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Spin oscillations in neutrino gravitational scattering

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arxiv 2311.14475 v2 pith:RFEZKY2B submitted 2023-11-24 hep-ph astro-ph.HEgr-qc

Mridupawan Deka (1) , Maxim Dvornikov (1 , 2) ((1) JINR , (2) IZMIRAN) This is my paper · ORCID
classification hep-phastro-ph.HEgr-qc
keywords neutrinospinoscillationsdiskmagneticparticlesaccountingaccretion
verification ladder T0 review T1 audit T2 compute T3 formal
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We study neutrino spin oscillations while the particles scatter off a rotating black hole surrounded by a thick magnetized accretion disk. Neutrino spin precession is caused by the interaction of the neutrino magnetic moment with the magnetic field in the disk which has both toroidal and poloidal components. Our calculation of the observed neutrino fluxes, accounting for spin oscillations, are based on numerical simulations of the propagation of a great number of incoming test particles using High Performance Parallel Computing. The obtained results significantly improve our previous findings. We briefly discuss the applications for the observations of astrophysical neutrinos.

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Cited by 1 Pith paper

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  1. Neutrino spin oscillations near a black hole

    hep-ph 2025-02 conditional novelty 5.0 of 10

    Neutrinos scattered by a black hole's accretion disk undergo non-negligible spin flip from the toroidal magnetic field alone, contrary to earlier studies.

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