The effect of primordial hydrogen/helium fractionation on the solar neutrino flux

Details The effect of primordial hydrogen/helium fractionation on the solar neutrino flux The effect of primordial hydrogen/helium fractionation on the solar neutrino flux

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...196..601w&link_type=abstract

Astrophysical Journal, vol. 196, Mar. 1, 1975, pt. 1, p. 601-605. NSF-NASA-supported research.

Astronomy and Astrophysics

Astrophysics

12

Helium, Hydrogen, Neutrinos, Solar Flux, Stellar Evolution, Astronomical Models, Fractionation, Particle Flux Density, Solubility, Stellar Envelopes, Stellar Structure

Scientific paper

If hydrogen and helium are immiscible below some critical temperature,
gravitational separation could occur in the proto-sun, resulting in a
nearly pure helium core and a nearly pure hydrogen shell. We have
constructed solar models according to this scenario and find the
neutrino flux reduced to 1.5-3 SNU.

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