On Signatures of a Possible New Physics Resonance in Atmospheric Air Showers Using a Parameterized Model
Jiri Kvita

TL;DR
This paper develops a parameterized model of atmospheric air showers to investigate how hypothetical new physics resonances at 100 GeV and 1 TeV could influence shower profiles, potentially aiding future detection of such phenomena.
Contribution
It introduces a simple model incorporating new physics resonances into atmospheric shower simulations, analyzing their effects on shower depth and shape, and proposing new methods for detection.
Findings
Resonances can affect shower depth at energies near their mass thresholds.
Decay modes influence the shape and direction of the modified shower profiles.
Visibility of resonances depends on their width, diminishing at narrower widths.
Abstract
We present a parameterized model of atmospheric particle showers initiated by cosmic rays. Few physics shower parameters are tuned in a comparison to the Conex generator. Resulting shower properties are studied, with a comment on the cases where multiple shower maxima develop. Finally, we implement simple models of new physics resonance of masses of 100 GeV and 1 TeV and examine their effects on the shower profile, depth and maximum variation in dependence of the decay channel of the hypothetical resonance. It is shown that a new resonance effects can appear at the energy threshold and can persist for about a decade in . Various assumed decay modes of the hypothetical resonance have different effects on the direction and shape of the modified average shower depth as function of the energy, with possible implications for current or future measurements. It is…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radiation Therapy and Dosimetry · Dark Matter and Cosmic Phenomena
