DOI: https://doi.org/10.18524/1810-4215.2012.25.83321

ON THE THEORETICAL BASING THE DIRECTION DEPENDENCE COSMOLOGICAL DECELERATION PARAMETER

L. M. Chechin

Анотація


For theoretical describing the asymmetry of Hubble's diagrams and calculating the anisotropy of deceleration parameter phenomenon the concepts of Universe rotation and its two-component model were involved. Our result (Δq/q0)max ≤ 0.48 is in good correlation with the value (Δq/q0)max = 0.76 -0.46+0.41 in (Cai & Tuo, 2011).

Ключові слова


anisotropy of the deceleration parameter; Universe principal axis

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Посилання


Cai R.-G., Tuo Zh.-L.: 2011, arXiv:1109.0941v4 [astroph.CO].

Schwarz D., Weinhorst B.: 2007, astro-ph 0706.0165v2.

Hudson M.J, Smith R.J., Lucey J.R., Branchini E.: 2004, arXiv:astro-ph/0404386v1

Zel’dovich Ya.B., Novikov I.D.: 1983, Relativistic Astrophysics, 2. The structure and evolution of the Universe. University of Chicago Press, 751 p.

Chechin L.M.: 2010, Astronomy Reports, 54, 719.




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