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A Cardy formula for off-diagonal three-point coefficients; or, how the geometry behind the horizon gets disentangled
by
Romero-Bermúdez, Aurelio
, Schalm, Koenraad
, Sabella-Garnier, Philippe
in
AdS-CFT Correspondence
/ Classical and Quantum Gravitation
/ Conformal Field Theory
/ Elementary Particles
/ Entanglement
/ Geometry
/ High energy physics
/ Operators (mathematics)
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ String Theory
2018
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A Cardy formula for off-diagonal three-point coefficients; or, how the geometry behind the horizon gets disentangled
by
Romero-Bermúdez, Aurelio
, Schalm, Koenraad
, Sabella-Garnier, Philippe
in
AdS-CFT Correspondence
/ Classical and Quantum Gravitation
/ Conformal Field Theory
/ Elementary Particles
/ Entanglement
/ Geometry
/ High energy physics
/ Operators (mathematics)
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ String Theory
2018
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A Cardy formula for off-diagonal three-point coefficients; or, how the geometry behind the horizon gets disentangled
by
Romero-Bermúdez, Aurelio
, Schalm, Koenraad
, Sabella-Garnier, Philippe
in
AdS-CFT Correspondence
/ Classical and Quantum Gravitation
/ Conformal Field Theory
/ Elementary Particles
/ Entanglement
/ Geometry
/ High energy physics
/ Operators (mathematics)
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ String Theory
2018
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A Cardy formula for off-diagonal three-point coefficients; or, how the geometry behind the horizon gets disentangled
Journal Article
A Cardy formula for off-diagonal three-point coefficients; or, how the geometry behind the horizon gets disentangled
2018
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Overview
A
bstract
In the AdS/CFT correspondence eternal black holes can be viewed as a specific entanglement between two copies of the CFT: the thermofield double. The statistical CFT Wightman function can be computed from a geodesic between the two boundaries of the Kruskal extended black hole and therefore probes the geometry behind the horizon. We construct a kernel for the AdS
3
/CFT
2
Wightman function that is independent of the entanglement. This kernel equals the average off-diagonal matrix element squared of a primary operator. This allows us to compute the Wightman function for an arbitrary entanglement between the double copies and probe the emergent geometry between a leftand right-CFT that are not thermally entangled.
Publisher
Springer Berlin Heidelberg,Springer Nature B.V,SpringerOpen
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