Classification and stability of black hole event horizon births: a contact geometry approach
Oscar Meneses Rojas

TL;DR
This paper applies contact geometry and singularity theory to classify and analyze the stability of black hole event horizon formation, focusing on crease sets and caustics using Legendrian projections.
Contribution
It extends the classification of black hole crease sets by incorporating stability analysis within a contact geometry framework, refining prior approaches.
Findings
Classified crease sets and caustics using Legendrian projections.
Refined stability analysis of horizon birth components.
Identified additional crease set components connected to null infinity.
Abstract
A classical result by Penrose establishes that null geodesics generating a black hole event horizon can only intersect at their entrance to the horizon in ``crossover'' points. This points together with limit points of this set, namely caustics, form the so-called "crease set". Light rays enter into the horizon through the crease set, characterizing the latter as the birth of the horizon. A natural question in this context refers to the classification and stability of the structural possibilities of black hole crease sets. In this work we revisit the strategy adopted by Gadioux & Reall for such a classification in the setting of singularity theory in contact geometry. Specifically, in such contact geometry setting, the event horizon is identified as a component (not connected to null infinity) of a so-called ``BigFront''. The characterization of BigFronts as Legendrian projections of…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Astrophysical Phenomena and Observations · Geometric Analysis and Curvature Flows
