Cosmological black holes on Taub–NUT space in five-dimensional Einstein–Maxwell theory

2007/02/28 by Daisuke Ida, Hideki Ishihara, Masashi Kimura +3
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #hep-th

paper · pdf · doi:10.1088/0264-9381/24/13/001

published as Class.Quant.Grav.24:3141-3150,2007 · 12 pages, 4 figures, some minor corrections, to be published in Classical and Quantum Gravity

arxiv created 2007/05/29 · openalex publication_date 2007/06/12 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/30

Abstract

The cosmological black hole solution on the Gibbons–Hawking space has been constructed. We also investigate the properties of this solution in the case of a single-black hole. Unlike the Kastor–Traschen solution, which becomes a static solution in a single-black hole, this solution is not static even in a single-black hole case.

Citations

• A Class of Exact Solutions of Einstein's Field Equations
• Topology change of coalescing black holes on Eguchi–Hanson space
• A rotating Kaluza–Klein black hole with squashed horizons
• Testing cosmic censorship with black hole collisions