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Phys. Rev. D 62, 084013 (2000) [14 pages]

Black hole scan

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Juan Crisóstomo
Centro de Estudios Científicos, CECS, Casilla 1469, Valdivia, Chile
Departamento de Física, Facultad de Ciencias, Universidad de Chile, Casilla 653, Santiago, Chile

Ricardo Troncoso
Centro de Estudios Científicos, CECS, Casilla 1469, Valdivia, Chile
Physique Théorique et Mathématique, Université Libre de Bruxelles, Campus Plaine, C.P. 231, B-1050, Bruxelles, Belgium

Jorge Zanelli
Centro de Estudios Científicos, CECS, Casilla 1469, Valdivia, Chile
Departamento de Física, Universidad de Santiago de Chile, Casilla 307, Santiago 2, Chile

Received 29 March 2000; published 22 September 2000

Gravitation theories selected by requiring that they have a unique anti–de Sitter vacuum with a fixed cosmological constant are studied. For a given dimension d, the Lagrangians under consideration are labeled by an integer k=1,2,,[(d-1)/2]. Black holes for each d and k are found and are used to rank these theories. A minimum possible size for a localized electrically charged source is predicted in the whole set of theories, except general relativity. It is found that the thermodynamic behavior falls into two classes: If d-2k=1, these solutions resemble the three dimensional black hole; otherwise, their behavior is similar to the Schwarzschild-AdS4 geometry.

© 2000 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.62.084013
DOI:
10.1103/PhysRevD.62.084013
PACS:
04.50.+h, 04.20.Jb, 04.70.-s