Amplification of correlation functions by gravity in the cosmic string model

Details Amplification of correlation functions by gravity in the cosmic string model Amplification of correlation functions by gravity in the cosmic string model

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phlb..191..257b&link_type=abstract

Physics Letters B, Volume 191, Issue 3, p. 257-262.

Physics

3

Scientific paper

Gravitational clustering can lead to a time dependence of the slope of correlation functions of galaxies and clusters of galaxies. In the cosmic string theory this effect is too weak to change the initial two-point correlation function of clusters. It can, however, lead to a steepening of the galaxy correlation function, provided the dark matter is cold.

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