Asymptotically flat black holes in 2+1 dimensions
Gokhan Alkac, Ercan Kilicarslan, Bayram Tekin

TL;DR
This paper explores various black hole solutions, including black flowers and radiating black holes, in 2+1 dimensional extended massive gravity theories, revealing their unique properties and differences from Einstein gravity.
Contribution
It demonstrates the existence of black flower solutions in extended massive gravity theories and shows they do not occur in Einstein gravity with perfect fluids.
Findings
Black flower solutions appear in extended massive gravity.
These solutions also solve Born-Infeld extended theories.
New conformally flat radiating solutions are found.
Abstract
Asymptotically flat black holes in dimensions are a rarity. We study the recently found black flower solutions (asymptotically flat black holes with deformed horizons), static black holes, rotating black holes and the dynamical black flowers (black holes with radiative gravitons ) of the purely quadratic version of new massive gravity. We show how they appear in this theory and we also show that they are also solutions to the infinite order extended version of the new massive gravity, that is the Born-Infeld extension of new massive gravity with an amputated Einsteinian piece. The same metrics also solve the topologically extended versions of these theories, with modified conserved charges and the thermodynamical quantities, such as the Wald entropy. Besides these we find new conformally flat radiating type solutions to these extended gravity models. We also show that these…
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.
