On the geodesic incompleteness of spacetimes containing marginally outer trapped surfaces
I. P. Costa e Silva

TL;DR
This paper investigates the conditions under which spacetimes containing marginally outer trapped surfaces (MOTS) exhibit geodesic incompleteness, extending singularity theorems to weaker causal conditions and emphasizing MOTS as black hole indicators.
Contribution
It demonstrates that singularities can be inferred from generic MOTS under weaker causal assumptions and establishes a Penrose-Hawking-type theorem for such surfaces.
Findings
Singularities arise with generic MOTS in causally simple spacetimes.
A Penrose-Hawking-type theorem applies when MOTS bounds a compact region.
Results extend singularity theorems to MOTS without requiring MOTS to be generic.
Abstract
In a recent paper, Eichmair, Galloway and Pollack have proved a Gannon-Lee-type singularity theorem based on the existence of marginally outer trapped surfaces (MOTS) on noncompact initial data sets for globally hyperbolic spacetimes. This result requires that the MOTS be generic in a suitable sense. In the same spirit, this author has proven some variants of that result which hold for weaker causal conditions on spacetime, but which concern (generic) marginally trapped surfaces (MTS) rather than MOTS, i.e., most of the results need a condition on the convergence of the ingoing family of normal null geodesics as well. However, much of the more recent literature has focused on MOTS rather than MTS as quasi-local substitutes for the description of black holes, as they are arguably more natural and easier to handle in a number of situations. It is therefore pertinent to ask to what extent…
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