Cosmic ray induced micro black hole showers
M.V. Garzelli, M. O'Loughlin, S. Nafooshe

TL;DR
This paper explores the hypothesis that microscopic black holes produced in ultra-high-energy cosmic ray collisions could explain discrepancies in observed air shower properties, suggesting new physics beyond standard models.
Contribution
It introduces the idea that microscopic black hole production in cosmic ray interactions may account for air shower anomalies within TeV gravity models.
Findings
Lepton distributions may better indicate black hole presence than photon distributions.
Preliminary results suggest black hole evaporation affects air shower characteristics.
The model offers a potential explanation for existing experimental discrepancies.
Abstract
Extended air showers originate from interactions between ultra-high-energy cosmic rays and nuclei in the Earth's atmosphere. At present there are some discrepancies between experimental observed properties of these air showers and theoretical predictions obtained by using standard hadronic interaction models for cosmic ray primaries with laboratory energies above 10^5 - 10^6 TeV. In this contribution, we will present a preliminary discussion of the possibility (in the framework of TeV gravity models) that shower development may begin with the production of a microscopic black hole (MBH) at the moment of the primary collision, which then evaporates and decays, by emitting gravitons and Standard Model quanta. From our preliminary investigations it appears that lepton distributions are more likely to reveal the presence of a MBH than photon distributions.
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Astrophysics and Cosmic Phenomena · Particle Accelerators and Free-Electron Lasers
