Crust-core transition of a neutron star: effects of the symmetry energy and temperature under strong magnetic fields

We study the simultaneous effects of the symmetry energy and temperature on the crust-core transition of a magnetar. The dynamical and the thermodynamical spinodals are used to calculate the transition region within a relativistic mean-field approach for the equation of state. Quantizing magnetic fields with intensities in the range of \( 2\times 10^{15}