Inhomogeneous and anisotropic Universe and apparent acceleration

G. Fanizza and L. Tedesco
Phys. Rev. D 91, 023006 – Published 22 January 2015

Abstract

In this paper, we introduce a Lemaître-Tolman-Bondi (LTB) Bianchi type I (plane symmetric) model of the Universe. We study and solve Einstein field equations. We investigate the effects of such a model of the Universe; in particular, these results are important in understanding the effect of the combined presence of an inhomogeneous and anisotropic universe. The observational magnitude-redshift data deviated from the UNION 2 catalog have been analyzed in the framework of this LTB anisotropic universe, and the fit has been achieved without the inclusion of any dark energy.

  • Figure
  • Received 20 October 2014

DOI:https://doi.org/10.1103/PhysRevD.91.023006

© 2015 American Physical Society

Authors & Affiliations

G. Fanizza* and L. Tedesco

  • Dipartimento di Fisica, Università di Bari, Via G. Amendola 173, 70126 Bari, Italy
  • Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy

  • *giuseppe.fanizza@ba.infn.it
  • luigi.tedesco@ba.infn.it

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Issue

Vol. 91, Iss. 2 — 15 January 2015

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