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The topology of fractal universesIt is shown how the genus per unit volume of isodensity surfaces in general nonlinear universes is related to the entire hierarchy of correlation functions. The general relation between the correlation function, the probability distribution of densities at several points, and the probability distributions of density and its derivatives at a point are given. Formulas for the area and genus per unit volume of isodensity surfaces are presented. As an application, after first reviewing the case of Gaussian fields, analytic results are reported for one particular example of a thoroughly nonlinear universe, Mandelbrot's Rayleigh-Levy random-walk fractal. While this fractal bears little resemblance to the real universe of galaxies, it possesses the singular and theoretically interesting property that in it cluster-cluster correlations are identically equal to galaxy-galaxy correlations to all orders.
Document ID
19890036963
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hamilton, A. J. S.
(Joint Institute for Laboratory Astrophysics Boulder, CO, United States)
Date Acquired
August 14, 2013
Publication Date
November 1, 1988
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 100
ISSN: 0004-6280
Subject Category
Astrophysics
Accession Number
89A24334
Funding Number(s)
CONTRACT_GRANT: NAGW-766
CONTRACT_GRANT: NSF AST-86-58022
CONTRACT_GRANT: NSG-7128
Distribution Limits
Public
Copyright
Other

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