Statistical physics for cosmic structures (Articolo in rivista)

Type
Label
  • Statistical physics for cosmic structures (Articolo in rivista) (literal)
Anno
  • 2008-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1140/epjb/e2008-00002-8 (literal)
Alternative label
  • Sylos Labini F. (1); Pietronero L. (2) (2008)
    Statistical physics for cosmic structures
    in The European physical journal. B, Condensed matter physics (Print)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Sylos Labini F. (1); Pietronero L. (2) (literal)
Pagina inizio
  • 615 (literal)
Pagina fine
  • 623 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://www.springerlink.com/content/a383v27547236886/ (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 64 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#note
  • fasc. (3-4). Springer. (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo
  • 3-4 (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1) “Enrico Fermi Center”, Piazzale del Viminale 2, 00184 Rome, Italy & “Istituto dei Sistemi Complessi” CNR, Via dei Taurini 19, 00185 Rome, Italy 2) Physics Department, University of Rome “Sapienza”, Piazzale A. Moro 2, 00185 Rome, Italy [ISC-CNR] (literal)
Titolo
  • Statistical physics for cosmic structures (literal)
Abstract
  • The recent observations of galaxy and dark matter clumpy distributions have provided new elements to the understanding of the problem of cosmological structure formation. The strong clumping characterizing galaxy structures seems to be present in the overall mass distribution and its relation to the highly isotropic Cosmic Microwave Background Radiation represents a fundamental problem. The extension of structures, the formation of power-law correlations characterizing the strongly clustered regime and the relation between dark and visible matter are the key problems both from an observational and a theoretical point of view. We discuss recent progresses in the studies of structure formation by using concepts and methods of statistical physics. (literal)
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