Quotes:
“There is no perfect solar model.”
“standard model is good, but not perfect.”
Selected References
1. Basu S, Dappen W, Nayfonov A. Helioseismic analysis of the hydrogen partition function in the solar interior. Astrophys J 1999;518(2):985-93.
2. Christensendalsgaard J, Dappen W. Solar oscillations and the equation of state. Astronomy and Astrophysics Review 1992;4(3):267-361.
3. Dappen W, Mihalas D, Hummer DG, Mihalas BW. The equation of state for stellar envelopes .3. thermodynamic quantities. Astrophys J 1988;332(1):261,&.
4. Elliott JR, Kosovichev AG. The adiabatic exponent in the solar core. Astrophys J 1998;500(2):L199-202.
5. Gough DO, Kosovichev AG, Toomre J, Anderson E, Antia HM, Basu S, Chaboyer B, Chitre SM, ChristensenDalsgaard J, Dziembowski WA, EffDarwich A, Elliott JR, Giles PM, Goode PR, Guzik JA, Harvey JW, Hill F, Leibacher JW, Monteiro MJPFG, Richard O, Sekii T, Shibahashi T, Takata M, Thompson MJ, Vauclair S, Vorontsov SV. The seismic structure of the sun. Science 1996;272(5266):1296-300.
6. Hummer DG, Mihalas D. The equation of state for stellar envelopes .1. an occupation probability formalism for the truncation of internal partition-functions. Astrophys J 1988;331(2):794-814.
7. Mihalas D, Dappen W, Hummer DG. The equation of state for stellar envelopes .2. algorithm and selected results. Astrophys J 1988;331(2):815-25.