Secondary neutrino and gamma-ray fluxes from SimProp and CRPropa

0546500 - FZÚ 2022 RIV GB eng J - Článek v odborném periodiku
Batista, R. A. … celkem 4 autorů
Secondary neutrino and gamma-ray fluxes from SimProp and CRPropa.
Journal of Cosmology and Astroparticle Physics. Roč. 2019, č. 5 (2019), č. článku 006. ISSN 1475-7516. E-ISSN 1475-7516
Výzkumná infrastruktura: AUGER-CZ - 90038
Klíčová slova: ultra high energy cosmic rays * ultra high energy photons and neutrinos
Obor OECD: Particles and field physics
Impakt faktor: 5.210, rok: 2019
Způsob publikování: Omezený přístup
https://doi.org/10.1088/1475-7516/2019/05/006

The interactions of ultra-high energy cosmic rays (UHECRs) with background photons in extragalactic space generate high-energy neutrinos and photons. Simulating UHECR propagation requires assumptions about physical quantities such as the spectrum of the extragalactic background light (EBL) and photodisintegration cross sections. These assumptions, as well as the approximations used in the codes, may influence the computed predictions both of cosmic-ray spectra and composition, and of cosmogenic neutrino and photon fluxes. Following up on our previous work where we studied the resulting uncertainties on cosmic-ray simulations, here we quantify those on neutrinos and photons, using the Monte Carlo codes CRPropa and SimProp in various source scenarios. We discuss the results in the light of the constraining power of the neutrino and photon spectra on the origin of the UHECRs.
Trvalý link: http://hdl.handle.net/11104/0322990