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dc.contributor.author Canfora Tartaglia, Fabrizio
dc.contributor.author Corral, Cristóbal
dc.contributor.author Diez, Borja
dc.date.accessioned 2026-02-08T03:29:38Z
dc.date.available 2026-02-08T03:29:38Z
dc.date.issued 2025-04-28
dc.identifier.issn 2470-0010
dc.identifier.uri https://repositorio.uss.cl/handle/uss/20488
dc.description Publisher Copyright: © 2025 authors. Published by the American Physical Society.
dc.description.abstract Euclidean anti-de Sitter (AdS) wormholes provide a natural setup for studying the anti-de Sitter/conformal field theory (AdS/CFT) correspondence with multiple boundaries. However, from a bottom-up perspective, they cannot be embedded in the four-dimensional Einstein-AdS-Maxwell theory if these boundaries have positive curvature. Nevertheless, Maldacena and Maoz showed that this obstruction could be circumvented by introducing merons in the four-dimensional Einstein-AdS-Yang-Mills theory. In this work, we show that Euclidean-AdS wormholes also exist in the four-dimensional Einstein-AdS-Skyrme theory, whose matter sector possesses a nontrivial baryonic charge. We compute its free energy and show that it does not depend on the integration constants whatsoever, resembling topological solitons. Additionally, we obtain its holographic stress tensor and show that it vanishes, allowing us to interpret this configuration as a holographic Bogomol'nyi-Prasad-Sommerfield (BPS) state. Other topologically nontrivial ground states in Einstein-Skyrme theory are found, such as gravitational instantons, representing the homotopically inequivalent vacua of the theory. We find that they develop Hawking-Page phase transitions above a critical temperature. Some of these solutions are periodic in Euclidean time, representing the gravitational analog of calorons in Yang-Mills theory. en
dc.language.iso eng
dc.relation.ispartof vol. 111 Issue: no. 084072 Pages: 084072
dc.source Physical Review D
dc.title Euclidean AdS wormholes and gravitational instantons in the Einstein-Skyrme theory en
dc.type Artículo
dc.identifier.doi 10.1103/PhysRevD.111.084072
dc.publisher.department Facultad de Ingeniería


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