Updating Standard Solar Models
Astrophysics
2009-10-28 v1
Abstract
We present an updated version of our standard solar model (SSM) where helium and heavy elements diffusion is included and the improved OPAL equation of state (Rogers 1994, Rogers Swenson \& Iglesias 1996) is used. In such a way the EOS is consistent with the adopted opacity tables, from the same Livermore group, an occurrence which should further enhance the reliability of the model. The results for the physical characteristics and the neutrino production of our SSM are discussed and compared with previous works on the matter.
Keywords
Cite
@article{arxiv.astro-ph/9605157,
title = {Updating Standard Solar Models},
author = {F. Ciacio and S. Degl'Innocenti and B. Ricci},
journal= {arXiv preprint arXiv:astro-ph/9605157},
year = {2009}
}
Comments
compress uuencoded postscript file of 8 pages and two figures; for any problem please write to [email protected]