Published January 1979
| Version v1
Report
Restricted
Production of high energy neutrinos in relativistic supernova shock waves
Description
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 γ-rays, however, may be detectable. 3 tables
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS., PC A02/MF A01.
Files
Restricted
The record is publicly accessible, but files are restricted to users with access.
Additional details
Publishing Information
- Imprint Pagination
- 12 p.
- Report number
- UCRL--82152
Conference
- Title
- 1978 DUMAD summer workshop.
- Dates
- 11 Aug 1978.
- Place
- San Diego, CA, USA.
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 10485938
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- COSMIC RADIATION; GEV RANGE 10-100; GEV RANGE 100-1000; ISOLATED VALUES; NEUTRINOS; PARTICLE PRODUCTION; RELATIVISTIC RANGE; SHOCK WAVES; SUPERNOVAE; TEV RANGE; THEORETICAL DATA; WHITE DWARF STARS
- Descriptors DEC
- DATA; DATA FORMS; DWARF STARS; ELEMENTARY PARTICLES; ENERGY RANGE; ERUPTIVE VARIABLE STARS; FERMIONS; GEV RANGE; INFORMATION; INTERACTIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; NUMERICAL DATA; PARTICLE INTERACTIONS; RADIATIONS; STARS; VARIABLE STARS
Optional Information
- Secondary number(s)
- CONF-7808107--1.