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

Articolo
Data di Pubblicazione:
1998
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 D ? 2, at least, in the range of scales ?1 - 200 Mpc (H0 = 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 200 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.
Tipologia CRIS:
01.01 Articolo in rivista
Keywords:
Clusters of Galaxies: Space Distribution; Galaxies: Space Distribution; Hubble Law; Universe: Large-Scale Structure
Elenco autori:
Montuori, Marco
Autori di Ateneo:
MONTUORI MARCO
Link alla scheda completa:
https://iris.cnr.it/handle/20.500.14243/20174
Pubblicato in:
FRACTALS-COMPLEX GEOMETRY PATTERNS AND SCALING IN NATURE AND SOCIETY
Journal
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URL

http://adsabs.harvard.edu/abs/1998Fract...6..231B
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