Magnetic horizons of ultra-high energy cosmic rays
The propagation of ultra-high energy cosmic rays in extragalactic magnetic fields can be diffusive, depending on the strength and properties of the fields. In some cases the propagation time of the particles can be comparable to the age of the universe, causing a suppression in the flux measured on...
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| Μορφή: | Conference item |
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Deutsches Elektronen-Synchrotron
2014
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