Published August 1991
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E sub 6 leptoquarks and the solar neutrino problem
Description
The possibility that non-conventional neutrino oscillations take place in the superstring inspired E sub 6 models is considered. In this context, the influence of leptoquark mediated interactions of the neutrinos with nucleons in the resonant flavor conversion is discussed. It is shown that this effect can be significant for v sub e - v sub tau oscillations if these neutrinos have masses required in the ordinary Mikheyev-Smirnov-Wolfenstein (MSW) effect, and may lead to a solution of the solar neutrino problem even in the absence of vacuum mixings. On the other hand, this model cannot lead to a resonant behavior in the sun if the neutrinos are massless
Availability note (English)
MF available from INIS under the Report Number; NTIS HC/MF A02; INIS.
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Additional details
Publishing Information
- Imprint Pagination
- 7 p.
- Report number
- N--92-11956
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 23040791
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- FLAVOR; LEPTONS; NUCLEONS; OSCILLATIONS; PARTICLE INTERACTIONS; QUARKS; SOLAR NEUTRINOS; STRING MODELS; THEORETICAL DATA
- Descriptors DEC
- BARYONS; DATA; ELEMENTARY PARTICLES; EXTENDED PARTICLE MODEL; FERMIONS; HADRONS; INFORMATION; INTERACTIONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NEUTRINOS; NUMERICAL DATA; ORGANOLEPTIC PROPERTIES; PARTICLE MODELS; POSTULATED PARTICLES; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION
Optional Information
- Contract/Grant/Project number
- Contract NAGW-1340
- Secondary number(s)
- NASA-CR--189005; NAS--1.26:189005; FERMILAB-PUB--91/206-A.