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Cosmogenic neutrinos challenge the cosmic ray proton dip model
- 1.0549480 - FZÚ 2022 RIV IT eng C - Konferenční příspěvek (zahraniční konf.)
Heinze, J. … celkem 4 autorů
Cosmogenic neutrinos challenge the cosmic ray proton dip model.
Proceedings of Science. Vol. 301. Trieste: Sissa Medilab srl, 2018, s. 1-8, č. článku 0589. ISSN 1824-8039.
[The 35th International Cosmic Ray Conference (ICRC2017). Busan (KR), 10.07.2017-20.07.2017]
Výzkumná infrastruktura: AUGER-CZ - 90038
Klíčová slova: ultra-high-energy cosmic rays * proton dip model
Obor OECD: Particles and field physics
https://pos.sissa.it/301/589/pdf
The origin and composition of ultra-high-energy cosmic rays (UHECRs) remain a mystery. The proton dip model describes the shape of the cosmic ray spectrum above 109 GeV by the effect of a pure proton spectrum propagating through the cosmic microwave background. In these interactions secondary neutrinos are produced.
Trvalý link: http://hdl.handle.net/11104/0325471
Počet záznamů: 1