Involute, minimal, outer and increasingly trapped spheres
Sean A. Hayward

TL;DR
This paper introduces seven refined stability conditions for trapped surfaces in spherical symmetry, exploring their hierarchy, equivalences in static spacetimes, and examples in black hole models, including dirty black holes.
Contribution
It proposes seven new refinements of trapped surface conditions, analyzes their hierarchy and equivalences, and provides examples in various black hole spacetimes.
Findings
Seven trapped surface refinements form a strict hierarchy under the null energy condition.
In static spacetimes, three main definitions of trapped surfaces are equivalent.
Examples include Reissner-Nordström black holes and a family of dirty black holes.
Abstract
Seven different refinements of trapped surfaces are proposed, each intended as potential stability conditions. This article concerns spherical symmetry, but each condition can be generalized. Involute trapped spheres satisfy a similar condition to minimal trapped spheres, which are are strictly minimal with respect to the Kodama vector. There is also a weaker version of involute trapped. Outer trapped spheres have positive surface gravity. Increasingly (future, respectively past) trapped spheres generate spheres which are more trapped in a (future, respectively past) causal direction, with three types: in any such causal direction, along the dual Kodama vector, and in some such causal direction. Assuming the null energy condition, the seven conditions form a strict hierarchy, in the above order. In static space-times, they reduce to three inequivalent definitions, namely minimal, outer…
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