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Towards interferometry of neutrino electromagnetism

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arxiv 2204.02886 v2 pith:FQI2YBKK submitted 2022-04-06 hep-ph

Towards interferometry of neutrino electromagnetism

classification hep-ph
keywords neutrinoeffectmediumphotonpolarizationangledependencederive
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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It is predicted within the Standard Model of elementary particles that asymmetric neutrino environments cause rotation of linear polarization of electromagnetic wave -- the birefringence. We demonstrate that this effect is strongly enhanced if additionally the photon is propagating through refractive medium, which effectively increases the photon exposure to the neutrino medium. Our estimate for infrared laser beam in $1\,\mathrm{m}$ long optical fiber exposed to reactor anti-neutrino flux results in linear polarization rotation by the angle $\sim4.6\times10^{-39}\,\mathrm{rad}$. We also derive the proper dependence of the effect on the angle between the directions of photon and neutrino propagation in the laboratory frame. For that purpose we derive the correct form of the basis of polarization four-vectors, which differs from the one widely used in literature. We also estimate the sub-leading optical effect of the neutrino medium due to the neutrino dipole magnetic moment, in terms of a variation of the refractive index and its angular dependence. A rough monochromatic approximation points towards the existence of a resonant enhancement of the effect.

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Cited by 2 Pith papers

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  1. Enhanced active-sterile neutrino polarizability at the intensity frontier

    hep-ph 2025-12 conditional novelty 7.0

    A new neutrino-photon interaction involving a sterile neutrino is constrained at NOMAD and MiniBooNE, and a light-mediator realization can fit the MiniBooNE excess.

  2. Neutrino-Induced Polarization Rotation in Active Galactic Nuclei Plasmas

    hep-ph 2026-01 conditional novelty 5.0

    Neutrino-induced polarization rotation in AGN plasmas is computed and found to produce a frequency scaling distinct from Faraday rotation, but with angles far below current polarimetric sensitivity.