The Classical Binary and Triplet Distribution Functions for Dilute Relativistic Plasma


The aim of this paper is to calculate the binary and triplet distribution functions for dilute relativistic plasma in terms of the thermal parameter μ where , is the mass of charge; c is the speed of light; k is the Boltzmann’s constant; and T is the absolute temperature. Our calculations are based on the relativistic Bogoliubov-Born-Green-Kirkwood-Yvon (BBGKY) hierarchy. We obtain classical binary and triplet distribution functions for one- and two-component plasmas. The excess free energy and pressure are represented in the forms of a convergent series expansions in terms of the thermal parameter μ.

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Hussein, N. , Eisa, D. and Sayed, E. (2015) The Classical Binary and Triplet Distribution Functions for Dilute Relativistic Plasma. Natural Science, 7, 42-54. doi: 10.4236/ns.2015.71005.

Conflicts of Interest

The authors declare no conflicts of interest.


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