Gravitational Collapse of Vacuum Gravitational Field Configurations

This paper proves a theorem about the existence of an apparent horizon in general relativity, which applies equally well to vacuum configurations and matter configurations. The theorem uses the reciprocal of the surface-to-volume ratio of a region on a space slice to measure the radius of the region, and uses the minimum value $K_{\mathrm{m}\mathrm{i}\mathrm{n}}$ of certain components of the extrinsic curvature to measure the strengh of the gravitational field in the region. The theorem proves that, if the product of the radius times $K_{\mathrm{m}\mathrm{i}\mathrm{n}}$ is larger than unity, then an apparent horizon must form, signalling the formation of a black hole.