Published August 1985 | Version v1
Report Metadata-only

Neutrino astronomy and the atmospheric background

Creators

Description

Some aspects of neutrino astronomy are illustrated by calculating the neutrino-induced muon flux from Cygnus X-3 binary X-ray source. The signal depends primarily on the power in cosmic rays at the source and on the distance to the source, and only relatively little on details of the matter distribution in the neighborhood of the source

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
19053708
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Numerical Data
Descriptors DEI
COSMIC MUONS; COSMIC NEUTRINOS; COSMIC X-RAY SOURCES; ENERGY SPECTRA; FLUX DENSITY; PARTICLE PRODUCTION; THEORETICAL DATA
Descriptors DEC
COSMIC RADIATION; COSMIC RAY SOURCES; DATA; ELEMENTARY PARTICLES; FERMIONS; INFORMATION; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MUONS; NEUTRINOS; NUMERICAL DATA; RADIATIONS; SECONDARY COSMIC RADIATION; SPECTRA