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Black hole scan

Juan CrisóstomoCentro de Estudios Científicos, CECS, Casilla 1469, Valdivia, ChileRicardo TroncosoCentro de Estudios Científicos, CECS, Casilla 1469, Valdivia, ChileJorge ZanelliCentro de Estudios Científicos, CECS, Casilla 1469, Valdivia, Chile
2000en
ABI

Аннотация

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 $k=1,2,\dots{},[(d\ensuremath{-}1)/2].$ 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 $d\ensuremath{-}2k=1,$ these solutions resemble the three dimensional black hole; otherwise, their behavior is similar to the Schwarzschild-${\mathrm{AdS}}_{4}$ geometry.

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Цитирований: 2Использованных источников: 0