Published June 2007
| Version v1
Journal article
High Energy Astroparticle Physics
Creators
- 1. APC - AstroParticules et Cosmologie, 10, rue Alice Domon et Lonie Duquet, 75205 Paris Cedex 13 (France) and Institut d'Astrophysique de Paris, 98bis Boulevard Arago, 75014 Paris (France)
Description
We give a brief (and highly incomplete) overview of the current experimental and theoretical status of high energy cosmic rays and their secondary γ-rays and neutrinos. We focus on the role of large scale magnetic fields and on multi-messenger aspects linking these three channels. We also recall that the flavor composition of neutrino fluxes from astrophysical sources contains information on both the source conditions and neutrino physics
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2007.02.081;
- arXiv
- arXiv:astro-ph/0612240v1;
- PII
- S0920-5632(07)00149-1;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 168
- Journal Page Range
- p. 219-224
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- Neutrino oscillation workshop
- Dates
- 9-15 Sep 2006
- Place
- Conca Specchiulla, Otranto (Italy)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39080571
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COSMIC RADIATION; COSMIC RADIO SOURCES; CURRENTS; FLAVOR MODEL; GAMMA RADIATION; MAGNETIC FIELDS; NEUTRINOS
- Descriptors DEC
- COMPOSITE MODELS; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; PARTICLE MODELS; PHYSICS; QUARK MODEL; RADIATIONS
Optional Information
- Copyright
- Copyright (c) 2007 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.