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Astroparticle Physics 35 (2011) 192
Ultrahigh Energy Nuclei in the Turbulent Galactic Magnetic Field
G. Giacinti1, 2, M. Kachelriess3, D.V. Semikoz1, G. Sigl1, 2
(11/2011)

In this work we study how the turbulent component of the Galactic magnetic field (GMF) affects the propagation of ultrahigh energy heavy nuclei. We investigate first how the images of individual sources and of the supergalactic plane depend on the properties of the turbulent GMF. Then we present a quantitative study of the impact of the turbulent field on (de-) magnification of source fluxes, due to magnetic lensing effects. We also show that it is impossible to explain the Pierre Auger data assuming that all ultrahigh energy nuclei are coming from Cen A, even in the most favorable case of a strong, extended turbulent field in the Galactic halo.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
2 :  ITP - Institut für Theoretische Physik
3 :  NTNU - Institutt for fysikk, NTNU
APC - THEORIE
Physique/Astrophysique/Phénomènes cosmiques de haute energie

Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie
Lien vers le texte intégral : 
http://fr.arXiv.org/abs/1104.1141