Published March 2016
| Version v1
Journal article
Common origin of the high energy astronomical gamma rays, neutrinos and cosmic ray positrons?
Description
We show that the observed fluxes, spectra and sky distributions of the high energy astronomical neutrinos, gamma rays and cosmic ray positrons satisfy the simple relations expected from their common production in hadronic collisions in/near source of high energy cosmic rays with diffuse matter.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.jheap.2015.12.001Additional details
Identifiers
- DOI
- 10.1016/j.jheap.2015.12.001;
- PII
- S221440481500066X;
Publishing Information
- Journal Title
- Journal of High Energy Astrophysics (Print)
- Journal Volume
- 9
- Journal Page Range
- p. 9-15
- ISSN
- 2214-4048
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51081278
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIATION; GAMMA RADIATION; HADRONS; NEUTRINOS; NONLUMINOUS MATTER; ORIGIN; POSITRONS; SKY; SPECTRA
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; RADIATIONS
Optional Information
- Copyright
- Copyright (c) 2015 Elsevier B.V.