International Journal of Geometric Methods in Modern Physics · 2013 · 22 citations · 7 references
Natural SciencesPhysicsCosmologyMathematical PhysicsTheoretical PhysicsCurved SpacetimeEinstein Field EquationsGeneral RelativitySpacetime GeometrySpecial RelativityTheoretical CosmologyAsymptotically Flat SpacetimesCurvatureCurvature TensorsEinstein Field Equations In CosmologyEnergy-momentum RelationFlat CosmologyGeneral Relativity In CosmologyScalar Curvature
The object of this paper is to study spacetimes admitting W 2 -curvature tensor. At first we prove that a W 2 -flat spacetime is conformally flat and hence it is of Petrov type O. Next, we prove that if the perfect fluid spacetime with vanishing W 2 -curvature tensor obeys Einstein's field equation without cosmological constant, then the spacetime has vanishing acceleration vector and expansion scalar and the perfect fluid always behaves as a cosmological constant. It is also shown that in a perfect fluid spacetime of constant scalar curvature with divergence-free W 2 -curvature tensor, the energy-momentum tensor is of Codazzi type and the possible local cosmological structure of such a spacetime is of type I, D or O.
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