MSW Interpretation of Solar Neutrino Data
- Original Mikheyev-Smirnov-Wolfenstein
articles
- Recent MSW
calculations
- MSW plots
-
MSW solutions for the
Bahcall-Pinsonneault SSM, 7/94, updated from
[ref].
(postscript file, 28K)
-
MSW solutions with different confidence levels, 7/94, updated from
[ref].
(postscript file, 23K)
-
MSW solutions for the
Turck-Chieze-Lopes SSM, 7/94, updated from
[ref].
(postscript file, 26K)
-
MSW solutions for sterile neutrinos, 7/94, updated from
[ref].
(postscript file, 23K)
-
MSW solutions for cool sun models with the core temperature
Tc left as a free parameter, 7/94, updated from
[ref].
(postscript file, 21K).
One obtains simultaneously Tc = 1.00 pm 0.03, relative to the
BP SSM prediction .
-
MSW solutions for models in which the initial B-8
flux is left as a free parameter (e.g., due to a lower
production cross section), 7/94, updated from
[ref].
(postscript file, 18K).
One obtains simultaneously a flux of 1.15 pm 0.53, relative to the
BP SSM prediction .
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Standard Solar Model Predictions
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Current data and comparison with standard
solar model predictions
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Astrophysical/nuclear physics explanations
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References
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Main window
Naoya Hata (hata@pacific.mps.ohio-state.edu);
Paul Langacker (pgl@langacker.hep.upenn.edu)