pith. sign in

arxiv: 1806.01849 · v2 · pith:EAP3GUNGnew · submitted 2018-06-05 · ✦ hep-th · gr-qc

Evidence for the existence of a novel class of supersymmetric black holes with AdS₅timesS⁵ asymptotics

classification ✦ hep-th gr-qc
keywords blackholessupersymmetrichairysolutionssupergravityasymptoticscharged
0
0 comments X p. Extension
pith:EAP3GUNG Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{EAP3GUNG}

Prints a linked pith:EAP3GUNG badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We construct a new class of charged, rotating hairy black holes in a consistent truncation of $\mathcal{N} = 8$ supergravity, which retains one charged scalar field and a U$(1)$ gauge field. These hairy solutions can be uplifted to solutions of type IIB supergravity with AdS$_5\times$S$^5$ asymptotics. We find rotating hairy black holes with finite entropy arbitrarily close to the supersymmetric bound - the resulting supersymmetric solution is a one-parameter extension of the Gutowski-Reall solution. These solutions have finite curvature invariants (including at extremality), but in the extremal limit exhibit diverging tidal forces in the near horizon region. Nevertheless, we argue that these limiting supersymmetric black holes can be consistently studied within the supergravity approximation.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Charged, rotating black holes in Einstein-Maxwell-dilaton theory

    gr-qc 2025-06 unverdicted novelty 7.0

    Numerical construction of asymptotically flat charged rotating black holes in EMd theory for arbitrary dilaton coupling gamma, with analysis of parameter space, zero-temperature limits, and hints of non-uniqueness.