An explanation for the solar neutrino problem

Details An explanation for the solar neutrino problem An explanation for the solar neutrino problem

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..140..203h&link_type=abstract

Solar Physics, Volume 140, Issue 1, pp.203-206

Physics

Scientific paper

A new mechanism of thermonuclear reaction is briefly introduced. It shows that a certain amount of thermonuclear reaction can take place in dense, low-temperature (T < 1 × 105 K) plasmas. At a super-high temperature, it is in agreement with the old thermonuclear reaction mechanism first presented by Gamow and Bethe. As most regions in the Sun are at moderate and low temperature, a sufficient amount of fusion energy is generated therein. Therefore the solar central temperature in standard models must be decreased to about 13.8 × 106 K. That would make the flux of high-energy neutrinos conform with the observational results.

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