Current constraints from cosmogenic neutrinos on the fraction of protons in UHECRs
Cosmogenic neutrinos are created when ultra-high-energy cosmic rays (UHECRs) interact with extragalactic photon backgrounds. In general, the expected flux of these cosmogenic neutrinos depends on multiple parameters, describing the sources and propagation of UHECRs. In our recent paper (van Vliet et...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
Sissa Medialab
2019
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