Dynamical Scaling of Matter Density Correlations in the Universe: an Application of the Dynamical Renormalization Group

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dc.creatorDominguez, A.
dc.creatorHochberg, D.
dc.creatorMartin-Garcia, J. M.
dc.creatorPerez-Mercader, J.
dc.creatorSchulman, L. S.
dc.date1999-01-15
dc.date.accessioned2026-07-07T02:30:01Z
dc.date.available2026-07-07T02:30:01Z
dc.descriptionWe show how the interplay of non-linear dynamics, self-gravity, and fluctuations leads to self-affine behavior of matter density correlations quite generically, i.e., with a power-law exponent whose value does not depend in a very direct way on the specific details of the dynamics. This we do by means of the Renormalization Group, a powerful analytic tool for extracting asymptotic behavior of many-body systems
dc.descriptionAccepted for publication in Astronomy & Astrophysics. 10 pages using A&A style file; 2 eps figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9901208
dc.identifierhttp://arxiv.org/abs/astro-ph/9901208
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13693
dc.subjectAstrophysics
dc.titleDynamical Scaling of Matter Density Correlations in the Universe: an Application of the Dynamical Renormalization Group
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