A redetermination of the neutrino mass-squared difference in tri-maximal mixing with terrestrial matter effects
Description
We re-fit for the neutrino mass-squared difference Δm2 in the threefold maximal (i.e. tri-maximal) mixing scenario using recent CHOOZ and SUPER-K data, taking account of matter effects in the Earth. While matter effects have little influence on reactor experiments and proposed long-baseline accelerator experiments with L < or ∼ 1000 km, they are highly significant for atmospheric experiments, suppressing naturally νe mixing and enhancing νμ - ντ mixing, so as to effectively remove the experimental distinction between threefold maximal and twofold maximal νμ - ντ mixing. Threefold maximal mixing is fully consistent with the CHOOZ and SUPER-K data and the best-fit value for the neutrino mass-squared difference is Δm2 ∼ (0.98 ± 0.230.30) x 10-3 eV2. (author)
Availability note (English)
Available from British Library Document Supply Centre- DSC:8715.1804(99-026)Additional details
Publishing Information
- Imprint Pagination
- 27 p.
- Journal Issue
- no.99-026
- Series
- Technical report
- ISSN
- 1358-6254
- Report number
- CLRC-RAL-TR--1999-026
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 30035066
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Non-conventional Literature
- Descriptors DEI
- COSMIC NEUTRINOS; ELECTRON NEUTRINOS; MASS; MIXING RATIO; MUON NEUTRINOS; NEUTRINO DETECTION; SOLAR NEUTRINOS
- Descriptors DEC
- COSMIC RADIATION; DETECTION; ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; NEUTRINOS; RADIATION DETECTION; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION