Solar neutrinos and turbulent diffusion

Details Solar neutrinos and turbulent diffusion Solar neutrinos and turbulent diffusion

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.290..683s&link_type=abstract

Nature, vol. 290, Apr. 23, 1981, p. 683-686.

Physics

16

Solar Neutrinos, Stellar Evolution, Stellar Rotation, Turbulent Diffusion, Helium Isotopes, Shear Flow, Stellar Interiors, Systems Stability

Scientific paper

Stellar turbulent diffusion generated by instabilities associated with shear flows in differentially rotating stars is examined. It is shown that there are observational and theoretical reasons to suspect that a slow diffusion process due to a mild turbulence is operating in stellar interiors. The consequences that turbulent diffusion may have for the solar neutrinos problem and the He-3/He-4 ratio at the solar surface, and the implications of continuing turbulent diffusion for stellar evolution, are also discussed.

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