Published September 1985
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Astrophysical and terrestrial neutrinos in Supernova detectors
Description
Supernova (SN) explosions are the place of very fundamental phenomena, whose privileged messengers are neutrinos. But such events are very rare. Then, SN detection has to be combined with other purposes. The recent developments of SN detectors have been associated with developments of underground particle physics (proton decay, monopoles ...). But here, I will restrict myself to discuss the possibilities for a supernova detector to be sensitive to other sources of neutrinos, astrophysical or terrestrial
Availability note (English)
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17075525.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 18 p.
- Report number
- CEA-CONF--8404
Conference
- Title
- National congress of the Societe Francaise de Physique.
- Dates
- 9-13 Sep 1985.
- Place
- Nice (France).
INIS
- Country of Publication
- France
- Country of Input or Organization
- France
- INIS RN
- 17075525
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANTINEUTRINOS; COSMIC NEUTRINOS; ELECTRON NEUTRINOS; MUON NEUTRINOS; NEUTRINO DETECTION; NEUTRINO OSCILLATION; SOLAR NEUTRINOS; SUPERNOVAE
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; BINARY STARS; COSMIC RADIATION; DETECTION; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; MATTER; NEUTRINOS; RADIATION DETECTION; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STARS; STELLAR RADIATION; VARIABLE STARS