Evaluation of Molecular-Dynamics Simulations for the Study of Hot Dense Coulomb Systems

Physics

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Solar Interior, Star Formation, Molecular Dynamics Methods

Scientific paper

In the plasma of solar and stellar interiors, Coulomb potentials are screened, resulting in increased nuclear reaction rates. Though Salpeter's approximation for static screening is widely accepted and used in stellar modelling, the question of screening in nuclear reactions has recently been revisited. In particular the issue of dynamic effects has been raised by Shaviv and Shaviv who apply the techniques of molecular dynamics to the conditions in the Sun's core in order to numerically determine the effect of screening. By directly calculating the motion of ions and electrons due to Coulomb interactions, they are able to compute the effect of screening without the mean field assumption inherent in Salpeter's approximation. However, Shaviv and Shaviv's work includes a variety of assumptions that must be evaluated before their results can be accepted. We carried out a pilot study of a small system under conditions similar to the solar core in order to examine the assumptions and approximations in Shaviv and Shaviv's numerical simulations. Our work confirms Shaviv and Shaviv's conclusion that instead of relying on the static approximation, dynamic effects must also be considered.

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