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The Classical Binary and Triplet Distribution Functions for Dilute Relativistic Plasma

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ABSTRACT
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 parameterμ.
 
Cite this paper
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.
 
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book/978-0-306-46031-9                                                                                             eww150126lx
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