The correlation function for density perturbations in an expanding universe. II - Nonlinear theory

Details The correlation function for density perturbations in an expanding universe. II - Nonlinear theory The correlation function for density perturbations in an expanding universe. II - Nonlinear theory

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...217..331m&link_type=abstract

Astrophysical Journal, Part 1, vol. 217, Oct. 15, 1977, p. 331-352.

Astronomy and Astrophysics

Astrophysics

61

Astronomical Models, Big Bang Cosmology, Correlation, Density Distribution, Perturbation Theory, Functionals, Galactic Evolution, Integral Equations

Scientific paper

A formalism is developed to find the two-point and higher-order correlation functions for a given distribution of sizes and shapes of perturbations which are randomly placed in three-dimensional space. The perturbations are described by two parameters such as central density and size, and the two-point correlation function is explicitly related to the luminosity function of groups and clusters of galaxies

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