Formation of Black Holes in Topologically Massive Gravity
Ivo Sachs
TL;DR
This paper introduces an exact solution in 3D topologically massive gravity that models black hole formation and horizon dynamics within a chiral AdS pp-wave spacetime.
Contribution
It provides a novel exact solution demonstrating black hole formation and horizon evolution in topologically massive gravity with negative cosmological constant.
Findings
Exact solution interpolates between past horizon and chiral AdS pp-wave.
Time reversal yields an AdS pp-wave with a future event horizon.
Advances understanding of horizon dynamics in 3D gravity theories.
Abstract
We present an exact solution in 3-dimensional topologically massive gravity with negative cosmological constant which dynamically interpolates between a past horizon and a chiral AdS pp-wave. Similarly, upon time reversal, one obtains an AdS pp-wave with a future event horizon
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.