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Bremsstrahlung from Neutrino Scattering via Magnetic Dipole Moments

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arxiv 2208.01207 v2 pith:ISQQLVR4 submitted 2022-08-02 hep-ph astro-ph.CO

Konstantin Asteriadis , Alejandro Quiroga Triviño , Martin Spinrath This is my paper · ORCID
classification hep-phastro-ph.CO
keywords neutrinomomentsscatteringbremsstrahlungdipolemagneticneutrinosbackground
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In this paper we discuss bremsstrahlung induced by neutrino scattering. This process should exist since neutrinos are expected to couple to photons via magnetic dipole and transition moments. These moments are loop-induced and tiny in the Standard Model with neutrino masses but could be significantly enhanced in extended theories. As concrete example we study the scattering of the two largest neutrino fluxes on earth, solar neutrinos and Cosmic Neutrino Background (CNB). It is tempting to consider this as a potential signature for CNB searches but it turns out that the signal is extremely small and unlikely to be observed.

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Cited by 2 Pith papers

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

  1. Detection prospects for the Cosmic Neutrino Background using matter interferometers

    hep-ph 2025-11 conditional novelty 6.0 of 10

    The Cosmic Neutrino Background is predicted to induce phase shifts of ~1e-22 to 1e-14 rad in matter interferometers, far below current and near-future sensitivity.

  2. Probing Terrestrial Relic Neutrino Charge with Mach-Zehnder Interferometer

    hep-ph 2025-06 reject novelty 5.0 of 10

    A Mach-Zehnder interferometer with one vertical arm is proposed to probe relic neutrino charge, with claimed sensitivity down to epsilon_nu ~ 10^-22, but the signal calculation is flawed.

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