Gravitational Collapse of Vacuum Gravitational Field Configurations
arXiv:gr-qc/9411024 · doi:10.1063/1.531007
Abstract
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 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 is larger than unity, then an apparent horizon must form, signalling the formation of a black hole.
arXiv comment10 pages and no figures, uses jnl macros (as at archive)
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