Charged black holes in a rotating Gross–Perry–Sorkin monopole background

2008/07/10 by Shinya Tomizawa, Akihiro Ishibashi · 3 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #hep-th

paper · pdf · doi:10.1088/0264-9381/25/24/245007

published as Class.Quant.Grav.25:245007,2008 · 25 pages, 6 figures

arxiv created 2008/07/10 · openalex publication_date 2008/11/27 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

We present a new class of stationary charged black hole solutions to five-dimensional Einstein–Maxwell–Chern–Simons theories. We construct the solutions by utilizing so-called the squashing transformation. At infinity, our solutions behave as a four-dimensional flat spacetime plus a 'circle' and hence describe a Kaluza–Klein black hole. More precisely, our solutions can be viewed as a charged rotating black hole in a rotating Gross–Perry–Sorkin monopole background with the black hole rotation induced from the background rotation.

Citations

• Mass and free energy in the thermodynamics of squashed Kaluza–Klein black holes
• D--branes and Spinning Black Holes
• A rotating Kaluza–Klein black hole with squashed horizons
• Large Mass Hierarchy from a Small Extra Dimension

Cited by

• Charged rotating Kaluza-Klein black holes in dilaton gravity
• Coset for Hopf fibration and squashing
• Extremal Kerr/CFT correspondence of five-dimensional rotating (charged) black holes with squashed horizons