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

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

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..30..225n&link_type=abstract

Astrophysics and Space Science, Volume 30, Issue 1, pp.225-231

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

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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