MSW Oscillations - LMA and Subdominant Effects
Creators
- 1. Theoretical Division, T-8, MS B285, Los Alamos National Laboratory, Los Alamos, NM 87545 (United States)
Description
These notes, based on a talk given at the Neutrino 2006 conference [Neutrino 2006, Santa Fe, New Mexico, USA, (http://neutrinosantafe06.com/)], review the sensitivity of solar neutrinos to certain types of new physics, namely modifications of neutrino-matter interactions by the exchange of a new heavy particle and a large neutrino transition moment. Both were first proposed in the 1970's as possible explanations for the solar neutrino "problem" and were actively investigated for many years. While since ruled out as the dominant mechanisms of the solar neutrino flavor conversion, they remain of great interest as subdominant effects, which, if observed, would open a window to new physics. We outline the sensitivity of the current experiments and describe progress that may be expected in the near future.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.nuclphysbps.2011.03.098Additional details
Identifiers
- DOI
- 10.1016/j.nuclphysbps.2011.03.098;
- PII
- S0920-5632(11)00166-6;
Publishing Information
- Journal Title
- Nuclear Physics. B, Proceedings Supplements
- Journal Volume
- 221
- Journal Page Range
- p. 79-84
- ISSN
- 0920-5632
- CODEN
- NPBSE7
Conference
- Title
- 22. international conference on neutrino physics and astrophysics
- Dates
- 13-19 Jun 2006
- Place
- Santa Fe, NM (United States)
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43112483
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CONVERSION; FLAVOR MODEL; INTERACTIONS; MODIFICATIONS; OSCILLATIONS; SENSITIVITY; SOLAR NEUTRINOS
- Descriptors DEC
- COMPOSITE MODELS; 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) 2011 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.