Can solar neutrino oscillation parameters be probed at accelerators? - INSPIRE

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Can solar neutrino oscillation parameters be probed at accelerators?

J.C. Romao
(
- Lisbon, IFM
)

1993

3 pages

Published in:

Nucl.Phys.B Proc.Suppl. 31 (1993) 245-247

Contribution to:

- Neutrino 92

DOI:

10.1016/0920-5632(93)90141-R

View in:

ADS Abstract Service

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Abstract: (Elsevier)

If supersymmetry is realized with spontaneous breaking of R-parity, there will be many phenomenological consequences. Here we show that the masses and mixing angles of the neutrinos lie in the correct range for the MSW explanation of the solar neutrino problem. At the same time the rates for the processes Z 0 → τ + chargino, τ → μ + Majoron and μ → ϵ + Majoron can be close to the present bounds.

talk: Granada 1992/06/07
neutrino: solar
neutrino: oscillation
resonance: oscillation
neutrino: mass
neutrino: mixing angle
supersymmetry
R parity: spontaneously broken
Z0: cascade decay
chargino

References(19)

Figures(0)

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