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Electroweak axion in light of GRB221009A

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arxiv 2210.08841 v3 pith:UWMPLVPB submitted 2022-10-17 hep-ph astro-ph.COastro-ph.HE

classification hep-phastro-ph.COastro-ph.HE
keywords axionelectroweakgrb221009aanomalyarxivassociatedboostconsistent
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abstract

Recently, arXiv:2210.05659 shows that a photon-axion like particle (ALP) oscillation can boost the survival rate of the high energy photons associated with the observed GRB221009A event. Here, we show that the proposed ALP is consistent with the electroweak axion with an anomaly free $Z_{10}$ Froggatt-Nielsen symmetry.

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  1. Carpet-3 detection of a photon-like air shower with estimated primary energy above 100 TeV in a spatial and temporal coincidence with GRB 221009A

    astro-ph.HE 2025-02 conditional novelty 6.0 of 10

    Carpet-3 reports a photon-like air shower with estimated energy around 300 TeV arriving from the direction of GRB 221009A about 75 minutes after the trigger, with a coincidence probability of about 0.9 percent.

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