Published August 1985
| Version v1
Report
Energy spectra of high energy atmospheric neutrinos
Description
Focusing on high energy neutrinos ( or = 1 TeV), a new calculation of atmospheric neutrino intensities was carried out taking into account EMC effects observed in p-A collisions at accelerators, recent measurement of primary cosmic ray spectrum, and results of cosmic ray muon spectrum and charge ratio. Other features of the present calculation are (1) taking into account kinematics of three body decays of kaons and charm particles in diffusion equations and (2) taking into account energy dependence of kaon production
Additional details
Publishing Information
- Imprint Title
- Nineteenth International Cosmic Ray Conference. HE sessions, volume 8
- Journal Page Range
- vp.
- Report number
- N--85-36066
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19053705
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- CHARM PARTICLES; COSMIC KAONS; COSMIC MUONS; COSMIC NEUTRINOS; ENERGY SPECTRA; PARTICLE DECAY; PARTICLE INTERACTIONS; PARTICLE PRODUCTION; TEV RANGE 01-10; THEORETICAL DATA
- Descriptors DEC
- BOSONS; COSMIC RADIATION; DATA; DECAY; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; HADRONS; INFORMATION; INTERACTIONS; IONIZING RADIATIONS; KAONS; LEPTONS; MASSLESS PARTICLES; MESONS; MUONS; NEUTRINOS; NUMERICAL DATA; PSEUDOSCALAR MESONS; RADIATIONS; SECONDARY COSMIC RADIATION; SPECTRA; STRANGE MESONS; STRANGE PARTICLES; TEV RANGE