On the Weyl curvature hypothesis

The Weyl curvature hypothesis of Penrose attempts to explain the high homogeneity and isotropy, and the very low entropy of the early universe, by conjecturing the vanishing of the Weyl tensor at the Big-Bang singularity. In previous papers it has been proposed an equivalent form of Einstein’s equation, which extends it and remains valid at an important class of singularities (including in particular the Schwarzschild, FLRW, and isotropic singularities). Here it is shown that if the Big-Bang singularity is from this class, it also satisfies the Weyl curvature hypothesis. As an application, we study a very general example of cosmological models, which generalizes the FLRW model by dropping the isotropy and homogeneity constraints. This model also generalizes isotropic singularities, and a class of singularities occurring in Bianchi cosmologies. We show that the Big-Bang singularity of this model is of the type under consideration, and satisfies therefore the Weyl curvature hypothesis. •The singularities we introduce are described by finite geometric/physical objects.•Our singularities have smooth Riemann and Weyl curvatures.•We show they satisfy Penrose’s Weyl curvature hypothesis (Weyl=0 at singularities).•Examples: FLRW, isotropic singularities, an extension of Schwarzschild’s metric.•Example: a large class of singularities which may be anisotropic and inhomogeneous.