Constraining Lorentz invariance violation from the depth of air-shower maximum
Nickolay S. Martynenko, Grigory I. Rubtsov, Petr S. Satunin, Andrey K. Sharofeev, Sergey V. Troitsky
astro-ph.HE, hep-ph
Submitted: 2026-08-05
Comments: 16 pages, 4 figures. To be submitted to Phys. Rev. D
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Quantum gravity phenomenology at the dawn of the multi-messenger era -- A review
- Lorentz-Violating Extension of the Standard Model
- Data Tables for Lorentz and CPT Violation
- Lorentz violation at high energy: concepts, phenomena and astrophysical constraints
- Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory
- Bounds on Lorentz invariance violation from muon fluctuations at the Pierre Auger Observatory
- Lorentz Invariance Violation and the QED Formation Length
- On calculation of cross sections in Lorentz violating theories
- Lorentz Violation and Ultrahigh-Energy Photons
- Limits on the Lorentz Invariance Violation from UHECR astrophysics
- Improved limits on Lorentz invariance violation from astrophysical gamma-ray sources
- Constraints on violation of Lorentz invariance from atmospheric showers initiated by multi-TeV photons
- New constraints on Lorentz Invariance violation from Crab Nebula spectrum beyond $100$ TeV
- Two-sided constraints on Lorentz Invariance violation from Tibet-AS$\gamma$ and LHAASO Very-High-Energy photon observations
- Changes in extensive air showers from isotropic Lorentz violation in the photon sector
- Improved bound on isotropic Lorentz violation in the photon sector from extensive air showers
- Photon decay in UHE air showers: stringent bound on Lorentz violation
- A new bound on Lorentz violation based on the absence of vacuum Cherenkov radiation in ultra-high energy air showers
- Shower formation constraints on cubic Lorentz Invariance Violation parameters in quantum electrodynamics
- Depth of Maximum of Air-Shower Profiles above 10^17.7 eV Measured with the Fluorescence Detector of the Pierre Auger Observatory
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