Arelativistic quantum approach to neutrino and antineutrino emission via the direct Urca process in strongly magnetized neutron-star matter

We study neutrino and antineutrino emission from the direct Urca process in neutron-star matter in the presence of strong magnetic fields. We calculate the neutrino emissivity of the direct Urca process, whereby a neutron converts to a proton, an electron and an antineutrino, or a proton-electron pair converts to a neutron-neutrino pair. We solve exact wave functions for protons and electrons in the states described with Landau levels. We find that the direct Urca process can satisfy the kinematic constraints even in density regions where this process could not normally occur in the absence of a magnetic field. (C) 2021 The Authors. Published by Elsevier B.

Automated summary

In this paper, we study the emission of neutrinos and antineutrinos from the direct Urca process in neutron-star matter in the presence of strong magnetic fields. By calculating the neutrino emissivity and solving the wave functions, we find that the direct Urca process can satisfy the kinematic constraints even in density regions where it would not normally occur without a magnetic field.