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Prospective constraints on Lorentz violation from ultrahigh-energy photon detection

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arxiv 1312.4368 v2 pith:N4YN3SZL submitted 2013-12-16 astro-ph.HE gr-qchep-phhep-th

classification astro-ph.HEgr-qchep-phhep-th
keywords lorentzphotonsviolationwillabsenceatmosphereconstraintsdetection
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We point out that violation of Lorentz invariance affects the interaction of high-energy photons with the Earth's atmosphere and magnetic field. In certain parameter region this interaction becomes suppressed and the photons escape observation passing through the atmosphere without producing air showers. We argue that a detection of photon-induced air showers with energies above 10^19 eV, implying the absence of suppression as well as the absence of photon decay, will put tight double-sided limits on Lorentz violation in the sector of quantum electrodynamics. These constraints will be by several orders of magnitude stronger than the existing ones and will be robust against any assumptions about the astrophysical origin of the detected photons.

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  1. Constraining Lorentz invariance violation from the depth of air-shower maximum

    astro-ph.HE 2026-08 conditional novelty 6.0 of 10

    A simulation-based toy analysis of Auger Xmax data yields M_LIV > 1.5e21 GeV (95% CL) for subluminal photon-sector Lorentz invariance violation, subject to simplified detector and composition assumptions.

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