Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
Marco Manno, Pablo Mart\'inez-Mirav\'e, Irene Tamborra

TL;DR
This paper explores how magnetic fields and matter influence neutrino flavor conversion during the collapse of massive stars, with implications for neutrino detection and astrophysical observations.
Contribution
It introduces a three-dimensional simulation study of neutrino flavor conversion considering magnetic moments and magnetic fields in magnetorotational stellar collapses.
Findings
Resonant flavor conversion occurs in matter during collapse.
Magnetic moments induce neutrino-antineutrino mixing for Majorana neutrinos.
Neutrino event rates depend on collapse orientation and flavor conversion scenarios.
Abstract
The magnetorotational collapse of massive stars copiously emits neutrinos of all flavors, with a prominent hierarchy between the non-electron and electron flavor average energies. Relying on a three-dimensional neutrino-magnetohydrodynamic simulation of a progenitor, we investigate flavor conversion in matter. We find that, in addition to resonant flavor conversion of neutrinos and antineutrinos in matter, (anti)neutrinos experience chirality-flipping interactions due to their non-zero magnetic moment () and large magnetic field in the source ( G). For Majorana neutrinos, this leads to resonant flavor-changing neutrino-antineutrino mixing. The event rate expected from a Galactic collapse at current and next-generation neutrino telescopes, such as IceCube and Hyper-Kamiokande, strongly depends on the orientation of the…
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