Photon decay in UHE air showers: stringent bound on Lorentz violation

TL;DR

This paper improves constraints on Lorentz violation by analyzing ultra-high-energy cosmic ray air showers, incorporating fluctuations in shower maximum depth to significantly tighten bounds on photon decay scenarios.

Contribution

It introduces the use of shower-to-shower fluctuations in $X_{max}$ to enhance bounds on Lorentz violation in UHE photon decay, improving previous limits by a factor of 50.

Findings

Stricter bounds on Lorentz violation from UHE photon decay.

Inclusion of shower fluctuations enhances sensitivity.

Improved constraints by a factor of 50.

Abstract

In extensive air showers induced by ultra-high-energy (UHE) cosmic rays, secondary photons are expected to be produced at energies far above those accessible by other means. It has been shown that the decay of such photons, as possible in certain theories allowing Lorentz violation, can lead to significant changes of the shower development. Based on observations of the average depth of the shower maximum $\left<X_\text{max}\right>$, a stringent bound on Lorentz violation has been placed in a previous work. Here we include the shower-to-shower fluctuations $\sigma(X_\text{max})$ as an additional observable. The combined comparison of $\left<X_\text{max}\right>$ and $\sigma(X_\text{max})$ to shower observations allows a much stricter test of the possible decay of UHE photons, improving the previous bound by a factor of 50.