2 papers
astro-ph.HE2025
Three-dimensional numerical simulations of neutron star cores in the two-fluid MHD approximation: simple configurations
Andrei Igoshev, Nicolás A. Moraga, Andreas Reisenegger +2
Magnetic field evolution in neutron star cores is not fully understood. We describe the field evolution both for one barotropic fluid as well as two collisionally coupled barotropi…
astro-ph.HE2023
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 (), the particles in their cores are in the "strong-coupling" regime, in w…