Rotating black holes with Nil or SL(2,$\,\mathbb{R}$) horizons

We construct rotating black holes in $N=2$, $D=5$ minimal and matter-coupled gauged supergravity, with horizons that are homogeneous but not isotropic. Such spaces belong to the eight Thurston model geometries, out of which we consider the cases Nil and SL$(2,\mathbb{R})$. In the former, we use the...

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Bibliographic Details
Published in:Journal of High Energy Physics
Main Authors: Federico Faedo, Silke Klemm, Pietro Mariotti
Other Authors: F.M. Faedo, S. Klemm, P. Mariotti
Format: Article in Journal/Newspaper
Language:English
Published: Springer : Societa Italiana di Fisica 2023
Subjects:
Online Access:https://hdl.handle.net/2434/970637
https://doi.org/10.1007/JHEP05(2023)138
http://arxiv.org/abs/2212.04890v2