Published 1993 | Version v1
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Solar neutrino oscillations

Creators

Description

The special properties of solar neutrinos that render this flux so uniquely important in searches for neutrino masses and flavor mixing are reviewed. The effects of matter, including density fluctuations and turbulence, on solar neutrino oscillations are explained through analogies with more familiar atomic physics phenomena

Availability note (English)

MF available from INIS under the Report Number; Also available from OSTI as DE94007265; NTIS; US Govt. Printing Office Dep.

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Additional details

Publishing Information

Imprint Pagination
12 p.
Report number
DOE/ER/40561--115

Conference

Title
International symposium on nuclear structure physics today.
Dates
11-14 May 1993.
Place
Taiwan (China).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
25053603
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
FLUCTUATIONS; MASS; NEUTRINO OSCILLATION; PARTICLE PROPERTIES; SOLAR NEUTRINOS
Descriptors DEC
ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; NEUTRINOS; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION; VARIATIONS

Optional Information

Contract/Grant/Project number
Contract FG06-90ER40561; Grant NAGW-2523
Funding organization
USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States).
Secondary number(s)
CONF-9305293--4.