Einstein manifolds are Riemannian manifolds whose Ricci curvature is proportional to the metric, meaning that the Ricci tensor satisfies the equation \( Ric = \lambda g \), where \( \lambda \) is a constant and \( g \) is the metric tensor. This condition implies that these manifolds exhibit uniform geometric properties and are significant in the study of general relativity, as they represent spacetime structures with constant scalar curvature.
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