Supersymmetric majoron signatures and solar neutrino oscillations

Details Supersymmetric majoron signatures and solar neutrino oscillations Supersymmetric majoron signatures and solar neutrino oscillations

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvl..60..397s&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 60, Feb. 1, 1988, p. 397-400. CAICYT-supported research.

Astronomy and Astrophysics

Astrophysics

74

Gravitation Theory, Oscillations, Solar Neutrinos, Supersymmetry, Broken Symmetry, Mathematical Models, Particle Mass, Quarks, Weak Interactions (Field Theory)

Scientific paper

Spontaneous R-parity breaking in supergravity solves the solar neutrino problem through matter-enhanced neutrino oscillations. The model may be tested in collider experiments and through "dynamical" effects associated with the existence of a weakly interacting majoron. Apart from astrophysical effects, majoron emission can produce observable changes in μ and τ decay spectra for parameter values that substantially reduce the solar neutrino flux. A signature of the model is the possible observation of the decay μ → e+ majoron.

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