Robustness of solar neutrino oscillations in the presence of non-standard physics

2007 ◽  
Author(s):  
O. G. Miranda ◽  
M. A. Tórtola ◽  
J. W. F. Valle
Keyword(s):  
Solar Neutrino ◽  
Neutrino Oscillations

Solar neutrino oscillations from superstrings

1986 ◽  
Vol 177 (1) ◽  
pp. 47-50 ◽  
Author(s):  
R.N. Mohapatra ◽  
J.W.F. Valle
Keyword(s):  
Solar Neutrino ◽  
Neutrino Oscillations

scholarly journals Solar Neutrino Projects

1990 ◽  
Vol 121 ◽  
pp. 157-169
Author(s):  
M. Spiro ◽  
D. Vignaud
Keyword(s):  
Heavy Water ◽  
Solar Neutrino ◽  
Neutrino Oscillations ◽  
Neutrino Flux ◽  
The Sun ◽  
Solar Neutrino Problem ◽  
Wide Range ◽  
Different Sources

AbstractAn overview of the solar neutrino projects is given, with an emphasis on the complementarity of the different experiments (gallium, indium, heavy water,...) to solve the solar neutrino problem that was raised by the chlorine and the Kamiokande results. The separation of the different sources of neutrinos in the Sun would contribute significantly to the astrophysical understanding of the Sun. Some of the planned experiments could be able to pinpoint neutrino oscillations (within a wide range of parameters) almost independently of solar models. Projects which are particularly sensitive to a variation of the neutrino flux with time are also discussed.

scholarly journals Neutrino Masses, Neutrino Oscillations and Dark Matter

1990 ◽  
Vol 121 ◽  
pp. 213-230
Author(s):  
Haim Harari
Keyword(s):  
Dark Matter ◽  
Solar Neutrino ◽  
Neutrino Oscillations ◽  
Mass Range ◽  
Neutrino Masses ◽  
Direct Measurements ◽  
Theoretical Considerations

AbstractWe discuss bounds on neutrino masses using an analysis based on direct measurements, cosmological bounds, oscillation experiments, the solar neutrino puzzle and theoretical considerations on neutrino decays. We present four possible solutions for the mass range of the three neutrino flavors. We outline experiments which can distinguish among these solutions and discuss their implications for the cosmological dark matter problem.

Realistic calculations of solar-neutrino oscillations

1981 ◽  
Vol 24 (2) ◽  
pp. 538-541 ◽  
Author(s):  
V. Barger ◽  
K. Whisnant ◽  
R. J. N. Phillips
Keyword(s):  
Solar Neutrino ◽  
Neutrino Oscillations

scholarly journals CONCLUDING REMARKS

2002 ◽  
Vol 17 (24) ◽  
pp. 3500-3508 ◽  
Author(s):  
NICOLA CABIBBO
Keyword(s):  
Cp Violation ◽  
Standard Model ◽  
Theoretical Prediction ◽  
Decay Mode ◽  
Solar Neutrino ◽  
Neutrino Oscillations ◽  
Expected Value ◽  
Sudbury Neutrino Observatory ◽  
The Standard Model ◽  
First Results

Important new results have been presented at this conference. The direct violation of CP in K0 → π + π has been firmly established in two independent experiments, NA48 at CERN and KTeV at Fermilab. Both Babar at SLAC and Belle at Kek have determined the CP violation in [Formula: see text] oscillations through the study of the golden KS + Ψ decay mode. The observed CP violation agrees with the expectations of the Standard model, based on the quark-mixing phenomenon. The first results of the Sudbury Neutrino Observatory, SNO, suggest that the long-lasting solar neutrino puzzle has been finally solved in terms of neutrino oscillations. Results appeared after the conference which modify the theoretical prediction of the muon anomaly. This new result, if confirmed, would drastically reduce the significance of the discrepancy between the theoretically expected value for the muon anomaly and the recent results of the Brookhaven experiment.

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