Statistical Physics for Cosmic Structures

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dc.creatorPietronero, Luciano
dc.creatorGabrielli, Andrea
dc.creatorLabini, Francesco Sylos
dc.date2001-10-08
dc.date.accessioned2026-07-07T12:23:23Z
dc.date.available2026-07-07T12:23:23Z
dc.descriptionIdeas of Statistical Physics are very relevant for cosmic structures especially considering that the field is undergoing a period of exceptional development with many new data appearing on a monthly basis. In the past years we have focused mostly on galaxy distributions and their statistical properties. This led to an interesting debate which will be resolved by the next generation of data in a couple of years. In addition here we discuss the statistical properties of the fluctuations of the cosmic microwave background which are small in amplitude but complex in structure. We finally discuss the connection between these observations and the Harrison-Zeldovich spectrum and its further implications on the theories of structure formation and the and the cosmological $N$-body simulations.
dc.description7 pages, latex, 2 postscript figures. To be published in the Proceedings of the Conference "StatsPhys21" held in Cancun (Mexico) July 15-21 2001
dc.identifierhttps://arxiv.org/abs/astro-ph/0110169
dc.identifierhttp://arxiv.org/abs/astro-ph/0110169
dc.identifierPhysica A306:395-401,2002
dc.identifierdoi:10.1016/S0378-4371(02)00517-4
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/213965
dc.subjectAstrophysics
dc.subjectCondensed Matter
dc.titleStatistical Physics for Cosmic Structures
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