PeV neutrinos from ultra-high-energy cosmic rays

Gunter Sigl, Arjen Van Vliet

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

We investigate the possibility that the recently detected TeV-PeV neutrino events by IceCube can originate from extragalactic ultra-high-energy cosmic ray interactions with the cosmic microwave background or the UV/optical/IR background. This is done by simulating the propagation of the cosmic rays from their sources to the observer, including the production and propagation of secondary neutrinos and gamma rays. For this purpose we use the publicly available simulation package CRPropa 2.0. We find that in all the scenarios considered here the simulated neutrino flux level remains at least one order of magnitude below the flux level indicated by the IceCube events, thus showing it is difficult to interpret the IceCube events in terms of a cosmogenic neutrino flux.

Original languageBritish English
Title of host publicationProceedings of the 49th Rencontres de Moriond - 2014 Electroweak Interactions and Unified Theories, EW 2014
EditorsEtienne Auge, Jacques Dumarchez, Jean Tron Thanh Van
Pages177-182
Number of pages6
ISBN (Electronic)9782954640037
StatePublished - 2014
Event49th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2014 - La Thuile, Italy
Duration: 15 Mar 201422 Mar 2014

Publication series

NameProceedings of the 49th Rencontres de Moriond - 2014 Electroweak Interactions and Unified Theories, EW 2014

Conference

Conference49th Rencontres de Moriond on Electroweak Interactions and Unified Theories, EW 2014
Country/TerritoryItaly
CityLa Thuile
Period15/03/1422/03/14

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