The limit on mean field theories and nuclear screening in stellar plasmas

Details The limit on mean field theories and nuclear screening in stellar plasmas The limit on mean field theories and nuclear screening in stellar plasmas

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..731...67s&link_type=abstract

EQUATION-OF-STATE AND PHASE-TRANSITION ISSUES IN MODELS OF ORDINARY ASTROPHYSICAL MATTER. AIP Conference Proceedings, Volume 73

Astronomy and Astrophysics

Astrophysics

1

Magnetohydrodynamics And Plasmas, Elementary Particle Processes, Thermodynamic Processes, Conduction, Convection, Equations Of State, Solar Interior

Scientific paper

We discuss the physical conditions in the core of the Sun and Main Sequence stars and show that the basic requirement for the validity of the Debye mean field theory is not satisfied. We apply Molecular Dynamics to a gedanken numerical experiment and investigate the implications to the screening problem. We show how the thermodynamic limit is approached and under what conditions. Examples of actual screening enhancement calculated under these conditions are brought.

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