Interpretation of ultra-high energy multi-messenger data
Charged ultra-high energy cosmic rays above ∼1017 eV are most likely accelerated in powerful astrophysical objects that have to meet a number of requirements to reach energies beyond the highest energies observed, a few 1020 eV, among them sufficient electromagnetic power and further constraints on...
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| Format: | Article |
| Language: | English |
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EDP Sciences
2013-06-01
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| Series: | EPJ Web of Conferences |
| Online Access: | http://dx.doi.org/10.1051/epjconf/20135301013 |