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arXiv · astro-ph/0111534

An inhomogeneous fractal cosmological model

Fulvio Pompilio·Marco Montuori
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Abstract

We present a cosmological model in which the metric allows for an inhomogeneous Universe with no intrinsic symmetries (Stephani models), providing the ideal features to describe a fractal distribution of matter. Constraints on the metric functions are derived using the expansion and redshift relations and allowing for scaling number counts, as expected in a fractal set. The main characteristics of such a cosmological model are discussed.

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Fulvio Pompilio, Marco Montuori. 2001-11-28. An inhomogeneous fractal cosmological model. https://doi.org/10.1088/0264-9381%2F19%2F2%2F302

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