Savina, P. (2020) Search for neutrino and photon primary particles in the EeV energy range with the Pierre Auger Observatory. Il nuovo cimento C, 43 (2-3). pp. 1-3. ISSN 1826-9885
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Abstract
The Pierre Auger Observatory is the world’s largest cosmic-ray observatory. Updated results on the search for ultra-high energy photons and neutrinos in the EeV (1 EeV= 1018 eV) energy range are presented. Ultra-high energy photons can be produced either in the interactions with the cosmic microwave background or by the decay of hypothetical super-massive particles. Ultra-high energy neutrinos may arise from astrophysical sources due to hadronic interactions in the surrounding matter. The reached sensitivity is shown to be better (for photons) or comparable (for neutrinos) to other detectors.
Item Type: | Article |
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Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
Depositing User: | Marina Spanti |
Date Deposited: | 18 Mar 2021 08:53 |
Last Modified: | 18 Mar 2021 08:53 |
URI: | http://eprints.bice.rm.cnr.it/id/eprint/20832 |
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