2008/01/31 by Y. Brihaye, Yves Brihaye, Eugen Radu +1 · 7 citations
Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Black hole (networking) #Classical mechanics #Cosmological constant #Cosmology and Gravitation Theories #Einstein #Entropy (arrow of time) #Gauss #Gauss–Bonnet theorem #Horizon #Mathematical physics #Physics #Quantum mechanics #Spacetime #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.1016/j.physletb.2008.02.005
published as Phys.Lett.B661:167-174,2008 · 10 pages, 6 figures, references added, minor modifications, typos corrected
openalex publication_date 2008/02/08 · arxiv created 2008/03/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We present arguments for the existence of five-dimensional rotating black holes with equal magnitude angular momenta in Einstein–Gauss–Bonnet theory with negative cosmological constant. These solutions posses a regular horizon of spherical topology and approach asymptotically an anti-de Sitter spacetime background. We discuss the general properties of these solutions and, using an adapted counterterm prescription, we compute their entropy and conserved charges.