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Phys. Rev. D 49, 975–986 (1994)

Dimensionally continued black holes

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Máximo Bañados*
Centro de Estudios Científicos de Santiago, Casilla 16443, Santiago 9, Chile
Departamento de Física, Facultad de Ciencias, Universidad de Chile, Casilla 653, Santiago, Chile

Claudio Teitelboim*
Centro de Estudios Científicos de Santiago, Casilla 16443, Santiago 9, Chile
Institute for Advanced Study, Olden Lane, Princeton, New Jersey 08540

Jorge Zanelli*
Centro de Estudios Científicos de Santiago, Casilla 16443, Santiago 9, Chile
Departamento de Física, Facultad de Ciencias, Universidad de Chile, Casilla 653, Santiago, Chile

Received 23 July 1993; published in the issue dated 15 January 1994

Static, spherically symmetric solutions of the field equations for a particular dimensional continuation of general relativity with a negative cosmological constant are studied. The action is, in odd dimensions, the Chern-Simons form for the anti-de Sitter group and, in even dimensions, the Euler density constructed with the Lorentz part of the anti-de Sitter curvature tensor. Both actions are special cases of the Lovelock action, and they reduce to the Hilbert action (with a negative cosmological constant) in the lower dimensional cases D=3 and D=4. Exact black hole solutions characterized by mass (M) and electric charge (Q) are found. In odd dimensions a negative cosmological constant is necessary to obtain a black hole, while in even dimensions both asymptotically flat and asymptotically anti-de Sitter black holes exist. The causal structure is analyzed and the Penrose diagrams are exhibited. The curvature tensor is singular at the origin for all dimensions greater than three. In dimensions of the form D=4k,4k-1, the number of horizons may be zero, one, or two, depending on the relative values of M and Q, while for a negative mass there is no horizon for any real value of Q. In the other cases, D=4k+1,4k+2, both naked and dressed singularities with a positive mass exist. As in three dimensions, in all odd dimensions anti-de Sitter space appears as a "bound state" of mass M=-1, separated from the continuous spectrum (M≥0) by a gap of naked curvature singularities. In even dimensions anti-de Sitter space has zero mass. The analysis is Hamiltonian throughout, considerably simplifying the discussion of the boundary terms in the action and the thermodynamics. The Euclidean black hole has the topology R2×SD-2. Evaluation of the Euclidean action gives explicit expressions for all the relevant thermodynamical parameters of the system. The entropy, defined as a surface term in the action coming from the horizon, is shown to be a monotonically increasing function of the black hole radius, different from the area for D>4.

© 1994 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.49.975
DOI:
10.1103/PhysRevD.49.975
PACS:
97.60.Lf, 04.20.Jb

*Electronic address: cecsphy@lascar.puc.cl