Statistical physics for cosmic structures (Contributo in atti di convegno)

Type
Label
  • Statistical physics for cosmic structures (Contributo in atti di convegno) (literal)
Anno
  • 2005-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1142/9789812701558_0010 (literal)
Alternative label
  • L. Pietronero (1); F. Sylos Labini (2) (2005)
    Statistical physics for cosmic structures
    in 31st Workshop of the International School of Solid State Physics, Erice, Sicily, Italy, 20 - 26 July 2004
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • L. Pietronero (1); F. Sylos Labini (2) (literal)
Pagina inizio
  • 91 (literal)
Pagina fine
  • 101 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://www.worldscientific.com/doi/abs/10.1142/9789812701558_0010 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#titoloVolume
  • Complexity, Metastability and Nonextensivity (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • (1) Dipartimento di Fisica, Universitá di Roma \"La Sapienza\", P.le A. Moro 2, 00185, Rome, Italy (2) \"Enrico Fermi Center\", Via Panisperna 89 A, Compendio del Viminale, 00184 Rome, Italy and Istituto dei Sistemi Complessi CNR, Via dei Taurini 19, 00185, Rome, Italy (literal)
Titolo
  • Statistical physics for cosmic structures (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#isbn
  • 978-981-256-525-9 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#curatoriVolume
  • Eds. C. Beck, G. Benedek, A. Rapisarda, C. Tsallis (literal)
Abstract
  • Galaxy structures form a complex irregular pattern, characterized by clusters of galaxies which are organized in filaments around large voids. Recently the Sloan Digital Sky Survey project is extending our knowledge of the galaxy distribution, by discovering new and larger structures. The fractal properties are becoming more clear and well established and the issue of the possible crossover toward homogeneity at large scale is revamping. We review the main statistical properties of galaxy distributions discussing the main theoretical open question in the perspective of complex systems. (literal)
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