Magneto-thermal evolution in the cores of adolescent neutron stars: The Grad-Shafranov equilibrium is never reached in the 'strong-coupling' regime

Nicolás A. Moraga, Francisco Castillo, Andreas Reisenegger +2

At the high temperatures present inside recently formed neutron stars ($T\gtrsim 5\times 10^8\text{K}$), the particles in their cores are in the "strong-coupling" regime, in w…