A van Vliet, RA Batista, JR Hörandel - arXiv preprint arXiv:1909.01932, 2019 - arxiv.org
Cosmogenic neutrinos are created when ultra-high-energy cosmic rays (UHECRs) interact with extragalactic photon backgrounds. In general, the expected flux of these cosmogenic …
Abstract The detection of Ultra-High-Energy (UHE) neutrinos around and above 1018 eV (1 EeV) can be the key to answering the long-standing question of the origin of the UHE cosmic …
A Vliet, RA Batista, J Horandel - 2019 - repository.ubn.ru.nl
With the detection of an astrophysical neutrino flux by IceCube [2] a new window to the Universe has opened. One possible origin of astrophysical neutrinos detected at Earth is …
OP Auger - arXiv preprint arXiv:1906.07419, 2019 - academia.edu
With the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky …