We study neutrino and anti-neutrino emissions through the neutrino-antineutrino pair emission and the direct urca processes in the strong magnetic field, The strong magnetic fields supply additional momentum and the neutrino emissivity
and largely enhance the emissivity. We solve exact wave functions for protons and electrons in the states described
with Landau levels. Both processes in strong magnetic fields are expected to contribute significantly
to the cooling of the magnetars.
Volume 380 -
Particles and Nuclei International Conference 2021 (PANIC2021) -
Nuclear and particle astrophysics
Neutron Star Cooling on Strong Magnetic Field : Neutrino -Antineutrino Pair Emission and Direct Urca Processes
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Published on:
May 24, 2022
Abstract
DOI: https://doi.org/10.22323/1.380.0320
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.