Published May 2006
| Version v1
Journal article
Spin flavor precession and solar neutrino data
Creators
- 1. Departamento de Fisica Centro de Investigacion y de Estudios Avanzados del IPN, A. P. 14-740 Mexico 07000 D F (Mexico)
Description
The current status of spin flavor precession (SFP) in the Sun is reviewed. It is shown that this mechanism is disfavored as a leading solution to the solar neutrino problem. The case of SFP as a sub-leading solution is also discussed. For this case, the recent KamLAND constraint on solar anti-neutrino flux provides a stringent constraint on the neutrino magnetic moment down to μν ≤ few x 10-12
Availability note (English)
Available online at http://stacks.iop.org/1742-6596/37/121/jpconf6_37_020.pdf or at the Web site for the Journal of Physics. Conference Series (Online) (ISSN 1742-6596) http://www.iop.org/Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 37
- Journal Issue
- 1
- Journal Page Range
- p. 121-126
- ISSN
- 1742-6596
Conference
- Title
- 9. Mexican workshop on particles and fields
- Dates
- 17-22 Nov 2003
- Place
- Colima (Mexico)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38028601
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- FLAVOR MODEL; MAGNETIC MOMENTS; MUON NEUTRINOS; PRECESSION; SOLAR NEUTRINOS; SPIN; SUN
- Descriptors DEC
- ANGULAR MOMENTUM; COMPOSITE MODELS; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MAIN SEQUENCE STARS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NEUTRINOS; PARTICLE MODELS; PARTICLE PROPERTIES; QUARK MODEL; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STARS; STELLAR RADIATION