Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory

0518868 - FZÚ 2020 RIV US eng J - Článek v odborném periodiku
Aab, A. - Abreu, A. - Aglietta, M. - Bakalová, Alena - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Juryšek, Jakub - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - dos Santos, Eva M. Martins - Schovánek, Petr - Trávníček, Petr - Vícha, Jakub - Yushkov, Alexey … celkem 391 autorů
Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory.
Physical Review D. Roč. 100, č. 8 (2019), s. 1-18, č. článku 082003. ISSN 2470-0010. E-ISSN 2470-0029
Grant CEP: GA MŠMT LTT18004; GA MŠMT LM2015038; GA MŠMT EF16_013/0001402
Grant ostatní: OP VVV - AUGER-CZ(XE) CZ.02.1.01/0.0/0.0/16_013/0001402
Institucionální podpora: RVO:68378271
Klíčová slova: Pierre Auger Observatory * cosmic ray * showers * invisible energy * fluorescence detection
Obor OECD: Particles and field physics
Impakt faktor: 4.833, rok: 2019
Způsob publikování: Omezený přístup
https://doi.org/10.1103/physrevd.100.082003

The determination of the primary energy of extensive air showers using the fluorescence detection technique requires an estimation of the energy carried away by particles that do not deposit all their energy in the atmosphere. This estimation is typically made using Monte Carlo simulations and thus depends on the assumed primary particle mass and on model predictions for neutrino and muon production. In this work we present a new method to obtain the invisible energy from events detected by the Pierre Auger Observatory. The method uses measurements of the muon number at ground level, and it allows us to significantly reduce the systematic uncertainties related to the mass composition and the high energy hadronic interaction models, and consequently to improve the estimation of the energy scale of the Pierre Auger Observatory.
Trvalý link: http://hdl.handle.net/11104/0303888