Published April 2013 | Version v1
Journal article

Ultrahigh energy cosmic ray fluxes and cosmogenic neutrinos

Creators

Description

We discuss the possible origin of the two neutrino shower events reported by the IceCube Collaboration at the Neutrino 2012 conference in Kyoto, Japan. The suspicion early on was that these two events are due to cosmogenic neutrinos and possibly by electron antineutrinos generating the Glashow resonance. The difference of the energy of the W− in the resonance and the energy estimates of the detected cascade events makes this assumption unlikely. The conclusion then may be that these high energy neutrinos are produced at sources of high energy cosmic rays such as Active Galactic Nuclei

Availability note (English)

Available from http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.095

Additional details

Identifiers

DOI
10.1016/j.nuclphysbps.2013.04.095;
PII
S0920-5632(13)00216-8;

Publishing Information

Journal Title
Nuclear Physics. B, Proceedings Supplements
Journal Volume
237-238
Journal Page Range
p. 233-235
ISSN
0920-5632
CODEN
NPBSE7

Conference

Title
Neutrino oscillation workshop
Dates
9-15 Sep 2012
Place
Conca Specchiulla, Otranto (Italy)

INIS

Country of Publication
Netherlands
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
45065591
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COSMIC RADIATION; COSMIC RAY FLUX; CROSS SECTIONS; ELECTRON ANTINEUTRINOS; GALAXY NUCLEI; ORIGIN; SHOWERS
Descriptors DEC
ANTILEPTONS; ANTIMATTER; ANTINEUTRINOS; ANTIPARTICLES; ELECTRON NEUTRINOS; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; NEUTRINOS; RADIATION FLUX; RADIATIONS

Optional Information

Copyright
Copyright (c) 2013 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.