Statistics – Computation
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...243..283f&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 2, March 1991, p. 283-294.
Statistics
Computation
5
Computational Astrophysics, Cosmology, Universe, Astronomical Models, Density Distribution, Hubble Constant
Scientific paper
The description of the cellular structure of the universe is realized with a power law distribution of matter within the framework of generalized Friedmann model. The inhomogeneity is normalized to present matter distribution. The distortion in Hubble flow by density inhomogeneity is calculated for different models. The extrapolation procedure for a global Hubble constant and other cosmological quantities are discussed. It is shown that the distortion in the Hubble flow has great meaning in the common cosmological tests as well as in the measurement of density distribution, clustering properties, and peculiar velocities on large scales.
Feng Long L.
Mo Hou-Jun
Ruffini Remo
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