Probability of a Solution to the Solar Neutrino Problem Within the Minimal Standard Model
arXiv:nucl-th/9610030 · doi:10.1103/PhysRevLett.77.3720
Abstract
Tests, independent of any solar model, can be made of whether solar neutrino experiments are consistent with the minimal Standard Model (stable, massless neutrinos). If the experimental uncertainties are correctly estimated and the sun is generating energy by light-element fusion in quasi-static equilibrium, the probability of a standard-physics solution is less than 2%. Even when the luminosity constraint is abandoned, the probability is not more than 4%. The sensitivity of the conclusions to input parameters is explored.
PRL, Revtex, 1 figure, 5 pages
References in corpus (20)
- Solar Models with Helium and Heavy Element Diffusion
- Solar Neutrinos: Radiative Corrections in Neutrino-Electron Scattering Experiments
- Standard Neutrino Spectrum from B-8 Decay
- Solar Model Uncertainties, MSW Analysis, and Future Solar Neutrino Experiments
- Astrophysical Solutions are Incompatible with the Solar Neutrino Data
- How Many Solar Neutrino Experiments Are Wrong?
- On The Vacuum Oscillation Solution of The Solar Neutrino Problem
- Implication of Combined Solar Neutrino Observation and their Theoretical Uncertainties
- The Temperature Dependence of Solar Neutrino Fluxes
- New Constraints on Neutrino Oscillations in Vacuum as a Possible Solution of the Solar Neutrino Problem
- How Well Do We (and Will We) Know Solar Neutrino Fluxes and Oscillation Parameters?
- Model Independent Determination of the Solar Neutrino Spectrum with and without MSW
- Neutrinos from the Sun: experimental results confronted with solar models
- Status of the Solar Neutrino Puzzle
- Semi-Empirical Bound on the Chlorinr-37 Solar Neutrino Experiment
- Implications of the GALLEX Source Experiment for the Solar Neutrino Problem
- Last Hope for an astrophysical solution to the solar neutrino problem
- On Solar Model Solutions to the Solar Neutrino Problem
- Treating Solar Model Uncertainties: A Consistent Statistical Analysis of Solar Neutrino Models and Data
- How Does the Sun Shine?
Cited by in corpus (33)
- Solar Fusion Cross Sections
- Measurement of the solar neutrino capture rate with gallium metal
- Nuclear weak-interaction processes in stars
- Helioseismology and Solar Abundances
- Where do we stand with solar neutrino oscillations?
- Neutrino Masses and Mixing: Evidence and Implications
- Phenomenology of Neutrino Oscillations
- Measurement of the response of a gallium metal solar neutrino experiment to neutrinos from a 51Cr source
- Solar Neutrinos: Status and Prospects
- Global Seismology of the Sun
- Solutions to Solar Neutrino Anomaly
- Measurement of the and Total B Solar Neutrino Fluxes with the Sudbury Neutrino Observatory Phase I Data Set
- Is Large Mixing Angle MSW the Solution of the Solar Neutrino Problems?
- Unknowns after the SNO Charged-Current Measurement
- The luminosity constraint on solar neutrino fluxes
- Does the Sun Appear Brighter at Night in Neutrinos?
- The Salpeter plasma correction for solar fusion reactions
- He Transport in the Sun and the Solar Neutrino Problem
- What will the first year of SNO show?
- Anomalous diffusion modifies solar neutrino fluxes
- How many sigmas is the solar neutrino effect?
- Potential for Precision Measurement of Solar Neutrino Luminosity by HERON
- Neutrino Oscillations
- Current Status of the Solar Neutrino Problem with Super-Kamiokande
- Solar Neutrinos
- Another Look at Just-So Solar Neutrino Oscillations
- Solar Neutrinos: Where We Are, What We Need
- Possible Tomography of the Sun's Magnetic Field with Solar Neutrinos
- Neutrino Magnetic Moment Upper Bound From Solar Neutrino Observations
- A Measurement of Gamow-Teller Strength for 176Yb -> 176Lu and the Efficiency of a Solar Neutrino Detector
- An analytic solution of the Boltzmann equation in the presence of self-generated magnetic fields in astrophysical plasmas
- Solar Neutrino Results from the Sudbury Neutrino Observatory
- Neutrino Magnetic Moment and Solar Neutrino Experiments