71 research outputs found
Static near-horizon geometries in five dimensions
We consider the classification of static near-horizon geometries of
stationary extremal (not necessarily BPS) black hole solutions of five
dimensional Einstein-Maxwell theory coupled to a Chern-Simons term with
coupling xi (with xi=1 corresponding to supergravity). Assuming the black holes
have two rotational symmetries, we show that their near-horizon geometries are
either the direct product AdS_3 X S^2 or a warped product of AdS_2 and compact
3d space. In the AdS_2 case we are able to classify all possible near-horizon
geometries with no magnetic fields. There are two such solutions: the direct
product AdS_2 X S^3 as well as a warped product of AdS_2 and an inhomogeneous
S^3. The latter solution turns out to be near-horizon limit of an extremal
Reissner-Nordstrom black hole in an external electric field. In the AdS_2 case
with magnetic fields, we reduce the problem (in all cases) to a single
non-linear ODE. We show that if there are any purely magnetic solutions of this
kind they must have S^1 X S^2 horizon topology, and for xi^2 <1/4 we find
examples of solutions with both electric and magnetic fields.Comment: Latex, 28 pages. v2: minor changes, reference adde
Classification of near-horizon geometries of extremal black holes
Any spacetime containing a degenerate Killing horizon, such as an extremal
black hole, possesses a well-defined notion of a near-horizon geometry. We
review such near-horizon geometry solutions in a variety of dimensions and
theories in a unified manner. We discuss various general results including
horizon topology and near-horizon symmetry enhancement. We also discuss the
status of the classification of near-horizon geometries in theories ranging
from vacuum gravity to Einstein-Maxwell theory and supergravity theories.
Finally, we discuss applications to the classification of extremal black holes
and various related topics. Several new results are presented and open problems
are highlighted throughout.Comment: 70 pages; invited review article for Living Reviews in Relativity; v2
some improvements and references adde
Integrability and the Kerr-(A)dS black hole in five dimensions
In this note we prove that the Hamilton-Jacobi equation for a particle in the
five dimensional Kerr-(A)dS black hole is separable, for arbitrary rotation
parameters. As a result we find an irreducible Killing tensor. We also consider
the Klein-Gordon equation in this background and show that this is also
separable. Finally we comment on extensions and implications of these results.Comment: 4 pages, RevTeX. v2: minus sign typos in eq. (17) and (18) of
published version correcte
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