Propagation of ultra high energy cosmic rays

Todor Stanev

doi:10.1016/j.crhy.2004.03.014

Propagation of ultra high energy cosmic rays
[Propagation des rayons cosmiques ultra-énergétiques]

Présenté par : Pierre Encrenaz

Todor Stanev ¹

¹ Bartol Research Institute, University of Delaware Newark, Delaware Newark, DE 19716, USA

Comptes Rendus. Physique, Ultimate energy particles in the Universe, Volume 5 (2004) no. 4, pp. 453-461.

Résumé
Abstract

Tout rayon cosmique dont l'énergie est proche de 10²⁰ eV subit des interactions inélastiques avec le fond cosmologique micro-onde ou avec d'autres champs de photons d'origine astrophysique, en perdant une partie de son énergie. Nous décrivons brièvement les mécanismes de perte d'énergie et en analysons les conséquences sur la propagation de protons dans l'epace extra-galactique. Nous décrivons également l'effet des champs magnétiques d'origine astrophysique sur la propagation.

All particles of energy approaching 10²⁰ eV interact inelastically in the microwave background and other astrophysical photon fields and lose energy. We describe briefly the energy loss processes and show the consequences of proton propagation in extragalactic space. We also discuss the influence of astrophysical magnetic fields on the propagation.

Publié le : 2004-04-24

DOI : 10.1016/j.crhy.2004.03.014

Keywords: Microwave background, Energy loss, GZK cutoff, Magnetic fields (galactic and extragalactic)
Mots-clés : Rayonnement fossile, Perte d'énergie, Coupure GZK, Champs magnétiques (galactiques et extra-galactiques)

Affiliations des auteurs :

Todor Stanev ¹

¹ Bartol Research Institute, University of Delaware Newark, Delaware Newark, DE 19716, USA

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Todor Stanev. Propagation of ultra high energy cosmic rays. Comptes Rendus. Physique, Ultimate energy particles in the Universe, Volume 5 (2004) no. 4, pp. 453-461. doi : 10.1016/j.crhy.2004.03.014. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2004.03.014/

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