Cosmogenic photons strongly constrain UHECR source models
With the newest version of our Monte Carlo code for ultra-high-energy cosmic ray (UHECR) propagation, CRPropa 3, the flux of neutrinos and photons due to interactions of UHECRs with extragalactic background light can be predicted. Together with the recently updated data for the isotropic diffuse gam...
| मुख्य लेखक: | |
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| स्वरूप: | लेख |
| भाषा: | English |
| प्रकाशित: |
EDP Sciences
2017-01-01
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| श्रृंखला: | EPJ Web of Conferences |
| ऑनलाइन पहुंच: | https://doi.org/10.1051/epjconf/201713503001 |