Deflection of ultra-high energy heavy nuclei in the Galactic magnetic field
In this work, we investigate the impacts a potential shift towards a heavy composition at the end of the cosmic ray (CR) spectrum would have on the future data [1, 2]. We present detailed simulations for the propagation of ultra-high energy (UHE) heavy nuclei, with E ≥ 60 EeV, within recent Galactic...
Main Authors: | Semikoz Dmitri, Sigl Günter, Giacinti Gwenael, Kachelrieß Michael |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2013-06-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20135306004 |
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