Baysal, Husnu2025-01-272025-01-2720120217-73231793-6632https://doi.org/10.1142/S0217732312502318https://hdl.handle.net/20.500.12428/25976We have calculated the total energy-momentum distribution associated with (n+2)-dimensional spherically symmetric model of the universe by using the Moller energy-momentum definition in general relativity (GR). We have found that components of Moller energy and momentum tensor for given spacetimes are different from zero. Also, we are able to get energy and momentum density of various well-known wormholes and black hole models by using the (n+2)-dimensional spherically symmetric metric. Also, our results have been discussed and compared with the results for four-dimensional spacetimes in literature.eninfo:eu-repo/semantics/closedAccessHigher-dimensional universesMoller energy momentum complexspherically-symmetric spacetimesgeneral relativityArticle274010.1142/S0217732312502318Q3WOS:0003144590000042-s2.0-84871419557Q2