Equilibrium Correlations in a Clustering Universe

Details Equilibrium Correlations in a Clustering Universe Equilibrium Correlations in a Clustering Universe

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chphl..20.2088z&link_type=abstract

Chinese Physics Letters, Volume 20, Issue 11, pp. 2088-2090 (2003).

Physics

Scientific paper

It is shown that the observed result of the two-point galaxy correlation function and the three-point correlation function in the Universe agrees with a quasi-equilibrium assumption of mass distribution. Utilizing the form of the three-point correlation, we find that the two-point correlation function can be obtained by solving an equation derived from maximizing entropy under some constraints in a self-gravitating particle model. A generalized non-extensive entropy is also introduced to improve our result.

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