Reconstructing the cosmological puzzle

dc.creatorPietronero, Luciano
dc.creatorLabini, Francesco Sylos
dc.date1999-10-08
dc.date.accessioned2026-07-07T02:33:45Z
dc.date.available2026-07-07T02:33:45Z
dc.descriptionIn the debate about galaxy correlation there are different questions which can be addressed separately: Which are the statistical methods able to properly detect scale invariance and describe, in general, the properties of irregular and regular distributions? Which are the implications for cosmology of the fractal behavior of galactic structures, up to a certain scale lambda_0? Which is the homogeneity scale lambda_0, i.e. the scale beyond which galaxy distribution has an eventual crossover to homogeneity? These are three different, but related, problems, which must be considered in different steps, from the point of view of data analysis as well as from the theoretical perspective.
dc.description21 pages, latex, 4 figures, also available at http://pil.phys.uniroma1.it/astro.html. To appear in the proceedings of the "VI Colloque de Cosmologie" Paris 16-18 June 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9910161
dc.identifierhttp://arxiv.org/abs/astro-ph/9910161
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14972
dc.subjectAstrophysics
dc.titleReconstructing the cosmological puzzle
dc.typetext

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