Artículo
Critical points of warped AdS/CFT and higher-curvature gravity
Fecha de publicación:
12/2022
Editorial:
American Physical Society
Revista:
Physical Review D
ISSN:
2470-0010
e-ISSN:
2470-0029
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
Warped anti-de Sitter (WAdS)/warped conformal field theory (WCFT) correspondence is an interesting realization of non-AdS holography. It relates three-dimensional warped anti-de Sitter (WAdS3) spaces to a special class of two-dimensional quantum field theory with chiral scaling symmetry that acts only on right-moving modes. The latter are often called warped conformal field theories (WCFT2), and their existence makes WAdS/WCFT particularly interesting as a tool to investigate a new type of two-dimensional conformal structure. Besides, WAdS/WCFT is interesting because it enables one to apply holographic techniques to the microstate counting problem of non-AdS, nonsupersymmetric black holes. Asymptotically WAdS3 black holes (WBH3) appear as solutions of topologically massive theories, Chern-Simons theories, and many other models. Here, we explore WBH3×ςD-3 solutions of D-dimensional higher-curvature gravity, with ςD-3 being different internal manifolds, typically given by products of deformations of hyperbolic spaces, although we also consider warped products with time-dependent deformations. These geometries are solutions of the second order higher-curvature theory at special (critical) points of the parameter space, where the theory exhibits a sort of degeneracy. We argue that the dual (W)CFT at those points is actually trivial. In many respects, these critical points of WAdS3×ςD-3 vacua are the squashed/stretched analogs of the AdSD Chern-Simons point of Lovelock gravity.
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Articulos(IAFE)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)
Citación
Caselli, Gerónimo; Giribet, Gaston; Goya, Andrés Fabio; Critical points of warped AdS/CFT and higher-curvature gravity; American Physical Society; Physical Review D; 106; 12; 12-2022; 126026-126037
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