Resonant Spin-Flavour Precession and Solar Neutrino Problem (第11回山陽サマ-・インスティチュ-ト)
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概要
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The energy spectrum of v_e survival probability in the Resonant Spin-Flavor Precession(RSFP) scenario is shown to have a desirable shape to explain the deficit of solar neutrinos. As the result, the RSFP scenario is argued to have rather broad allowed region to reconcile all the data of three kinds of solar neutrino experiments.
- 素粒子論グループ 素粒子研究編集部の論文
- 1996-01-20
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関連論文
- Effective Action Approach to Heavy Particle Contributions and Wilsonian Renormalization
- Resonant Spin-Flavour Precession and Solar Neutrino Problem (第11回山陽サマ-・インスティチュ-ト)
- Quaternionic Approach to Gauge Theories with Extra Generations and CP Violation