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

被引:7
|
作者
Aktas, C. [1 ]
机构
[1] Canakkale Onsekiz Mart Univ, Art & Sci Fac, Dept Math, TR-17100 Canakkale, Turkey
来源
关键词
Ruban universe; general relativity; teleparallel gravity; LRS Bianchi I universe; energy-momentum distribution; BLACK-HOLE; SCALAR FIELD; LOCALIZATION; EINSTEIN; MODELS;
D O I
10.1142/S0217751X19500118
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
In this study, we obtain Einstein, Bergmann-Thomson (BT), Landau-Lifshitz (LL), Moller, 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 Moller 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 Aygun et al., Taser et al., Dogru et al., Banerjee-Sen, Tryon and Xulu in different gravitation theories.
引用
收藏
页数:12
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