Supersonic turbulent stress and the solar neutrino flux

Details Supersonic turbulent stress and the solar neutrino flux Supersonic turbulent stress and the solar neutrino flux

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974pasau...2..263p&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 8th, Hobart, Australia, May 22-24, 1974.) Astronomical Society of Au

Astronomy and Astrophysics

Astronomy

Astronomical Models, Neutrinos, Nuclear Fusion, Solar Corpuscular Radiation, Turbulence Effects, Abundance, Solar Flux, Stellar Evolution, Stellar Structure, Supersonic Flow

Scientific paper

An investigation conducted by Prentice (1973) concerning a relation between a small burnt out solar central core and a low neutrino flux is considered. It is demonstrated that supersonic turbulence within a metal-rich burning central convective core provides the necessary physical mechanism required for obtaining the conditions suitable for a low neutrino flux after 4.7 billion years of nuclear evolution.

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