On the validity of the quasi-linear theory for the cosmological three-point correlation function

Details On the validity of the quasi-linear theory for the cosmological three-point correlation function On the validity of the quasi-linear theory for the cosmological three-point correlation function

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasj...43..661i&link_type=abstract

Astronomical Society of Japan, Publications (ISSN 0004-6264), vol. 43, no. 5, 1991, p. 661-669. Research supported by Yamada Sci

Statistics

Computation

5

Bbgky Hierarchy, Computational Astrophysics, Galactic Mass, Spatial Distribution, Statistical Correlation, Hubble Constant, Universe

Scientific paper

Quasi-linear theory was found to be successful for the cosmological
two-point correlation function and is shown to be inapplicable for the
three-point correlation. Another important conclusion obtained is that
the initial correlations equal to or higher than three-point do not
affect the higher-order correlations after a sufficiently long time.

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