Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...408..347t&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 408, no. 1, p. 347-367.
Astronomy and Astrophysics
Astrophysics
216
Helioseismology, Nuclear Astrophysics, Solar Interior, Solar Neutrinos, Stellar Models, Solar Oscillations, Stellar Evolution, Stellar Structure
Scientific paper
This paper focuses mainly on the neutrino puzzle and discusses the point of view that neutrinos and helioseismology are two complementary probes of the solar interior. We first analyze the physical differences noticed between already published solar models and their consequences for neutrino predictions. We propose new results on the solar neutrino predictions and acoustic mode frequencies for l = 0-150, in the classical framework of stellar evolution. We quantify the influence of precise composition, nuclear reaction rates, screening effect, and opacity calculations on both neutrino and acoustic mode frequency predictions. Our present predictions are 6.4 +/- 1.4 SNU for the chlorine experiment, 4.4 +/- 1.1 x 10 exp 6/sq cm/s for the water detector, and 122.5 +/- 7 SNU for the gallium detector.
Lopes Ilidio
Turck-Chieze Sylvaine
No associations
LandOfFree
Toward a unified classical model of the sun - On the sensitivity of neutrinos and helioseismology to the microscopic physics 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 Toward a unified classical model of the sun - On the sensitivity of neutrinos and helioseismology to the microscopic physics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Toward a unified classical model of the sun - On the sensitivity of neutrinos and helioseismology to the microscopic physics will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1852339