Published April 1, 2003
| Version v1
Journal article
Solar neutrino oscillations and indications of matter effects in the Sun
Creators
- 1. Dipartimento di Fisica and Sezione INFN di Bari Via Amendola 173, 70126 Bari (Italy)
Description
Assuming the current best-fit solutions to the solar neutrino problem at large mixing angle, we briefly illustrate how prospective data from the Sudbury Neutrino Observatory (SNO) and from the Kamioka Liquid Scintillator Antineutrino Detector (KamLAND) can increase our confidence in the occurrence of standard matter effects on active neutrino flavor oscillations in the Sun, which are starting to emerge from current data
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.67.073001;
- arXiv
- arXiv:hep-ph/0211414v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 67
- Journal Issue
- 7
- Journal Page Range
- p. 073001-073001.6
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35075430
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- ANTINEUTRINOS; FLAVOR MODEL; NEUTRINO DETECTION; NEUTRINO OSCILLATION; SOLAR NEUTRINOS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; COMPOSITE MODELS; DETECTION; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MATTER; NEUTRINOS; PARTICLE MODELS; QUARK MODEL; RADIATION DETECTION; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION
Optional Information
- Notes
- (c) 2003 The American Physical Society