dorsal/arxiv
View SchemaProbability of a Solution to the Solar Neutrino Problem Within the Minimal Standard Model
| Authors | Karsten M. Heeger, R. G. H. Robertson |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9610030 |
| URL | https://arxiv.org/abs/nucl-th/9610030 |
| DOI | 10.1103/PhysRevLett.77.3720 |
| Journal | Phys.Rev.Lett.77:3720-3723,1996 |
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.
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"abstract": "Tests, independent of any solar model, can be made of whether solar neutrino\nexperiments are consistent with the minimal Standard Model (stable, massless\nneutrinos). If the experimental uncertainties are correctly estimated and the\nsun is generating energy by light-element fusion in quasi-static equilibrium,\nthe probability of a standard-physics solution is less than 2%. Even when the\nluminosity constraint is abandoned, the probability is not more than 4%. The\nsensitivity of the conclusions to input parameters is explored.",
"arxiv_id": "nucl-th/9610030",
"authors": [
"Karsten M. Heeger",
"R. G. H. Robertson"
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"doi": "10.1103/PhysRevLett.77.3720",
"journal_ref": "Phys.Rev.Lett.77:3720-3723,1996",
"title": "Probability of a Solution to the Solar Neutrino Problem Within the Minimal Standard Model",
"url": "https://arxiv.org/abs/nucl-th/9610030"
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