Density Singularities and Cosmic Structures

Preprint

18 April 1997

preprint
Published by arXiv in arXiv

Abstract

We show that an array of singular density concentrations accounts for the scaling exponents observed in the luminous matter distribution in the Universe for scales below 10Mpc. This model provides a good description of the matter distribution on those smaller scales.

Keywords

DENSITY CONCENTRATIONS
MATTER DISTRIBUTION
EXPONENTS OBSERVED
COSMIC STRUCTURES
SCALING EXPONENTS
SINGULAR DENSITY
LUMINOUS MATTER
SMALLER SCALES
SINGULARITIES

All Related Versions

Version 1, 1997-04-18, ArXiv
Version 2, 1997-06-25, ArXiv
Published version: Monthly Notices of the Royal Astronomical Society, 291 (3), 585.

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