Aygun, S.Tarhan, I.Baysal, H.2025-01-272025-01-2720070256-307X1741-3540https://doi.org/10.1088/0256-307X/24/2/015https://hdl.handle.net/20.500.12428/25993The energy-momentum distributions of Einstein's simplest static geometrical model for an isotropic and homogeneous universe are evaluated. For this purpose, Einstein, Bergmann-Thomson, Landau-Lifshitz (LL), Moller and Papapetrou energy-momentum complexes are used in general relativity. While Einstein and Bergmann-Thomson complexes give exactly the same results, LL and Papapetrou energy-momentum complexes do not provide the same energy densities. The Moller energy-momentum density is found to be zero everywhere in Einstein's universe. Also, several spacetimes are the limiting cases considered here.eninfo:eu-repo/semantics/openAccessRadiating Charged-ParticleBlack-HoleGeneral TheoryTetrad TheoryLocalizationDistributionsSpacetimeMassArticle24235535810.1088/0256-307X/24/2/015Q3WOS:0002441164000152-s2.0-34247191239Q1