Fluid hydrogen at high density - Pressure dissociation

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Free Energy, Hydrogen Plasma, Liquid Hydrogen, Plasma Density, Thermal Dissociation, Astrophysics, Chemical Equilibrium, Equations Of State, Perturbation Theory, Plasma Pressure

Scientific paper

A model for the Helmholtz free energy of fluid hydrogen at high density and high temperature is developed. This model aims at describing both pressure and temperature dissociation and ionization and bears directly on equations of state of partially ionized plasmas, as encountered in astrophysical situations and high-pressure experiments. This paper focuses on a mixture of hydrogen atoms and molecules and is devoted to the study of the phenomenon of pressure dissociation at finite temperatures. In the present model, the strong interactions are described with realistic potentials and are computed with a modified Weeks-Chandler-Andersen fluid perturbation theory that reproduces Monte Carlo simulations to better than 3 percent. Theoretical Hugoniot curves derived from the model are in excellent agreement with experimental data.

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