Published December 2011 | Version v1
Journal article

MSW Oscillations - LMA and Subdominant Effects

  • 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.2011.03.098

Additional 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.