A Classical Solution for the Solar Neutrino Puzzle

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概要

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• If the mixture of hydrogen and iron is hot enough for an almost complete ionization of iron, and at the same time it is cool and dense enough to produce electron inhomogenities around the iron ions, then Debye-Huckel approximation predicts separation of an iron-rich phase from the hydrogen-rich phase. The necessary conditions are fulfilled for most of the solar interior. Precipitation of iron reduces the opacity, decreases the central temperature and suppresses the solar flux of energetic neutrinos. For chlorine target, the estimated neutrino signal is decreased with respect to the standard model considerably, for gallium target it remains practically unchanged.

• 理論物理学刊行会の論文
• 1987-01-25

著者

• Ruff Imre

  Research Group For Theoretical Chemistry Eotvos University

• DEARBORN David

  Lawrence Livermore Laboratory, University of California

• MARX George

  Research Institute for Fundamental Physics, Kyoto University

• Marx George

  Research Institute For Fundamental Physics Kyoto University

• Dearborn David

  Lawrence Livermore Laboratory University Of California

関連論文

• A Classical Solution for the Solar Neutrino Puzzle

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