skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Remarks on mechanical approach to observable Universe

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2]
  1. CREST and NASA Research Centers, North Carolina Central University, Fayetteville st. 1801, Durham, North Carolina 27707 (United States)
  2. Astronomical Observatory, Odessa National University, Dvoryanskaya st. 2, Odessa 65082 (Ukraine)

We consider the Universe deep inside the cell of uniformity. At these scales, the Universe is filled with inhomogeneously distributed discrete structures (galaxies, groups and clusters of galaxies), which perturb the background Friedmann model. Here, the mechanical approach (Eingorn and Zhuk, 2012) is the most appropriate to describe the dynamics of the inhomogeneities which is defined, on the one hand, by gravitational potentials of inhomogeneities and, on the other hand, by the cosmological expansion of the Universe. In this paper, we present additional arguments in favor of this approach. First, we estimate the size of the cell of uniformity. With the help of the standard methods of statistical physics and for the galaxies of the type of the Milky Way and Andromeda, we get that it is of the order of 190 Mpc which is rather close to observations. Then, we show that the nonrelativistic approximation (with respect to the peculiar velocities) is valid for z∼<10, i.e. approximately for 13 billion years from the present moment. We consider scalar perturbations and, within the ΛCDM model, justify the main equations. Moreover, we demonstrate that radiation can be naturally incorporated into our scheme. This emphasizes the viability of our approach. This approach gives a possibility to analyze different cosmological models and compare them with the observable Universe. For example, we indicate some problematic aspects of the spatially flat models. Such models require a rather specific distribution of the inhomogeneities to get a finite potential at any points outside gravitating masses. We also criticize the application of the Schwarzschild-de Sitter solution to the description of the motion of test bodies on the cosmological background.

OSTI ID:
22373575
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2014, Issue 05; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Dynamics of astrophysical objects against the cosmological background
Journal Article · Mon Apr 01 00:00:00 EDT 2013 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22373575

Hubble flows and gravitational potentials in observable Universe
Journal Article · Sat Sep 01 00:00:00 EDT 2012 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22373575

Recessional velocities and Hubble's law in Schwarzschild-de Sitter space
Journal Article · Mon Mar 15 00:00:00 EDT 2010 · Physical Review. D, Particles Fields · OSTI ID:22373575