Artículo
Extremal surfaces and thin-shell wormholes
Fecha de publicación:
10/2022
Editorial:
American Physical Society
Revista:
Physical Review D: Particles, Fields, Gravitation and Cosmology
ISSN:
1550-7998
e-ISSN:
2470-0029
Idioma:
Inglés
Tipo de recurso:
Artículo publicado
Clasificación temática:
Resumen
We study extremal surfaces in a traversable wormhole geometry that connects two locally AdS5 asymptotic regions. In the context of the AdS/CFT correspondence, we use these to compute the holographic entanglement entropy for different configurations: First, we consider an extremal surface anchored at the boundary on a spatial 2-sphere of radius R. The other scenario is a slab configuration which extends in two of the boundary spacelike directions while having a finite size L in the third one. We show that in both cases the divergent and the finite pieces of the holographic entanglement entropy give results consistent with the holographic picture and this is used to explore the phase transitions that the dual theory undergoes. The geometries we consider here are stable thin-shell wormholes with flat codimension-one hypersurfaces at fixed radial coordinate. They appear as electrovacuum solutions of higher-curvature gravity theories coupled to Abelian gauge fields. The presence of the thin shells produces a refraction of the extremal surfaces in the bulk, leading to the presence of cusps in the phase space diagram. Further, the traversable wormhole captures a phase transition for the subsystems made up of a union of disconnected regions in different boundaries. We discuss these and other features of the phase diagram.
Palabras clave:
HOLOGRAPHY
,
ENTANGLEMENT
,
ENTROPY
,
WORMHOLES
Archivos asociados
Licencia
Identificadores
Colecciones
Articulos(IFIBA)
Articulos de INST.DE FISICA DE BUENOS AIRES
Articulos de INST.DE FISICA DE BUENOS AIRES
Citación
Chernicoff, Mariano; Giribet, Gaston Enrique; Rubín de Celis, Emilio; Extremal surfaces and thin-shell wormholes; American Physical Society; Physical Review D: Particles, Fields, Gravitation and Cosmology; 106; 8; 10-2022; 1-16
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