Involute, minimal, outer and increasingly trapped spheres

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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Substantially extended to include detailed study of static space-times. 10 REVTeX4 pages

Scientific paper

10.1103/PhysRevD.81.024037

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 and increasingly trapped spheres. For a widely considered class of so-called nice (or non-dirty) black holes, minimal trapped and outer trapped become equivalent. Reissner-Nordstr\"om black holes provide examples of this, and that increasingly trapped differs. Examples where all three refinements differ are provided by a simple family of dirty black holes parameterized by mass and singularity area.

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