MSW Oscillations: LMA and Subdominant Effects - INSPIRE

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MSW Oscillations: LMA and Subdominant Effects

Alexander Friedland
(
- Los Alamos
)

Dec, 2006

8 pages

Part of Neutrino physics and astrophysics. Proceedings, 22nd International Conference, Neutrino 2006, Santa Fe, USA, June 13-19, 2006

Published in:

Nucl.Phys.B Proc.Suppl. 221 (2011) 79-84

Contribution to:

- Neutrino 2006

e-Print:

hep-ph/0612266 [hep-ph]

DOI:

10.1016/j.nuclphysbps.2011.03.098

Report number:

LA-UR-06-6774

View in:

ADS Abstract Service

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Abstract:

New physics near the TeV scale could modify neutrino-matter interactions or generate a relatively large neutrino magnetic (transition) moment. Both types of effects have been discussed since the 1970's as alternatives to mass-induced neutrino flavor oscillations. Nowadays, the availability of high-statistics data makes it possible to turn the idea around and ask: How well do the simple mass-induced oscillations describe solar neutrinos? At what level are the above-mentioned nonstandard effects excluded? Can we use solar neutrinos to constrain physics beyond the Standard Model? These notes review the sensitivity of the present-day solar neutrino experiments to the nonstandard neutrino interactions and transition moment and outline progress that may be expected in the near future. Based on a talk given at the Neutrino 2006 conference.

Note:

8 pages, 5 figures, based on talk given at Neutrino 2006 Report-no: LA-UR-06-6774

talk: Santa Fe 2006/06/13
neutrino: solar
neutrino: oscillation
MSW effect
neutrino: interaction
neutrino: magnetic moment
magnetic moment: transition
numerical calculations: interpretation of experiments

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