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dc.contributor.authorBrewer, Jasmine Therese
dc.contributor.authorRajagopal, Krishna
dc.contributor.authorSadofyev, Andrey
dc.contributor.authorvan der Schee, Wilke
dc.date.accessioned2018-07-02T14:42:58Z
dc.date.available2018-07-02T14:42:58Z
dc.date.issued2018-02
dc.date.submitted2017-11
dc.identifier.issn1029-8479
dc.identifier.urihttp://hdl.handle.net/1721.1/116711
dc.description.abstractSome of the most important experimentally accessible probes of the quark- gluon plasma (QGP) produced in heavy ion collisions come from the analysis of how the shape and energy of sprays of energetic particles produced within a cone with a specified opening angle (jets) in a hard scattering are modified by their passage through the strongly coupled, liquid, QGP. We model an ensemble of back-to-back dijets for the purpose of gaining a qualitative understanding of how the shapes of the individual jets and the asymmetry in the energy of the pairs of jets in the ensemble are modified by their passage through an expanding cooling droplet of strongly coupled plasma, in the model in a holographic gauge theory that is dual to a 4+1-dimensional black-hole spacetime that is asymptotically anti-de Sitter (AdS). We build our model by constructing an ensemble of strings in the dual gravitational description of the gauge theory. We model QCD jets in vacuum using strings whose endpoints are moving “downward” into the gravitational bulk spacetime with some fixed small angle, an angle that represents the opening angle (ratio of jet mass to jet energy) that the QCD jet would have in vacuum. Such strings must be moving through the gravitational bulk at (close to) the speed of light; they must be (close to) null. This condition does not specify the energy distribution along the string, meaning that it does not specify the shape of the jet being modeled. We study the dynamics of strings that are initially not null and show that strings with a wide range of initial conditions rapidly accelerate and become null and, as they do, develop a similar distribution of their energy density. We use this distribution of the energy density along the string, choose an ensemble of strings whose opening angles and energies are distributed as in perturbative QCD, and show that we can then fix one of the two model parameters such that the mean jet shape for the jets in the ensemble that we have built matches that measured in proton-proton collisions reasonably well. This is a novel way for hybridizing relevant inputs from perturbative QCD and a strongly coupled holographic gauge theory in the service of modeling jets in QGP. We send our ensemble of strings through an expanding cooling droplet of strongly coupled plasma, choosing the second model parameter so as to get a reasonable value for R AA jet , the suppression in the number of jets, and study how the mean jet shape and the dijet asymmetry are modified, comparing both to measurements from heavy ion collisions at the LHC.en_US
dc.publisherSpringer/SISSAen_US
dc.relation.isversionofhttp://dx.doi.org/10.1007/JHEP02(2018)015en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.sourceTopicHub SCOAP3en_US
dc.titleEvolution of the mean jet shape and dijet asymmetry distribution of an ensemble of holographic jets in strongly coupled plasmaen_US
dc.typeArticleen_US
dc.identifier.citationBrewer, Jasmine, Krishna Rajagopal, Andrey Sadofyev, and Wilke van der Schee. “Evolution of the Mean Jet Shape and Dijet Asymmetry Distribution of an Ensemble of Holographic Jets in Strongly Coupled Plasma.” Journal of High Energy Physics 2018, no. 2 (February 2018).en_US
dc.contributor.departmentMassachusetts Institute of Technology. Center for Theoretical Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.mitauthorBrewer, Jasmine Therese
dc.contributor.mitauthorRajagopal, Krishna
dc.contributor.mitauthorSadofyev, Andrey
dc.contributor.mitauthorvan der Schee, Wilke
dc.relation.journalJournal of High Energy Physicsen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-03-12T14:26:46Z
dc.rights.holderThe Author(s)
dspace.orderedauthorsBrewer, Jasmine; Rajagopal, Krishna; Sadofyev, Andrey; van der Schee, Wilkeen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-3084-0663
dc.identifier.orcidhttps://orcid.org/0000-0001-5812-8718
dc.identifier.orcidhttps://orcid.org/0000-0001-9679-2409
dc.identifier.orcidhttps://orcid.org/0000-0003-2477-6623
mit.licensePUBLISHER_CCen_US


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