PUBLICATIONS OF THE ASTRONOMICAL OBSERVATORY OF BELGRADE 107, Page 135-138, https://doi.org/10.69646/14sbac23p
PPROCEEDINGS OF THE XIV SERBIAN-BULGARIAN ASTRONOMICAL CONFERENCE, Vrnjačka Banja, Serbia, September 23-27, 2024, Eds. Milan S. Dimitrijević, Evgeni Semkov, Zoran Simić, Goran Damljanović, Momchil Dechev
Published by: Astronomical Observatory, Volgina 7, 11060 Belgrade 38, Serbia

The modeling of plasma behavior from mid up to strong non-ideality, e.g. plasma with a dominant Coulomb interaction is of interest. The micro field is strongly dependent on a form of used pseudo-potential. It is important to have in mind that the plasma behavior is considered as a variation to the main form of a potential. It was obvious from previous papers that the pseudo-potentials used in solid state physics, e.g. ab-initio ones, could be used successfully in describing of a dense plasma. Here we present the candidates potentials calculated with ab-initio method that should be analyzed in order to be used for describing a dense plasma. As a result, after studying of the potentials, it is expected to have a method of introducing a more complex atoms and ions in existing plasma model.