Aktaş, Can2025-01-272025-01-2720190217-751X1793-656Xhttps://doi.org/10.1142/S0217751X19500118https://hdl.handle.net/20.500.12428/21354In 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.eninfo:eu-repo/semantics/closedAccessRuban universegeneral relativityteleparallel gravityLRS Bianchi I universeenergy-momentum distributionArticle343-410.1142/S0217751X19500118Q3WOS:0004592938000012-s2.0-85061510267Q2