We construct a stretched (aka Warped) Anti-de Sitter black hole in 3 dimensions supported by a real scalar field configuration. The latter is regular everywhere outside and on the horizon. No hair theorems in 3 dimensions demand the matter to be coupled to the curvature in a non-minimal way; however, this coupling can still be of the Horndeski type, i.e. yielding second order field equations similar to those appearing in the context of Galileon theories. These Warped-Anti-de Sitter black holes exhibit interesting thermodynamical properties, such as finite Hawking temperature and entropy. We compute the black hole entropy in the gravity theory and speculate with the possibility of this to admit a microscopic description in terms of a dual (W...
A holographic description of three-dimensional warped black holes suffers from ambiguities due to a ...
15 pagesInternational audienceWe investigate stationary, rotationally symmetric solutions of a recen...
In this paper, we analytically calculate the quasinormal modes of scalar, vector, tensor, and spinor...
We construct a stretched (aka warped) anti-de Sitter black hole in three dimensions supported by a r...
We study a new class of solutions of three-dimensional topological massive gravity. These solutions ...
We provide a simple holographic description for a warped conformal field theory (WCFT) at finite tem...
Abstract: We consider warped AdS3 black holes in generic higher derivatives gravity theories in 2+1 ...
International audienceIn three-dimensional de Sitter space classical black holes do not exist, and t...
International audienceIn three-dimensional de Sitter space classical black holes do not exist, and t...
International audienceIn three-dimensional de Sitter space classical black holes do not exist, and t...
In this paper we apply the thermodynamics method to investigate the holographic pictures for the BTZ...
We study regular spacelike warped black holes in the three dimensional general massive gravity model...
In the context of warped conformal field theories (WCFT), the derivation of the warped Cardy formula...
We analytically calculate the quasi-normal modes of various perturbations of the spacelike stretched...
15 pagesInternational audienceWe investigate stationary, rotationally symmetric solutions of a recen...
A holographic description of three-dimensional warped black holes suffers from ambiguities due to a ...
15 pagesInternational audienceWe investigate stationary, rotationally symmetric solutions of a recen...
In this paper, we analytically calculate the quasinormal modes of scalar, vector, tensor, and spinor...
We construct a stretched (aka warped) anti-de Sitter black hole in three dimensions supported by a r...
We study a new class of solutions of three-dimensional topological massive gravity. These solutions ...
We provide a simple holographic description for a warped conformal field theory (WCFT) at finite tem...
Abstract: We consider warped AdS3 black holes in generic higher derivatives gravity theories in 2+1 ...
International audienceIn three-dimensional de Sitter space classical black holes do not exist, and t...
International audienceIn three-dimensional de Sitter space classical black holes do not exist, and t...
International audienceIn three-dimensional de Sitter space classical black holes do not exist, and t...
In this paper we apply the thermodynamics method to investigate the holographic pictures for the BTZ...
We study regular spacelike warped black holes in the three dimensional general massive gravity model...
In the context of warped conformal field theories (WCFT), the derivation of the warped Cardy formula...
We analytically calculate the quasi-normal modes of various perturbations of the spacelike stretched...
15 pagesInternational audienceWe investigate stationary, rotationally symmetric solutions of a recen...
A holographic description of three-dimensional warped black holes suffers from ambiguities due to a ...
15 pagesInternational audienceWe investigate stationary, rotationally symmetric solutions of a recen...
In this paper, we analytically calculate the quasinormal modes of scalar, vector, tensor, and spinor...