pith. sign in

arxiv: 1009.3568 · v1 · pith:WAUHTHO2new · submitted 2010-09-18 · ✦ hep-th

Compactified black holes in five-dimensional U(1)**3 ungauged supergravity

classification ✦ hep-th
keywords blackfive-dimensionalholessolutionssupergravityungaugedasymptoticsbehave
0
0 comments X
read the original abstract

We present stationary, nonextremal three charge rotating black hole solutions in the five-dimensional U(1)^3 ungauged supergravity. At infinity, our solutions behave as a four-dimensional flat spacetime with a compact extra-dimension and hence describe spherical black holes with Kaluza-Klein asymptotics.

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. Static four-charge squashed black hole in five-dimensional $STU-W^2U$ supergravity and its thermodynamics

    hep-th 2026-01 unverdicted novelty 5.0

    The paper derives an exact static Kaluza-Klein black hole with four electric charges and squashed S3 horizon in 5D STU-W2U supergravity and verifies that its thermodynamics obey the first law and Bekenstein-Smarr form...