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Quantum Langevin molecular dynamics determination of the solar-interior equation of state

The equation of state (EOS) of the solar interior is accurately and smoothly determined from \textit{ab initio} simulations named quantum Langevin molecular dynamics (QLMD) in the pressure range of $58 \leq P \leq 4.6\times10^5$ Mbar at the temperature range of $1 \leq T \leq 1500$ eV. The central pressure is calculated, and compared with other models. The effect of heavy elements such as carbon and oxygen on the EOS is also discussed.

preprint2010arXivOpen access
Jiayu DaiYong HouJianmin Yuan
physics.atom-phphysics.plasm-phastro-ph.SR
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Jiayu DaiYong HouJianmin Yuan

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