Radial Gravitational Collapse Causes Timelike Incompleteness
arXiv:2401.16297 · doi:10.1103/PhysRevD.109.084034
Abstract
We show that a globally hyperbolic spacetime containing a trapped surface and satisfying the strong energy condition and a condition on certain radial tidal forces must be timelike geodesically incomplete. This constitutes a "timelike" version of Penrose's celebrated singularity theorem. Recall that the latter concludes that certain spacetimes are null incomplete, providing the first theoretical evidence that black holes actually exist in our Universe. By concluding timelike instead of null incompleteness, we obtain, at the expense of stronger assumptions, a clearer physical interpretation and the existence of an event horizon.
arXiv commentSlightly updated exposition, 5 pages
References in corpus (7)
- On smooth Cauchy hypersurfaces and Geroch's splitting theorem
- Singularity theorems based on trapped submanifolds of arbitrary co-dimension
- Singularity theorems for -Lorentzian metrics
- Penrose's 1965 singularity theorem: From geodesic incompleteness to cosmic censorship
- The Hawking-Penrose singularity theorem for -Lorentzian metrics
- A gravitational collapse singularity theorem consistent with black hole evaporation
- A new singularity theorem for black holes which allows chronology violation in the interior