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Theoretical forms of two- and three-point galaxy correlation functions

✍ Scribed by Jiasheng Chen; Martin A. Pomerantz; Zhenlong Zou

Publisher: Elsevier Science
Year: 1989
Tongue: English
Weight: 443 KB
Volume: 326
Category: Article
ISSN: 0016-0032
DOI: 10.1016/0016-0032(89)90060-4

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✦ Synopsis

The power law form of the two-point galaxy correlation function 5, and a relationship between 5 and the three-point correlation function [, are derived theoretically. These derivations provide a theoretical basis for expressions that heretofore have been based solely upon observations of galaxy or cluster clustering.

s d%(l, 2)vp s d6pc(L 2)vp vfi E ~~._____~~~ = s d%U> 2) n2a6<(x, t) .

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