Physics
Scientific paper
Nov 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...74..471g&link_type=abstract
Space Science Reviews, Volume 74, Issue 3-4, pp. 471-474
Physics
Cosmology, Gravitation
Scientific paper
We consider the influence of the nonlinear stage of gravitational instability on the two-point correlation functions of gravitationally bound objects. Based on the theory of nonlinear gravitational contraction of a single density peak of dissipationless matter (Gurevich and Zybin, 1988a,b; 1990) we develop a method for calculating the two-point correlation functions of different objects of any mass. The method works good in the region of strong correlations and can be easily extended to calculate higher correlation functions. We show that the main contribution to the correlation function ξi in the region of strong correlations ξi ≫ 1 is made by pair systems located outside large clusters of objects. In this region the shape of ξi is determined only by the nonlinear dynamics of gravitational contraction of dissipationless matter and has the form ξi ≈C τ -α, where α≈1.8 is a universal parameter.
Gurevich Aleksander V.
Zelnikov M. I.
Zybin Kirill P.
No associations
LandOfFree
Nonlinear Theory of the Two-Point Correlation Function does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Nonlinear Theory of the Two-Point Correlation Function, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear Theory of the Two-Point Correlation Function will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1182517