2011/05/01 by Rui-Hong Yue, De-Cheng Zou, Tian-Yi Yu +1
Physics and Astronomy · #Angular momentum #Astrophysical Phenomena and Observations #Binary black hole #Black Holes and Theoretical Physics #Black hole (networking) #Cosmology and Gravitation Theories #Hawking radiation #Kerr metric #Metric (unit) #Rotating black hole #gr-qc #hep-th
paper · pdf · doi:10.1088/1674-1056/20/5/050401
published as Chin.Phys.B20:050401,2011 · 9 pages
openalex publication_date 2011/05/01 · arxiv created 2011/07/14 · arxiv updated 2011/10/04 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
This paper presents a new metric and studies slowly rotating Gauss-Bonnet black holes with one nonvanishing angular momentum in five dimensional anti-de Sitter spaces. Taking the angular momentum parameter a up to second order, the slowly rotating black hole solutions are obtained by working directly in the action. In addition, it also finds that this method is applicable in higher order Lovelock gravity.