English

New hairy black hole solutions with a dilaton potential

High Energy Physics - Theory 2009-11-10 v2 General Relativity and Quantum Cosmology

Abstract

We consider black hole solutions with a dilaton field possessing a nontrivial potential approaching a constant negative value at infinity. The asymptotic behaviour of the dilaton field is assumed to be slower than that of a localized distribution of matter. A nonabelian SU(2) gauge field is also included in the total action. The mass of the solutions admitting a power series expansion in 1/r1/r at infinity and preserving the asymptotic anti-de Sitter geometry is computed by using a counterterm subtraction method. Numerical arguments are presented for the existence of hairy black hole solutions for a dilaton potential of the form V(ϕ)=C1exp(2α1ϕ)+C2exp(2α2ϕ)+C3V(\phi)=C_1 \exp(2\alpha_1 \phi)+C_2 \exp(2\alpha_2 \phi)+C_3, special attention being paid to the case of N=4,D=4{\cal N}=4, D=4 gauged supergravity model of Gates and Zwiebach.

Keywords

Cite

@article{arxiv.hep-th/0410154,
  title  = {New hairy black hole solutions with a dilaton potential},
  author = {Eugen Radu and D. H. Tchrakian},
  journal= {arXiv preprint arXiv:hep-th/0410154},
  year   = {2009}
}

Comments

12 pages, 4 figures; v2:references added, typos corrected, small changes in Section 4