Higher dimensional Yang-Mills black holes in third order Lovelock gravity

Details Higher dimensional Yang-Mills black holes in third order Lovelock gravity Higher dimensional Yang-Mills black holes in third order Lovelock gravity

2008-01-11

arxiv.org/abs/0801.1726v2

Phys.Lett.B665:125-130,2008

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages, 3 figures, to appear in Phys. Lett. B

Scientific paper

10.1016/j.physletb.2008.06.007

By employing the higher (N\TEXTsymbol{>}5) dimensional version of the Wu-Yang Ansatz we obtain magnetically charged new black hole solutions in the Einstein-Yang-Mills-Lovelock (EYML) theory with second ($\alpha_{2}$) and third ($\alpha_{3}$)order parameters. These parameters, where $\alpha_{2}$ is also known as the Gauss-Bonnet parameter, modify the horizons (and the resulting thermodynamical properties) of the black holes. It is shown also that asymptotically ($r\to \infty $), these parameters contribute to an effective cosmological constant -without cosmological constant- so that the solution behaves de-Sitter (Anti de-Sitter) like.

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