2020
DOI: 10.1007/jhep11(2020)167
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Knitting wormholes by entanglement in supergravity

Abstract: We construct a single-boundary wormhole geometry in type IIB supergravity by perturbing two stacks of N extremal D3-branes in the decoupling limit. The solution interpolates from a two-sided planar AdS-Schwarzschild geometry in the interior, through a harmonic two-center solution in the intermediate region, to an asymptotic AdS space. The construction involves a CPT twist in the gluing of the wormhole to the exterior throats that gives a global monodromy to some coordinates, while preserving orientability. The… Show more

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Cited by 9 publications
(5 citation statements)
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“…In this setting, the ER=EPR principle says that this entanglement can be geometrized as a wormhole that connects the black hole interior to the far radiation region. Much effort has gone into making this idea concrete, including the development of stringy models [47], large supergravity wormholes 3 created by entanglement [50], and toy models which exhibit phase transitions driven by coupling [46,[51][52][53] or entanglement [33].…”
Section: An Example: Er=epr From a Classical Scalar Fieldmentioning
confidence: 99%
“…In this setting, the ER=EPR principle says that this entanglement can be geometrized as a wormhole that connects the black hole interior to the far radiation region. Much effort has gone into making this idea concrete, including the development of stringy models [47], large supergravity wormholes 3 created by entanglement [50], and toy models which exhibit phase transitions driven by coupling [46,[51][52][53] or entanglement [33].…”
Section: An Example: Er=epr From a Classical Scalar Fieldmentioning
confidence: 99%
“…In the UV complete realization in terms of multiple AdS throats, one might of course ask whether there could be wormhole configurations that join these individual throats, perhaps via some generalization of the construction presented in [56]. The general point is that our construction only mimics an ensemble average provided we have sufficient statistics.…”
Section: Holographic Interpretationmentioning
confidence: 99%
“…In this setting, the ER = EPR principle says that this entanglement can be geometrized as a wormhole that connects the black hole interior to the far radiation region. Much effort has gone into making this idea concrete, including the development of stringy models [49][50][51], large supergravity wormholes 10 created by entanglement [54], and toy models which exhibit phase transitions driven by coupling [47,[55][56][57] or entanglement [33].…”
Section: An Example: Er = Epr From a Classical Scalar Fieldmentioning
confidence: 99%