2011
DOI: 10.1103/physrevd.83.106009
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Constructing local bulk observables in interacting AdS/CFT

Abstract: Local operators in the bulk of AdS can be represented as smeared operators in the dual CFT. We show how to construct these bulk observables by requiring that the bulk operators commute at spacelike separation. This extends our previous work by taking interactions into account. Large-N factorization plays a key role in the construction. We show diagrammatically how this procedure is related to bulk Feynman

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Cited by 175 publications
(348 citation statements)
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“…At higher orders in this perturbation theory we will need to confront the problem of defining local operators in a diffeomorphism invariant theory, but we postpone discussion of this until section 5. It is not obvious from the definition that the operators (2.2) have the expected commutators in the bulk; this has been checked perturbatively within low point correlation functions in [19], but must eventually break down in states with enough excitations to avoid a contradiction with the argument in our introduction. We will argue below that, within the subspace of states that are "perturbatively close" to the vacuum, it breaks down only at the level of non-perturbatively small corrections.…”
Section: Jhep04(2015)163mentioning
confidence: 85%
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“…At higher orders in this perturbation theory we will need to confront the problem of defining local operators in a diffeomorphism invariant theory, but we postpone discussion of this until section 5. It is not obvious from the definition that the operators (2.2) have the expected commutators in the bulk; this has been checked perturbatively within low point correlation functions in [19], but must eventually break down in states with enough excitations to avoid a contradiction with the argument in our introduction. We will argue below that, within the subspace of states that are "perturbatively close" to the vacuum, it breaks down only at the level of non-perturbatively small corrections.…”
Section: Jhep04(2015)163mentioning
confidence: 85%
“…We can now give a version of this argument that includes the gravitational dressing; from figure 8, we see that we should modify the previous statement to "commutes with all local operators at the boundary except at one point". Were this to hold as an operator equation in the CFT, it would now not imply that the operator in the center must be trivial in the CFT, but it would imply that this operator can be nontrivial at 19 A subtlety here is that they send their geodesics from arbitrary boundary times, but take them to be orthogonal to the boundary in the temporal direction as well as the S d−1 directions. These operators agree with ours at t = 0, which is where we will study them, but as a matter of principle we have not made their choice because we want to restrict to Schrodinger-picture operators acting on a fixed time slice at the boundary.…”
Section: Defining Local Operatorsmentioning
confidence: 99%
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“…The main limitation of these considerations is the absence of an actual reconstruction of operators with approximate bulk locality, in the spirit of [23,[49][50][51][52][53][54][55]. In this sense, we have strived to characterize horizon complementarity in the absence of an actual 'horizon', using only deep UV data.…”
Section: Discussionmentioning
confidence: 99%