English

On the fractal structure of galaxy distribution and its implications for cosmology

Astrophysics 2007-05-23 v1

Abstract

Two fundamental empirical laws have been established in the analysis of galaxy space distribution. First, recent analyses have revealed that the three dimensional distribution of galaxies and clusters is characterized by large scale structures and huge voids: such a distribution shows fractal correlations up to the limits of the available samples. This has confirmed the earlier de Vaucouleurs power-law density - distance relation, now corresponding to a fractal structure with dimension D2D \approx 2, at least, in the range of scales 1÷200Mpc \sim 1 \div 200 Mpc (H0=55km/sec/MpcH_0 = 55 km/sec/Mpc). An eventual cut-off towards homogenization has not been yet identified. Second, since Hubble's discovery, the linear redshift-distance law has been well established within 200Mpc200 Mpc and also much deeper. The co-existence of these laws within the same scales is a challenge for the standard cosmology where the linear Hubble law is a strict consequence of homogeneity of the expanding universe. This puzzle is now sufficiently strong to raise doubts for the standard cosmology.

Keywords

Cite

@article{arxiv.astro-ph/9803142,
  title  = {On the fractal structure of galaxy distribution and its implications for cosmology},
  author = {Yurij V. Baryshev and Francesco Sylos Labini and Marco Montuori and Luciano Pietronero and Pekka Teerikorpi},
  journal= {arXiv preprint arXiv:astro-ph/9803142},
  year   = {2007}
}

Comments

25 pages, latex, 4 figures, also available at http://www.phys.uniroma1.it/DOCS/PIL/pil.html Accepted for publication in "Fractals"