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New Resonances of Supernova Neutrinos in Twisting Magnetic Fields

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arxiv 2303.13572 v2 pith:3J6GL2RQ submitted 2023-03-23 hep-ph astro-ph.HEastro-ph.SRhep-ex

classification hep-phastro-ph.HEastro-ph.SRhep-ex
keywords magneticneutrinosconversionfieldneutrinoresonantspinsupernova
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We investigate the effect of resonant spin conversion of the neutrinos induced by the geometrical phase in a twisting magnetic field. We find that the geometrical phase originating from the rotation of the transverse magnetic field along the neutrino trajectory can trigger a new resonant spin conversion of Dirac neutrinos inside the supernova, even if there were no such transitions in the fixed-direction field case. We have shown that even though resonant spin conversion is too weak to affect solar neutrinos, it could have a remarkable consequence on supernova neutronization bursts where very intense magnetic fields are quite likely. We demonstrate how the flavor composition at Earth can be used as a probe to establish the presence of non-negligible magnetic moments, potentially down to $10^{-15}~\mu_B$ in upcoming neutrino experiments like the Deep Underground Neutrino Experiment (DUNE), and the Hyper-Kamiokande (HK). Possible implications are analyzed.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Decoupling Neutrino Magnetic Moment from Mass with $SU(2)_L$ Invariance

    hep-ph 2025-06 reject novelty 7.0 of 10

    A loop-level neutrino magnetic moment is generated via an SU(2)_L adjoint fermion 'bridge', making the mass diagram vanish by tracelessness of the generators, though RG mixing limits the observable size.

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