Effects of Magnetohydrodynamics Matter Density Fluctuations on the Solar Neutrino Resonant Spin-Flavor Precession
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| Natura: | Artículo científico |
| Lingua: | en |
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Sociedade Brasileira de Física
2000
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| _version_ | 1876441308901408768 |
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| author | N. Reggiani |
| author_facet | N. Reggiani |
| contents | Effects of Magnetohydrodynamics Matter Density Fluctuations on the Solar Neutrino Resonant Spin-Flavor Precession N. Reggiani M.M. Guzzo J.H. Colonia P.C. Holanda Física, Astronomía y Matemáticas Taking into account the stringent limits from helioseismology observations on possible matter density fluctuations described by magnetohydrodynamics theory, we find the corresponding time variations of solar neutrino survival probability due to the resonant spin-flavor precession phenomenon with amplitude of order O(10%). We discuss the physics potential of high statistics real time experiments, like as Superkamiokande, to observe the effects of such magnetohydrodynamics fluctuations on their data. We conclude that these observations could be thought as a test of the resonant spin-flavor precession solution to the solar neutrino anomaly. 2000 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46413500018 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.3 Vol.30 |
| format | Artículo científico |
| id | redalyc_46413500018 |
| institution | Redalyc |
| language | en |
| publishDate | 2000 |
| publisher | Sociedade Brasileira de Física |
| spellingShingle | Effects of Magnetohydrodynamics Matter Density Fluctuations on the Solar Neutrino Resonant Spin-Flavor Precession N. Reggiani Física, Astronomía y Matemáticas Effects of Magnetohydrodynamics Matter Density Fluctuations on the Solar Neutrino Resonant Spin-Flavor Precession N. Reggiani M.M. Guzzo J.H. Colonia P.C. Holanda Física, Astronomía y Matemáticas Taking into account the stringent limits from helioseismology observations on possible matter density fluctuations described by magnetohydrodynamics theory, we find the corresponding time variations of solar neutrino survival probability due to the resonant spin-flavor precession phenomenon with amplitude of order O(10%). We discuss the physics potential of high statistics real time experiments, like as Superkamiokande, to observe the effects of such magnetohydrodynamics fluctuations on their data. We conclude that these observations could be thought as a test of the resonant spin-flavor precession solution to the solar neutrino anomaly. 2000 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46413500018 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.3 Vol.30 |
| title | Effects of Magnetohydrodynamics Matter Density Fluctuations on the Solar Neutrino Resonant Spin-Flavor Precession |
| topic | Física, Astronomía y Matemáticas |
| url | https://www.redalyc.org/articulo.oa?id=46413500018 |