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arXiv · 2009.00851

Self-consistent approach for measuring the energy spectra and composition of cosmic rays and determining the properties of hadronic interactions at high energy

Abstract

Air showers, produced by the interaction of energetic cosmic rays with the atmosphere, are an excellent alternative to study particle physics at energies beyond any human-made particle accelerator. For that, it is necessary to identify first the mass composition of the primary cosmic ray (and its energy). None of the existing high energy interaction models have been able to reproduce coherently all air shower observables over the entire energy and zenith angle phase space. This is despite having tried all possible combinations for the cosmic ray mass composition. This proposal outlines a self-consistent strategy to study high energy particle interactions and identify the energy spectra and mass composition of cosmic rays. This strategy involves the participation of different particle accelerators and astrophysics experiments. This is important to cover the entire cosmic ray energy range and a larger phase-space of shower observables to probe the high energy interaction models.

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Andrea Addazi, Andy Buckley, Jose Bellido, Zhen Cao, Ruben Conceição, Lorenzo Cazon, Armando di Matteo, Bruce Dawson, Kasumasa Kawata, Paolo Lipari, Analiza Mariazzi, Marco Muzio, Shoichi Ogio, Sergey Ostapchenko, Mário Pimenta, Tanguy Pierog, Andres Romero-Wolf, Felix Riehn, David Schmidt, Eva Santos, Frank Schroeder, Karen Caballero-Mora, Pat Scott, Takashi Sako, Carlos Todero Peixoto, Ralf Ulrich, Darko Veberic, Martin White. 2020-09-02. Self-consistent approach for measuring the energy spectra and composition of cosmic rays and determining the properties of hadronic interactions at high energy. https://arxiv.org/abs/2009.00851

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