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...
| المؤلف الرئيسي: | |
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| التنسيق: | مقال |
| اللغة: | English |
| منشور في: |
EDP Sciences
2017-01-01
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| سلاسل: | EPJ Web of Conferences |
| الوصول للمادة أونلاين: | https://doi.org/10.1051/epjconf/201713503001 |