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Clustering in galaxy distribution: comparison between redshift surveys

Marco Montuori, Luciano Pietronero and Maurizio Bottaccio

Physica A: Statistical Mechanics and its Applications, 2002, vol. 305, issue 1, 242-246

Abstract: The characterization of the galaxy clustering properties in the universe is one of the most interesting and controversial issues in modern cosmology. Here we present the results of the analysis of the recently available three-dimensional catalogues of galaxies, performed with the tools of modern statistical analysis. We focus on the problem of determination of crossover scale to homogeneity in the distribution of luminous matter.

Keywords: Large scale structure; Fractals (search for similar items in EconPapers)
Date: 2002
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Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:305:y:2002:i:1:p:242-246

DOI: 10.1016/S0378-4371(01)00669-0

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Physica A: Statistical Mechanics and its Applications is currently edited by K. A. Dawson, J. O. Indekeu, H.E. Stanley and C. Tsallis

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