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

2010/09/18 by Shinya Tomizawa, Tomizawa, Shinya · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #High Energy Physics - Theory (hep-th) #Pulsars and Gravitational Waves Research

paper · pdf · doi:10.48550/arxiv.1009.3568

openalex publication_date 2010/09/18 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

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.

Cited by

• Four-charge static non-extremal black holes in the five-dimensional N=2, STU-W²U supergravity

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