A New Solution of the Solar Neutrino Problem : Astrophysics and Relativity
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概要
- 論文の詳細を見る
We report a new solution to explain the observed deficit of the solar neutrino flux by Homestake, Kamiokande II and III, GALLEX and SAGE experiments. We use the matter mixing and the helicity oscillation in the twisting magnetic fields in the sun. Our model predicts the short (seasonal) and long (11 years) time variations of the solar neutrino flux. Three kinds of data observed by Homestake, Kamiokande, GALLEX and SAGE detectors are reproduced well if the mixing angle and the squared mass difference are in the small area around sin^22θ≃0.01 and Δm^2≃1.3 ×10^<-8> eV^2.
- 理論物理学刊行会の論文
- 1994-10-25
著者
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Takasugi E
Osaka Univ.
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Ohta Kazutoshi
Department Of Surgery Ohta Nishinouchi General Hospital
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Ohta Kazutoshi
Department Of Physics Graduate School Of Science Osaka University
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Ohta Kazutoshi
Department Of Physics Osaka University
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TAKASUGI Eiichi
Department of Physics, Osaka University
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Takasugi Eiichi
Department Of Physics Graduate School Of Science Osaka University
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TAKASUGI Eiichi
Department of Physics, Osaka University:Department of Physics, Hokkaido University
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TAKASUGI Eiichi
Institute of Physics, College of General Education, Osaka University
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Ohta Kohichi
Department of Physics, Osaka University
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