First-principles Equation of State and Shock Compression Predictions of Warm Dense Hydrocarbons
arXiv:1706.09073 · doi:10.1103/PhysRevE.96.013204
Abstract
We use path integral Monte Carlo and density functional molecular dynamics to construct a coherent set of equation of state for a series of hydrocarbon materials with various C:H ratios (2:1, 1:1, 2:3, 1:2, and 1:4) over the range of g/cm and K. The shock Hugoniot curve derived for each material displays a single compression maximum corresponding to -shell ionization. For C:H=1:1, the compression maximum occurs at 4.7-fold of the initial density and we show radiation effects significantly increase the shock compression ratio above 2 Gbar, surpassing relativistic effects. The single-peaked structure of the Hugoniot curves contrasts with previous work on higher- plasmas, which exhibit a two-peak structure corresponding to both - and -shell ionization. Analysis of the electronic density of states reveals that the change in Hugoniot structure is due to merging of the -shell eigenstates in carbon, while they remain distinct for higher- elements. Finally, we show that the isobaric-isothermal linear mixing rule for carbon and hydrogen EOSs is a reasonable approximation with errors better than 1% for stellar-core conditions.
7 pages, 4 figures. Accepted by Physical Review E
References in corpus (5)
- All-Electron Path Integral Monte Carlo Simulations of Warm Dense Matter: Application to Water and Carbon Plasmas
- First Principles Calculations of Shock Compressed Fluid Helium
- First-Principles Prediction of the Softening of the Silicon Shock Hugoniot Curve
- Equation of state for partially ionized carbon at high temperatures
- Ab initio calculation of thermodynamic, transport, and optical properties of CH plastics