Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
1995-02-08
Class.Quant.Grav.12:1753-1770,1995; ERRATUM-ibid.12:2355,1995
Physics
High Energy Physics
High Energy Physics - Theory
24 pages, phyzzx, epsf, 7 in-text figures. Small addition to introduction, and a few extra references
Scientific paper
10.1088/0264-9381/12/7/017
The properties of static spherically symmetric black holes, which are both electrically and magnetically charged, and which are coupled to the dilaton in the presence of a cosmological constant, Lambda, are considered. It is shown that apart from the Reissner-Nordstrom-de Sitter solution with constant dilaton, such solutions do not exist if Lambda > 0 (in arbitrary spacetime dimension >=4 ). However, asymptotically anti-de Sitter dyonic black hole solutions with a non-trivial dilaton do exist if Lambda < 0. Both these solutions and the asymptotically flat (Lambda = 0) solutions are studied numerically for arbitrary values of the dilaton coupling parameter, g_0, in four dimensions. The asymptotically flat solutions are found to exhibit two horizons if g_0 = 0, 1, \sqrt{3}, \sqrt{6}, ..., \sqrt{n(n+1)/2},..., and one horizon otherwise. For asymptotically anti-de Sitter solutions the result is similar, but the corresponding values of g_0 are altered in a non-linear fashion which depends on Lambda and the mass and charges of the black holes. All dyonic solutions with Lambda <= 0 are found to have zero Hawking temperature in the extreme limit, however, regardless of the value of g_0.
Poletti Stephen J.
Twamley Jason
Wiltshire David L.
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