Equation of State for laboratory astrophysics applications

Details Equation of State for laboratory astrophysics applications Equation of State for laboratory astrophysics applications

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ap%26ss.336...53c&link_type=abstract

Astrophysics and Space Science, Volume 336, Issue 1, pp.53-59

Astronomy and Astrophysics

Astrophysics

Equation Of State, Shockwave Experiments, Molecular Dynamics

Scientific paper

New improvements on the calculation of Equation of State (EOS) for laboratory astrophysics applications are presented. A new empirical multiplier for the EOS is included to the original quotidian equation of state (QEOS) model developed by More et al. (Phys. Fluids 31:3059, 1988) to adapt it to the available experimental data and ab initio molecular dynamics simulation. This model is used to obtain EOS tables suited for an adaptive mesh refinement hydrodynamic code with radiation transport for high energy density plasmas simulations called ARWEN introduced by Ogando and Velarde (J. Quant. Spectrosc. Radiat. Transf. 71(2-6):541, 2001).

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