Rigidity of marginally outer trapped 2-spheres

Abstract

In a matter-filled spacetime, perhaps with positive cosmological constant, a stable marginally outer trapped 2-sphere must satisfy a certain area inequality. Namely, as discussed in the paper, its area must be bounded above by $4\pi /c$, where $c>0$ is a lower bound on a natural energy-momentum term. We then consider the rigidity that results for stable, or weakly outermost, marginally outer trapped 2-spheres that achieve this upper bound on the area. In particular, we prove a splitting result for 3-dimensional initial data sets analogous to a result of Bray, Brendle and Neves [10] concerning area minimizing 2-spheres in Riemannian 3-manifolds with positive scalar curvature. We further show that these initial data sets locally embed as spacelike hypersurfaces into the Nariai spacetime. Connections to the Vaidya spacetime and dynamical horizons are also discussed.

v3: 18 pages; added references and an acknowledgment of NSF support. Version to appear in Communications in Analysis and Geometry. (This paper supersedes arXiv:1503.05540 and arXiv:1504.06754)

Cited by in corpus (1)

• Upper Bound for Diameter of Cosmological Black Holes and Nonexistence of Black Strings