Asymptotic Behavior of Spherically Symmetric Marginally Trapped Tubes

Abstract

We give conditions on a general stress-energy tensor T_{αβ} in a spherically symmetric black hole spacetime which are sufficient to guarantee that the black hole will contain a (spherically symmetric) marginally trapped tube which is eventually achronal, connected, and asymptotic to the event horizon. Price law decay per se is not required for this asymptotic result, and in this general setting, such decay only implies that the marginally trapped tube has finite length with respect to the induced metric. We do, however, impose a smallness condition (B1) which one may obtain in practice by imposing decay on the T_{vv} component of the stress-energy tensor. We give two applications of the theorem to self-gravitating Higgs field spacetimes, one using weak Price law decay, the other certain strong smallness and monotonicity assumptions.

43 pages, 7 figures. Updated to agree with published version; Theorem 1 strengthened slightly, minor issues fixed

References in corpus (2)

• Introduction to dynamical horizons in numerical relativity
• Strong cosmic censorship for T^2-symmetric cosmological spacetimes with collisionless matter

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