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dc.contributor.authorAthanasiou, Christiana
dc.contributor.authorChesler, Paul Michael
dc.contributor.authorLiu, Hong
dc.contributor.authorNickel, Marcel Dominik Johannes
dc.contributor.authorRajagopal, Krishna
dc.date.accessioned2010-08-10T18:57:20Z
dc.date.available2010-08-10T18:57:20Z
dc.date.issued2010-02
dc.date.submitted2010-06
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1721.1/57487
dc.description.abstractUsing gauge/gravity duality, we compute the energy density and angular distribution of the power radiated by a quark undergoing circular motion in strongly coupled N=4 supersymmetric Yang-Mills theory. We compare the strong coupling results to those at weak coupling, finding them to be very similar. In both regimes, the angular distribution of the radiated power is in fact similar to that of synchrotron radiation produced by an electron in circular motion in classical electrodynamics: the quark emits radiation in a narrow beam along its velocity vector with a characteristic opening angle α∼1/γ. To an observer far away from the quark, the emitted radiation appears as a short periodic burst, just like the light from a lighthouse does to a ship at sea. Our strong coupling results are valid for any strongly coupled conformal field theory with a dual classical gravity description.en_US
dc.description.sponsorshipUnited States. Dept. of Energy. Offices of Nuclear and High Energy Physics (Grant Nos. DE-FG02-94ER40818, DE-FG02-05ER41360, and DE-FG02-00ER41132)en_US
dc.language.isoen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.81.126001en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAPSen_US
dc.titleSynchrotron radiation in strongly coupled conformal field theoriesen_US
dc.typeArticleen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.approverRajagopal, Krishna
dc.contributor.mitauthorAthanasiou, Christiana
dc.contributor.mitauthorChesler, Paul Michael
dc.contributor.mitauthorLiu, Hong
dc.contributor.mitauthorRajagopal, Krishna
dc.relation.journalPhysical Review Den_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsAthanasiou, Christiana; Chesler, Paul M.; Liu, Hong; Nickel, Dominik; Rajagopal, Krishnaen
dc.identifier.orcidhttps://orcid.org/0000-0002-4911-3183
dc.identifier.orcidhttps://orcid.org/0000-0001-5812-8718
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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