Published June 2005
| Version v1
Journal article
Solar Neutrino Day-Night Effect
- 1. Division of Mathematical Physics, Department of physics, Royal Institute of Technology (KTH), AlbaNova University Center, SE-106 91 Stockholm (Sweden)
Description
We summarize the results of Ref. [M. Blennow, T. Ohlsson and H. Snellman, Phys. Rev. D 69 (2004) 073006, hep-ph/0311098] in which we determine the effects of three flavor mixing on the day-night asymmetry in the flux of solar neutrinos. Analytic methods are used to determine the difference in the day and night solar electron neutrino survival probabilities and numerical methods are used to determine the effect of three flavor mixing at detectors
Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2005.01.243;
- PII
- S0920-5632(05)00277-X;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 143
- Journal Page Range
- p. 578
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 21. international conference on neutrino physics and astrophysics
- Acronym
- NEUTRINO 2004
- Dates
- 14-19 Jun 2004
- Place
- Paris (France)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37109030
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASYMMETRY; ELECTRON NEUTRINOS; FLAVOR MODEL; SOLAR ELECTRONS; SOLAR NEUTRINOS
- Descriptors DEC
- COMPOSITE MODELS; ELECTRONS; ELEMENTARY PARTICLES; FERMIONS; LEPTONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; NEUTRINOS; PARTICLE MODELS; QUARK MODEL; RADIATIONS; SOLAR PARTICLES; SOLAR RADIATION; STELLAR RADIATION
Optional Information
- Copyright
- Copyright (c) 2005 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.