Statistical Mechanics of the Cosmological Many-body Problem

Details Statistical Mechanics of the Cosmological Many-body Problem Statistical Mechanics of the Cosmological Many-body Problem

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1150..252m&link_type=abstract

FRONTIERS IN PHYSICS: 3rd International Meeting. AIP Conference Proceedings, Volume 1150, pp. 252-261 (2009).

Physics

Observational Cosmology, Galaxy Clusters, Thermodynamic Processes, Conduction, Convection, Equations Of State, Spectroscopy And Spectrophotometry, Dark Matter

Scientific paper

The statistical mechanical description of the cosmological many-body problem is reviewed in light of the recent advances [1, 2, 3]. This description makes it possible to take into account the extended nature of galaxies, include the effect of higher order contributions, allow a description for the two-component system of galaxies and possibly account for a fraction of the dark matter in the Universe, besides providing a more fundamental basis for the earlier results. The spatial galaxy distribution function is shown as a powerful statistic showing excellent agreement with observations and N-body simulation results.

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