Graph Neural Networks for Photon Searches with the Underground Muon Detector of the Pierre Auger Observatory
Ezequiel Rodriguez (on behalf of the Pierre Auger Collaboration)

TL;DR
This paper introduces a deep learning-based method using graph neural networks to distinguish ultra-high-energy photons from hadronic cosmic rays by analyzing data from the Pierre Auger Observatory's detectors, aiming to improve indirect photon detection.
Contribution
The paper presents a novel graph attention network approach for photon-hadron discrimination utilizing combined surface and underground muon detector data, enhancing sensitivity to diffuse photon fluxes.
Findings
Effective discrimination between photon and hadron-induced air showers.
Potential to improve detection sensitivity for ultra-high-energy photons.
Framework adaptable to increasing data volumes in future observations.
Abstract
Ultra-high-energy photons have long been sought as tracers of the most energetic processes in the Universe. Several sources can contribute to a diffuse photon flux, including interactions of cosmic rays with Galactic matter and radiation fields, as well as more exotic scenarios such as the decay of super-heavy dark matter. Regardless of their origin, the expected flux is extremely low, making direct detection impractical and thereby requiring indirect detection by extensive ground-based detector arrays. In this contribution, we present a novel method for photon-hadron discrimination in the energy range of to based on deep learning algorithms. Our approach relies on information from both the Surface Detector (SD) and the Underground Muon Detector (UMD) of the Pierre Auger Observatory. The SD consists of an array of water-Cherenkov detectors. It is used to measure…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies
