Standard solar models with CESAM code - Neutrinos and helioseismology

Details Standard solar models with CESAM code - Neutrinos and helioseismology Standard solar models with CESAM code - Neutrinos and helioseismology

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...268..775b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 268, no. 2, p. 775-791.

Astronomy and Astrophysics

Astronomy

67

Astronomical Models, Computer Programs, Helioseismology, Solar Neutrinos, Stellar Evolution, Abundance, Computerized Simulation, Equations Of State, Opacity, P Waves, Solar Convection (Astronomy), Thermonuclear Reactions

Scientific paper

A new code for stellar evolution named CESAM has been constructed and standard solar models have been computed using it. Their global characteristics, predicted capture rates of neutrinos for the chlorine and gallium experiments, and their seismological properties are given and compared to the observational constraints. The emphasis is put on the effect of the recent opacities of Livermore for different mixtures, corresponding to recent abundances determination, and on the neutrino predictions and solar oscillations.

Affiliated with

Also associated with

No associations

Rating

Standard solar models with CESAM code - Neutrinos and helioseismology 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 Standard solar models with CESAM code - Neutrinos and helioseismology, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Standard solar models with CESAM code - Neutrinos and helioseismology will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1271855