Reduction of solar neutrino flux by variable Fermi coupling constant and high He-3 abundance

Details Reduction of solar neutrino flux by variable Fermi coupling constant and high He-3 abundance Reduction of solar neutrino flux by variable Fermi coupling constant and high He-3 abundance

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....35..385s&link_type=abstract

Astronomy and Astrophysics, vol. 35, no. 3, Oct. 1974, p. 385-388.

Astronomy and Astrophysics

Astrophysics

2

Abundance, Helium Isotopes, Neutrinos, Nuclear Reactions, Solar Corpuscular Radiation, Coupling, Deuterium, Entropy, Gravitational Fields, Heat Flux, Luminous Intensity, Nuclear Fusion, Relativistic Effects

Scientific paper

Two recently suggested hypotheses for the explanation of the disagreement between theory and observation of the solar neutrino flux are discussed. It is shown that the two theories - namely, the dependence of the weak interaction coupling constant on the gravitational potential and a high initial abundance of He-3 - cannot reduce the predicted neutrino flux to below the present-day upper limit.

Affiliated with

Also associated with

No associations

Rating

Reduction of solar neutrino flux by variable Fermi coupling constant and high He-3 abundance does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Reduction of solar neutrino flux by variable Fermi coupling constant and high He-3 abundance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Reduction of solar neutrino flux by variable Fermi coupling constant and high He-3 abundance will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-791251