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The main sequence stars and the photon-neutrino coupling theory of weak interactions

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Abstract

To test the photon-neutrino coupling theory of weak interactions as presented by Bandyopadhyay (1968), detailed models of the Main Sequence stars with neutrino emission based on this theory are computed. The models are compared with the observational data, and it is concluded that the photon-neutrino coupling theory would seem to be definitely excluded on astrophysical grounds.

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Authors and Affiliations

  1. Dept. of Physics, Kyoto University, Kyoto, Japan

    Minoru Nishida

  2. Dept. of Earth Science and Astronomy, College of General Education, University of Tokyo, Meguro-ku, Tokyo, Japan

    Atsuma Yamasaki

Authors
  1. Minoru Nishida
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  2. Atsuma Yamasaki
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Nishida, M., Yamasaki, A. The main sequence stars and the photon-neutrino coupling theory of weak interactions. Astrophys Space Sci 30, 225–231 (1974). https://doi.org/10.1007/BF00645766

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  • DOI: https://doi.org/10.1007/BF00645766

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