The progress of the three-point correlation function

Details The progress of the three-point correlation function The progress of the three-point correlation function

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pabei..24..142h&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 24, No. 2, p. 142 - 159 (2006)

Astronomy and Astrophysics

Astrophysics

Astrophysics, Three-Point Correlation Function, Review, Formation, Large-Scale Structure, Statistics

Scientific paper

Three-point correlation function (3PCF) and its Fourier counter part, bispectrum, are the lowest statistics that quantify the non-Gaussian behavior of the large scale structure induced by the gravitational instability. In the present paper, the basic theory of the three-point correlation function and its Fourier counter part, bispectrum, are introduced firstly, then the results of 3PCF and bispectrum measured from the galaxies survey and simulations and predicted by the halo model are summarized.

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