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...
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| フォーマット: | 論文 |
| 言語: | English |
| 出版事項: |
EDP Sciences
2017-01-01
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| シリーズ: | EPJ Web of Conferences |
| オンライン･アクセス: | https://doi.org/10.1051/epjconf/201713503001 |