Dilaton black holes in the de Sitter or anti–de Sitter universe

Chang Jun Gao and Shuang Nan Zhang
Phys. Rev. D 70, 124019 – Published 16 December 2004

Abstract

Poletti and Wiltshire have shown that, with the exception of a pure cosmological constant, the solution of a dilaton black hole in the background of de Sitter or anti–de Sitter universe, does not exist in the presence of one Liouville-type dilaton potential. In this work we obtain the dilaton black-hole solutions in the background of the de Sitter or anti–de Sitter universe, with the combination of three Liouville-type dilaton potentials.

  • Received 9 October 2004

DOI:https://doi.org/10.1103/PhysRevD.70.124019

©2004 American Physical Society

Authors & Affiliations

Chang Jun Gao1,* and Shuang Nan Zhang1,2,3,4,†

  • 1Department of Physics and Center for Astrophysics, Tsinghua University, Beijing 100084, China‡
  • 2Physics Department, University of Alabama, Huntsville, Alabama 35899, USA
  • 3Space Science Laboratory, NASA Marshall Space Flight Center, SD50, Huntsville, Alabama 35812, USA
  • 4Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100039, China

  • *Email address: gaocj@mail.tsinghua.edu.cn
  • Email address: zhangsn@mail.tsinghua.edu.cn
  • Mailing address.

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Issue

Vol. 70, Iss. 12 — 15 December 2004

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