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Photon emission by an electron in a constant background field modeling a Lorentz-noninvariant vacuum

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arxiv 2405.19557 v2 pith:4ZTRNK7G submitted 2024-05-29 hep-ph

Anatoly V. Borisov This is my paper · ORCID
classification hep-ph
keywords backgroundfieldelectronradiationconstantangularastrophysicalcalculated
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The power and the probability of electromagnetic radiation from an electron in a constant background tensor field violating Lorentz invariance are calculated. The case of a background field of the quasielectric type is considered. The angular distribution and the polarization of the radiation are studied. Using present experimental constraints on the background field strength, it is shown that the radiation effect can manifest itself under astrophysical conditions at ultrahigh electron energy.

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  1. Vacuum Cherenkov radiation for nonminimal dimension-5 Lorentz violation

    hep-ph 2025-08 conditional novelty 6.0 of 10

    Isotropic dimension-5 Lorentz violation in fermions is constrained to below 1e-18 GeV^-1 (proton, m-type) and 3e-28 GeV^-1 (proton, a-type) by the absence of vacuum Cherenkov radiation in cosmic rays.

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