Quantum Langevin molecular dynamics determination of the solar-interior equation of state
Solar and Stellar Astrophysics
2013-03-26 v1 Atomic Physics
Plasma Physics
Abstract
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 Mbar at the temperature range of 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.
Keywords
Cite
@article{arxiv.1008.0966,
title = {Quantum Langevin molecular dynamics determination of the solar-interior equation of state},
author = {Jiayu Dai and Yong Hou and Jianmin Yuan},
journal= {arXiv preprint arXiv:1008.0966},
year = {2013}
}
Comments
to publish in APJ