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arXiv · 1005.5401

A black hole with no marginally trapped tube asymptotic to its event horizon

Catherine Williams
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Abstract

We construct an example of a spherically symmetric black hole interior in which there is NO (spherically symmetric) marginally trapped tube asymptotic to the event horizon. The construction uses a self-gravitating massive scalar field matter model, and the key condition we impose is that the scalar field $ϕ$ be bounded below by a positive constant along the event horizon.

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Catherine Williams. 2010-05-28. A black hole with no marginally trapped tube asymptotic to its event horizon. https://arxiv.org/abs/1005.5401

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