Cosmogenic neutrinos and ultra-high energy cosmic ray models

• Published in: arXiv.org
• Main Authors: Aloisio, R, Boncioli, D, A di Matteo, Grillo, A F, Petrera, S, Salamida, F
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 06.10.2015
• Subjects: Astronomical models; Augers; Chemical composition; Computer simulation; Cosmic rays; Fluxes; High energy astronomy; Monte Carlo simulation; Neutrinos; Observatories; Organic chemistry; Physics - High Energy Astrophysical Phenomena; Physics - High Energy Physics - Phenomenology
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.1505.04020

We use an updated version of {\it SimProp}, a Monte Carlo simulation scheme for the propagation of ultra-high energy cosmic rays, to compute cosmogenic neutrino fluxes expected on Earth in various scenarios. These fluxes are compared with the newly detected IceCube events at PeV energies and with recent experimental limits at EeV energies of the Pierre Auger Observatory. This comparison allows us to draw some interesting conclusions about the source models for ultra-high energy cosmic rays. We will show how the available experimental observations are almost at the level of constraining such models, mainly in terms of the injected chemical composition and cosmological evolution of sources. The results presented here will also be important in the evaluation of the discovery capabilities of the future planned ultra-high energy cosmic ray and neutrino observatories.