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dc.date.accessioned 2020-02-20T13:18:54Z
dc.date.available 2020-02-20T13:18:54Z
dc.date.issued 2019-04-03
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/89434
dc.description.abstract We have recently presented a geometry dual to a Schwinger-Keldysh closed time contour, with two equal β/2 length Euclidean sections, which can be thought of as dual to the Thermo Field Dynamics formulation of the boundary CFT. In this work we study non-perturbative holographic excitations of the thermal vacuum by turning on asymptotic Euclidean sources. In the large-N approximation the states are found to be thermal coherent states and we manage to compute its eigenvalues. We pay special attention to the high temperature regime where the manifold is built from pieces of Euclidean and Lorentzian black hole geometries. In this case, the real time segments of the Schwinger-Keldysh contour get connected by an Einstein-Rosen wormhole through the bulk, which we identify as the exterior of a single maximally extended black hole. The Thermal-AdS case is also considered but, the Lorentzian regions become disconnected, its results mostly follows from the zero temperature case. en
dc.language en es
dc.subject AdS-CFT Correspondence es
dc.subject Black Holes es
dc.subject Thermal Field Theory es
dc.title Holographic excited states in AdS black holes en
dc.type Articulo es
sedici.identifier.other https://doi.org/10.1007/JHEP04(2019)028 es
sedici.identifier.issn 1029-8479 es
sedici.creator.person Botta Cantcheff, Marcelo Ángel Nicolás es
sedici.creator.person Martínez, Pedro Jorge es
sedici.creator.person Silva, Guillermo Ariel es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nd/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Journal of High Energy Physics es
sedici.relation.journalVolumeAndIssue 2019 es


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Creative Commons Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NoDerivatives 4.0 International (CC BY-ND 4.0)