Energy–momentum distributions of Ruban universe in general relativity and teleparallel gravity

Author:

Aktaş C.1

Affiliation:

1. Çanakkale Onsekiz Mart University, Art and Science Faculty, Department of Mathematics, 17100 Çanakkale, Turkey

Abstract

In this study, we obtain Einstein, Bergmann–Thomson (BT), Landau–Lifshitz (LL), Møller, Papapetrou (PP) and Tolman energy–momentum (EM) distributions for Ruban universe model in general relativity (GR) and teleparallel gravity (TG). We obtain same results for Einstein, Bergmann–Thomson and Landau–Lifshitz energy–momentum distributions in GR and TG. Also, we get same results for Einstein and Tolman energy–momentum distributions in GR. The Møller energy–momentum results are different in GR and TG. Also, using Ruban universe model, we obtain LRS Bianchi type I solutions and we get zero energy–momentum results for this universe model in GR and TG. These results of LRS Bianchi type I universe model agree with Aygün et al., Taşer et al., Doğru et al., Banerjee–Sen, Tryon and Xulu in different gravitation theories.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference63 articles.

1. R. C. Tolman, Relativity, Thermodynamics and Cosmology (Oxford University Press, 1934), p. 227.

2. Spin and Angular Momentum in General Relativity

3. On the localization of the energy of a physical system in the general theory of relativity

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