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

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

2010-08-05

arxiv.org/abs/1008.0966v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

to publish in APJ

Scientific paper

10.1088/0004-637X/721/2/1158

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.

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