학술논문

Production of high energy neutrinos in relativistic supernova shock waves
Document Type
Conference
Author
Source
Conference: 1978 DUMAD summer workshop, San Diego, CA, USA, 11 Aug 1978
Subject
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COSMIC NEUTRINOS
PARTICLE PRODUCTION
SUPERNOVAE
SHOCK WAVES
GEV RANGE 10-100
GEV RANGE 100-1000
ISOLATED VALUES
RELATIVISTIC RANGE
TEV RANGE
THEORETICAL DATA
WHITE DWARF STARS
COSMIC RADIATION
DATA
DATA FORMS
DWARF STARS
ELEMENTARY PARTICLES
ENERGY RANGE
ERUPTIVE VARIABLE STARS
FERMIONS
GEV RANGE
INFORMATION
INTERACTIONS
IONIZING RADIATIONS
LEPTONS
MASSLESS PARTICLES
NEUTRINOS
NUMERICAL DATA
PARTICLE INTERACTIONS
RADIATIONS
STARS
VARIABLE STARS 640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar, Radio & X-Ray Sources
Language
English
Abstract
The possibility of producing high-energy neutrinos (> approx. 10 GeV) in relativistic supernova shock waves is considered. It is shown that, even if the dissipation in such shocks is due to hard hadron--hadron collisions, the resulting flux of neutrinos is too small to be observed by currently envisioned detectors. The associated burst of hard ..gamma..-rays, however, may be detectable. 3 tables.