Primordial density fields, super-homogeneity and galaxy clustering

Details Primordial density fields, super-homogeneity and galaxy clustering Primordial density fields, super-homogeneity and galaxy clustering

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007newar..51..437s&link_type=abstract

New Astronomy Reviews, Volume 51, Issue 3-4, p. 437-441.

Astronomy and Astrophysics

Astronomy

Dark Energy, Cosmology, Superclusters, Large-Scale Structure Of The Universe

Scientific paper

Main statistical properties of matter density fields predicted by standard models of galaxy formation are discussed with particular emphasis on the statistical interpretation of the Harrison Zeldovich (H Z) tail of the matter power spectrum. The problem of sampling a Gaussian density field with H Z tail is considered and some observational implications of these results are discussed.

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