Influence of structured extragalactic magnetic fields on the propagation of UHECRs

Details Influence of structured extragalactic magnetic fields on the propagation of UHECRs Influence of structured extragalactic magnetic fields on the propagation of UHECRs

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..439a&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

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Scientific paper

The origin of the highest energy cosmic rays (UHECRs, E ≥ 1019 eV) remains a mystery. The Pierre Auger experiment will collect an unprecendented statistics at those energies, and therefore allow to detect potential sources. We discuss the influence of extragalactic magnetic fields, which are still poorly known, on the propagation of UHECRs and show that they can lead to substantial deflections and even changes in the spectrum shape if there are heavy nuclei.

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