Supersymmetric isolated horizons in ADS spacetime
arXiv:0808.0905 · doi:10.1016/j.physletb.2008.10.020
Abstract
We discuss various physical aspects of nonextremal, extremal and supersymmetric black holes in asymptotically anti-de Sitter (ADS) spacetimes. Specifically, we discuss how the isolated horizon (IH) framework leads to an ambiguity-free description of rotating black holes in these spacetimes. We then apply this framework to investigate the properties of supersymmetric isolated horizons (SIHs) in four-dimensional N = 2 gauged supergravity. Among other results we find that they are necessarily extremal, that rotating SIHs must have non-trivial electromagnetic fields, and that non-rotating SIHs necessarily have constant curvature horizon cross sections and a magnetic (though not electric) charge.
15 pages, 1 figure; v2: two references added; minor corrections; to appear in Physics Letters B
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Cited by in corpus (13)
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- Uniqueness of near-horizon geometries of rotating extremal AdS(4) black holes
- Black holes and black hole thermodynamics without event horizons
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