  Dense plasmas occur in stars, giant planets and in inertial fusion
experiments. Accurate modeling of the electronic structure of these plasmas
allows for prediction of material properties that can in turn be used to
simulate these astrophysical objects and terrestrial experiments. But modeling
them remains a challenge. Here we explore the Korringa-Kohn-Rostoker Green's
function (KKR-GF) method for this purpose. We find that it is able to predict
equation of state in good agreement with other state of the art methods, where
they are accurate and viable. In addition, it is shown that the computational
cost does not significantly change with temperature, in contrast with other
approaches. Moreover, the method does not use pseudopotentials - core states
are calculated self consistently. We conclude that KKR-GF is a very promising
method for dense plasma simulation.
