Rotating Dilaton Black Holes
Bj{\o}rn Jensen, Ulf Lindstr\"om

TL;DR
This paper investigates rotating black hole solutions in a system combining gravity, electromagnetism, and a dilaton field, revealing special cases where rotation can be generated from non-rotating solutions due to enhanced symmetries.
Contribution
It identifies the conditions under which rotating solutions can be generated from non-rotating ones in dilaton black hole systems, highlighting the role of target space symmetries for specific dilaton couplings.
Findings
Rotating solutions are only generated for specific dilaton couplings a=0, ±√3.
Target space symmetry is enlarged at these special coupling values.
New solutions are constructed using symmetry transformations.
Abstract
We consider the axially symmetric coupled system of gravitation, electromagnetism and a dilaton field. Reducing from four to three dimensions, the system is described by gravity coupled to a non-linear -model. We find the target space isometries and use them to generate new solutions. It seems that it is only possible to generate rotating solutions from non-rotating ones for the special cases when the dilaton coupling parameter . For those particular values, the target space symmetry is enlarged.
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.
