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dc.contributor.authorKristjansen, C
dc.contributor.authorSemenoff, GW
dc.contributor.authorYoung, D
dc.date.accessioned2016-03-14T12:37:35Z
dc.date.issued2013-01-17
dc.date.issued2013
dc.date.issued2013
dc.identifier.other10.1007/JHEP01(2013)117
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/11456
dc.descriptionJHEP is an open-access journal funded by SCOAP3 and licensed under CC BY 4.0en_US
dc.descriptionarchiveprefix: arXiv primaryclass: hep-th reportnumber: NORDITA-2012-81 slaccitation: %%CITATION = ARXIV:1210.7015;%%
dc.descriptionarchiveprefix: arXiv primaryclass: hep-th reportnumber: NORDITA-2012-81 slaccitation: %%CITATION = ARXIV:1210.7015;%%
dc.description.abstractWe compute the one-point functions of chiral primary operators in the nonsupersymmetric defect conformal field theory that is dual to the IIB string theory on AdS5 × S 5 background with a probe D7 brane with internal gauge field flux, both in perturbative Yang-Mills theory and in the string theory dual. The former is expected to be accurate at weak coupling whereas the latter should be accurate in the planar strong coupling limit of the gauge theory. We consider the distinct cases where the D7 brane has geometry AdS4 × S 4 with an instanton bundle of the worldvolume gauge fields on S 4 and AdS4 × S 2 × S 2 with Dirac monopole bundles on each S 2 . The gauge theory computation and the string theory computation can be compared directly in the planar limit and then a subsequent limit where the worldvolume flux is large. We find that there is exact agreement between the two in the leading order.
dc.description.sponsorshipC.F.K. and D.Y. were supported in part by FNU through grant number 272-08-0329. G.W.S. is supported by NSERC of Canada and by the Villum foundation through their Velux Visiting Professor program.en_US
dc.format.extent117 - 117
dc.language.isoenen_US
dc.relation.ispartofJHEP
dc.titleChiral primary one-point functions in the D3-D7 defect conformal field theory
dc.typeJournal Article
dc.rights.holder© SISSA, Trieste, Italy 2013
dc.identifier.doi10.1007/JHEP01(2013)117
dc.relation.isPartOfJHEP
dc.relation.isPartOfJHEP
pubs.organisational-group/Queen Mary University of London
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering
pubs.organisational-group/Queen Mary University of London/Faculty of Science & Engineering/Physics and Astronomy
pubs.volume1301


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