Stationary Lifshitz black holes of R^2-corrected gravity theory
Ozgur Sarioglu

TL;DR
This paper generalizes static Lifshitz black holes in R^2-corrected gravity to include rotation, providing exact solutions that encompass the BTZ black hole as a special case, thus broadening the understanding of such solutions.
Contribution
It introduces a new class of stationary Lifshitz black hole solutions in R^2 gravity, extending previous static solutions and connecting to the BTZ black hole in three dimensions.
Findings
Derived exact stationary Lifshitz black hole solutions.
Showed solutions reduce to BTZ black hole in specific limits.
Expanded the landscape of analytic solutions in R^2 gravity.
Abstract
In this short note, I present a generalization of a set of static D-dimensional (D >= 3) Lifshitz black holes, which are solutions of the gravitational model obtained by amending the cosmological Einstein theory with the addition of only the curvature-scalar-squared term and that are described by two parameters, to a more general class of exact, analytic solutions that involves an additional parameter which now renders them stationary. In the special D=3 and the dynamical exponent z=1 case, the parameters can be adjusted so that the solution becomes identical to the celebrated BTZ black hole metric.
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.
