2014
DOI: 10.1007/jhep08(2014)145
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Universality of long-distance AdS physics from the CFT bootstrap

Abstract: Abstract:We begin by explicating a recent proof of the cluster decomposition principle in AdS ≥4 from the CFT ≥3 bootstrap. The CFT argument also computes the leading interactions between distant objects in AdS ≥4 , and we confirm the universal agreement between the CFT bootstrap and AdS gravity in the semi-classical limit.We proceed to study the generalization to CFT 2 , which requires knowledge of the Virasoro conformal blocks in a lightcone OPE limit. We compute these blocks in a semiclassical, large centra… Show more

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Cited by 372 publications
(858 citation statements)
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“…The light cone limit of crossing equations has proved useful for studying the large spin asymptotics of the operator spectrum [57,58,[123][124][125][126][127][128][129][130]. Here we analyze the crossing equation (4.13) in the light cone limit.…”
Section: Appendix C: Light Cone Limitmentioning
confidence: 99%
“…The light cone limit of crossing equations has proved useful for studying the large spin asymptotics of the operator spectrum [57,58,[123][124][125][126][127][128][129][130]. Here we analyze the crossing equation (4.13) in the light cone limit.…”
Section: Appendix C: Light Cone Limitmentioning
confidence: 99%
“…So essentialy we have a CFT with a large symmetry group that has a bulk dual, and also having two equi-dimensional scalars. This picture is similar to [63], except we have two scalars instead of one. We will match the anomalous dimensions for the O(2) model in the field theory with this picture on the holographic side.…”
Section: Holographic Calculation: Example O(2) Modelmentioning
confidence: 99%
“…The shift in energy due to gravitational and gauge interactions between the scalar fields in AdS 5 as an expansion in inverse distance corresponds to the CFT computation of anomalous dimensions of the large spin ( 1) double-twist operators. Computing the first order energy shift due to gravitational interactions in the bulk is equivalent to computing the gravitational interaction of a scalar field in AdS-Schwarzschild black hole [63]. We start with the AdS-Schwarzschild 2 black hole in five dimensions,…”
Section: Jhep06(2016)136mentioning
confidence: 99%
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