Gravitational Debye-Hueckel theory for a Newtonian cosmology

Details Gravitational Debye-Hueckel theory for a Newtonian cosmology Gravitational Debye-Hueckel theory for a Newtonian cosmology

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..89..143k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 89, no. 1, Jan. 1983, p. 143-158.

Physics

Condensed Matter

Statistical Mechanics

6

Cosmology, Debye-Huckel Theory, Gravitation Theory, Newton Theory, Statistical Mechanics, Thermodynamic Equilibrium, Collisional Plasmas, Correlation, Coulomb Potential, Distribution Functions, Gibbs Free Energy, Liouville Equations, Particle Interactions, Spatial Distribution

Scientific paper

A correlation function approach is used to formulate a gravitational analogue of equilibrium Debye-Hückel theory appropriate for an expanding Newtonian cosmology. By factoring out the overall expansion of the Universe, one obtains a sensible mathematical framework in which a thermodynamic limit appears to exist. Moreover, one finds that, to lowest non-trivial order, the correlational energy actually vanishes.

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