of the baryonic density.
Parallel (the continuous lines) and perpendicular (the marks) pressures for -equilibrium matter [panels (a) and (c)] and isochemical potential quark matter [panels (b) and (d)]. Densities of interest for each scenario are considered. In (a) and (b) the pressures are shown as a function of the baryonic density and in (c) and (d) as a function of .