An inhomogeneous fractal cosmological model

Details An inhomogeneous fractal cosmological model An inhomogeneous fractal cosmological model

2001-11-28

arxiv.org/abs/astro-ph/0111534v1

Class.Quant.Grav. 19 (2002) 203-212

Astronomy and Astrophysics

Astrophysics

11 pages, no figures, accepted for publication on Classical and Quantum Gravity

Scientific paper

10.1088/0264-9381/19/2/302

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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