Ionisation balance and equation of state of hot, dense carbon plasmas at pressures up to a few 100 Gbar

Open Access

Fig. 7

Comparison of pressure as a function of mass density for carbon plasmas at a temperature of 100 eV, as predicted by the FPMD method (Clerouin et al. 2022), the QAAM model, and the QMD simulations (Faussurier et al. 2021).

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