Black hole scan

Juan Crisóstomo, Ricardo Troncoso, and Jorge Zanelli
Phys. Rev. D 62, 084013 – Published 22 September 2000
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Abstract

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,,[(d1)/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 d2k=1, these solutions resemble the three dimensional black hole; otherwise, their behavior is similar to the Schwarzschild-AdS4 geometry.

  • Received 29 March 2000

DOI:https://doi.org/10.1103/PhysRevD.62.084013

©2000 American Physical Society

Authors & Affiliations

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

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Issue

Vol. 62, Iss. 8 — 15 October 2000

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