Statistical mechanics of light elements at high pressure. III. Molecular hydrogen
Journal Article
·
· Astrophys. J., v. 181, no. 3, pp. 1031-1038
The high-pressure thermodynamic properties of a molecular hydrogen fluid are calculated in the classical domain using a Monte Carlo approach. A recent theoretical intermolecular potential of the exp -- 6 form which gives good agreement with low-pressure experimental data, and fair agreement with highpressure data, is used. Melting curves and adiabats with relevance to planetary models are calculated. A possible application of the theory of pressure-induced opacity in molecular hydrogen is noted. (auth)
- Research Organization:
- Univ. of Texas, Austin
- NSA Number:
- NSA-29-003299
- OSTI ID:
- 4419483
- Journal Information:
- Astrophys. J., v. 181, no. 3, pp. 1031-1038, Other Information: Orig. Receipt Date: 30-JUN-74
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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