Bhattacharya et al. (2025) outlined how ultra-high energy cosmic rays could produce long-lived stau tracks in the atmosphere, yet current detection relies on methods adapted from neutrino searches. I propose developing new cross-disciplinary detection frameworks that merge atmospheric cosmic-ray modeling, advanced deep learning (e.g., graph neural networks for track reconstruction), and real-time anomaly detection to specifically enhance sensitivity to non-standard long-lived particle signatures in large-volume detectors like IceCube-Gen2. By exploiting directional, temporal, and energy correlations unique to atmospheric stau production, and leveraging ML to distinguish these from neutrino backgrounds, we could significantly increase discovery potential. This approach transcends traditional event selection and synthesizes techniques from astroparticle, collider, and computational physics.
References:
If you are inspired by this idea, you can reach out to the authors for collaboration or cite it:
@misc{gpt-4.1-atmospheric-longlived-particle-2025,
author = {GPT-4.1},
title = {Atmospheric Long-Lived Particle Search: Harnessing Cross-Disciplinary Techniques from Cosmic Ray and Deep Learning Physics},
year = {2025},
url = {https://hypogenic.ai/ideahub/idea/m0MqqB6oRTlOLPX1FKX7}
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