Modeling pressure-ionization of hydrogen in the context of astrophysics

High Pressure Research

Volumn 16, Issue 5-6, 2000, Pages 331-343

  Saumon, D ^a   Chabrier, G ^b   Wagner, D J ^c   Xie, X ^d  

^a VANDERBILT UNIVERSITY   (United States)

^b UNIVERSITÉ DE LYON   (France)

^c RENSSELAER POLYTECHNIC INSTITUTE   (United States)

^d INTEL CORPORATION   (United States)

Author keywords

Effective potentials; Equation of state; Hydrogen; Plasma phase transition; Pressure ionization

Indexed keywords

EID: 0001378383     PISSN: 08957959     EISSN: None     Source Type: Journal    
DOI: 10.1080/08957950008201434     Document Type: Article

References (30)

1. Holmes, N. C., Ross, M. and Nellis, W. J. (1995). Phys. Rev. B, 52, 15835.
2. Celliers, P. M., Collins, G. W., Da Silva, L. B., Gold, D. M., Cauble, R., Wallace, R. J. and Foord, M. E. (1999). Submitted to Phys. Rev. Letters.
3. Weir, S. T., Mitchell, A. C. and Nellis, W. J. (1996). Phys. Rev. Lett., 76, 1860.
4. Da Silva, L. B. et al. (1997). Phys. Rev. Lett., 78, 483.
5. Collins, G. W. et al. (1998). Science, 281, 1178.
6. Guillot, T., Gautier, D. and Hubbard, W. B. (1997). Icarus, 130, 534.
7. A Hugoniot is the curve in (P, ρ, T) space which represents the locus of shocked states of the material, starting from one initial pre-shock state.
8. Nellis, W. J., Mitchell, A. C., van Thiel, M., Devine, G. J. and Trainor, R. J. (1983). J. Chem. Phys., 79, 1480.
9. Saumon, D. and Chabrier, G. (1989). Phys. Rev. Lett., 62, 2397.
10. Saumon, D. and Chabrier, G. (1991). Phys. Rev. A, 44, 5122.
11. Saumon, D. and Chabrier, G. (1992). Phys. Rev. A, 46, 2084.
12. Saumon, D., Chabrier, G. and Van Horn, H. M. (1995). Astrophys. J. Suppl., 99, 713.
13. Rogers, F. J. and Young, D. A. (1997). Phys. Rev. E, 56, 5876.
14. Magro, W. R., Ceperley, D. M., Pierleoni, C. and Bernu, B. (1996). Phys. Rev. Lett., 76, 1240.
15. Rogers, F. J. (1994). Equation of State of Stellar Plasmas, p. 16, In: The Equation of State in Astrophysics, Eds. Chabrier, G. and Schatzman, E., Cambridge, Great Britain.
16. Däppen, W. (1994). Helioseismology: the Sun as a Strongly-constrained, Weakly-coupled Plasma, p. 368, In: The Equation of State in Astrophysics, Eds. Chabrier, G. and Schatzman, E., Cambridge, Great Britain.
17. Ross, M., Ree, F. H. and Young, D. A. (1983). J. Chem. Phys., 79, 1487.
18. Harris, G. M. (1959). J. Chem. Phys., 31, 1211.
19. Mihalas, D., Däppen, W. and Hummer, D. G. (1988). Astrophys. J., 331, 815.
20. Hummer, D. G. and Mihalas, D. (1988). Astrophys. J., 331, 794.
21. Porter, R. N. and Karplus, M. (1964). J. Chem. Phys., 40, 1105.
22. Kolos, W. and Wolniewicz, L. (1965). J. Chem. Phys., 43, 2429.
23. Stevenson, D. J. and Salpeter, E. E. (1977). Astrophys. J. Suppl., 35, 221.
24. Chabrier, G., Saumon, D., Hubbard, W. B. and Lunine, J. I. (1992). Astrophys. J., 391, 817.
25. Saumon, D., Hubbard, W. B., Chabrier, G. and Van Horn, H. M. (1992). Astrophys. J., 391, 827.
26. Mao, H. K. and Hemley, R. J. (1994). Rev. Mod. Phys., 66, 671.
27. Ross, M. (1998). Phys. Rev. B, 58, 669.
28. Zinamon, Z. and Rosenfeld, Y. (1998). Phys. Rev. Lett., 81, 4668.
29. Collins, G. W. et al. (1999). Submitted to Phys. Rev. Lett.
30. Collins, G. W. (Private communication).