Gravitational Collapse of Vacuum Gravitational Field Configurations
Douglas M. Eardley (ITP)

TL;DR
This paper establishes a theorem in general relativity that predicts apparent horizon formation, indicating black hole creation, based on the geometric and curvature properties of vacuum and matter configurations.
Contribution
It introduces a new criterion involving surface-to-volume ratio and extrinsic curvature to determine apparent horizon formation in vacuum gravitational fields.
Findings
Proves a condition for apparent horizon existence in vacuum configurations.
Links the product of region radius and curvature to black hole formation.
Provides a geometric measure for gravitational collapse in general relativity.
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.
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