Ultra High Energy Cosmic Radiation: Experimental and Theoretical Status

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type , Conference object 01 Jan 2006Embargo end date: 01 Jan 2006 France Publisher:AIPJournal:AIP Conference Proceedings, volume 878, pages 405-411 (issn: 0094-243X,

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Authors: Sigl, G.;

doi: 10.1063/1.2409112 , 10.48550/arxiv.astro-ph/0609257

arXiv: astro-ph/0609257

Ultra High Energy Cosmic Radiation: Experimental and Theoretical Status

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Abstract

We give a brief overview of the current experimental and theoretical status of cosmic rays above ~10**17 eV. We focus on the role of large scale magnetic fields and on multi-messenger aspects linking charged cosmic ray with secondary gamma-ray and neutrino fluxes.

7 pages, 2 figures, to appear in the proceedings of "The Dark Side of the Universe", Madrid, June 2006

Country

France

Related Organizations

Sorbonne University
France
UNIVERSITE PARIS DESCARTES
France
Paris Observatory
France
French National Centre for Scientific Research
France
University of Paris
France

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Keywords

[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph], High Energy Physics - Phenomenology, High Energy Physics - Phenomenology (hep-ph), [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics (astro-ph), FOS: Physical sciences, [SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph], Astrophysics

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