Quasi-self-similar stable clustering solution of the two-point correlation functions

Details Quasi-self-similar stable clustering solution of the two-point correlation functions Quasi-self-similar stable clustering solution of the two-point correlation functions

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pabei..19s..67s&link_type=abstract

"Progress in Astronomy, Vol. 19, Supp., p. 67 - 71 (2001). In: Proceedings of the Fourth China-Germany Workshop on Cosmology "Co

Astronomy and Astrophysics

Astronomy

Cosmology, Galaxy Clustering

Scientific paper

We discuss a model to extend the stable clustering solution for the two-point correlation function in non-Einstein-de Sitter universes. For this purpose we introduce an idea of quasi-self-similar evolution, which is based on the assumption that the evolution of the two-point correlation is a succession of stages of evolution, each of which spans a short enough period to be considered approximately self-similar. Combined with the stable conditions, our model predicts the behavior of the two-point correlation function in the strongly nonlinear regime which is consistent with the high-resolution N-body simulations.

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