A new air-shower observable to constrain hadronic interaction models

Autor(es)

Prado, Raul R. ; de Souza, Vitor

• Tipo de documento: Artigo Científico
• Fonte: Astroparticle Physics; v. 93, p. 28-37, JUL 2017.
• Citações Web of Science: 0

Resumo

The energy spectrum of muons at ground level in air showers is studied and a new observable is proposed to constrain hadronic interaction models used in air shower simulations. An asymmetric Gaussian function is proposed to describe the muon ground energy spectrum and its parameters are studied regarding primary particle, energy and hadronic interaction models. Based on two realistic measurements of the muon density at a given distance from the shower axis, a new observable (r mu is defined. Considering realistic values of detector resolutions and number of measured events, it is also shown r mu, can be successfully used to constrain low and high energy hadronic interaction models. The study is focused in the energy range between 10(17.5) and 10(18.0) eV because of the importance of this interval for particle physics and astrophysical models. The constraining power of the new observable is shown to be large within current experimental capabilities. (C) 2017 Elsevier B.V. All rights reserved. (AU)

• Processo FAPESP: 14/10460-1 - Análise de chuveiros atmosféricos extensos: física de partículas com aceleradores extraterrestres
• Beneficiário: Raul Ribeiro Prado
• Linha de fomento: Bolsas no Brasil - Doutorado
• Processo FAPESP: 14/19946-4 - Nova geração de detectores de múons RPC para medida de raios cósmicos de altíssima energia com grande precisão
• Beneficiário: Carola Dobrigkeit Chinellato
• Linha de fomento: Auxílio à Pesquisa - Regular
• Processo FAPESP: 15/15897-1 - Cherenkov Telescope Array - CTA
• Beneficiário: Luiz Vitor de Souza Filho
• Linha de fomento: Auxílio à Pesquisa - Temático