Solar opacities based on the ion-sphere and ion-correlation models

Details Solar opacities based on the ion-sphere and ion-correlation models Solar opacities based on the ion-sphere and ion-correlation models

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...393..409r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 393, no. 1, July 1, 1992, p. 409-413.

Astronomy and Astrophysics

Astrophysics

5

Plasma Density, Solar Interior, Solar Neutrinos, Stellar Models, Wave Functions, Debye-Huckel Theory, Ion Distribution, Opacity, Photoabsorption

Scientific paper

Solar opacities based on the ion-sphere and ion-correlation models are given for the Grevesse mixture. Uncertainties connected with these models are pointed out. Although at low densities both may be realistic, at high densities when the interionic distances are comparable with the wavelengths of the bound-state wave functions, they have to be improved. Neither can give an accurate many-body representation of the plasma, and the question of which is more realistic can be answered only by more accurate computer simulation.

Affiliated with

Also associated with

No associations

Rating

Solar opacities based on the ion-sphere and ion-correlation models 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 Solar opacities based on the ion-sphere and ion-correlation models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar opacities based on the ion-sphere and ion-correlation models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1204321