Sufficient condition for Blackhole formation in spherical gravitational collapse
Roberto Giambo', Fabio Giannoni, Giulio Magli

TL;DR
This paper establishes a sufficient condition for cosmic censorship in spherical gravitational collapse, based on properties of the apparent horizon and physical reasonableness of matter models.
Contribution
It formulates and proves a sufficient condition for black hole formation in spherical collapse, linking horizon properties with matter model assumptions.
Findings
Sufficient condition for black hole formation established
Condition relies on apparent horizon properties
Applicable under physically reasonable matter models
Abstract
A sufficient condition for the validity of Cosmic Censorship in spherical gravitational collapse is formulated and proved. The condition relies on an attractive mathematical property of the apparent horizon, which holds if ''minimal'' requirements of physical reasonableness are satisfied by the matter model.
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