中国物理B ›› 2011, Vol. 20 ›› Issue (5): 50401-050401.doi: 10.1088/1674-1056/20/5/050401

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A new metric for rotating black holes in Gauss–Bonnet gravity

邹德成1, 杨战营1, 岳瑞宏2, 于添翼2   

  1. (1)Department of Physics, Northwest University, Xi'an 710069, China; (2)Faculty of Science, Ningbo University, Ningbo 315211, China
  • 收稿日期:2010-11-08 修回日期:2010-12-27 出版日期:2011-05-15 发布日期:2011-05-15
  • 基金资助:
    Project supported by the National Natural Science Foundation of China (Grant Nos. 10875060, 10975180 and 11047025).

A new metric for rotating black holes in Gauss–Bonnet gravity

Yue Rui-Hong (岳瑞宏)aZou De-Cheng (邹德成)b, Yu Tian-Yi (于添翼)a, Yang Zhan-Ying (杨战营)b    

  1. a Faculty of Science, Ningbo University, Ningbo 315211, China; b Department of Physics, Northwest University, Xi'an 710069, China
  • Received:2010-11-08 Revised:2010-12-27 Online:2011-05-15 Published:2011-05-15
  • Supported by:
    Project supported by the National Natural Science Foundation of China (Grant Nos. 10875060, 10975180 and 11047025).

摘要: This paper presents a new metric and studies slowly rotating Gauss–Bonnet black holes with a 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.

关键词: Gauss–Bonnet gravity, slow rotation, anti-de Sitter spaces

Abstract: This paper presents a new metric and studies slowly rotating Gauss–Bonnet black holes with a 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.

Key words: Gauss–Bonnet gravity, slow rotation, anti-de Sitter spaces

中图分类号:  (Higher-dimensional gravity and other theories of gravity)

  • 04.50.-h
04.65.+e (Supergravity)