2012
DOI: 10.1103/physrevd.85.126006
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Shining a gluon beam through quark-gluon plasma

Abstract: We compute the energy density radiated by a quark undergoing circular motion in strongly coupled N = 4 supersymmetric Yang-Mills plasma. If it were in vacuum, this quark would radiate a beam of strongly coupled radiation whose angular distribution has been characterized and is very similar to that of synchrotron radiation produced by an electron in circular motion in electrodynamics. Here, we watch this beam of gluons getting quenched by the strongly coupled plasma. We find that a beam of gluons of momenta ∼ q… Show more

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Cited by 27 publications
(46 citation statements)
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“…The conclusion that we reach is consistent with conclusions (also qualitative) reached by analyzing the quenching of a beam of gluons by strongly coupled N ¼ 4 SYM plasma [12]. In a different sense, weak-coupling analyses of the quenching of a high energy parton by a slab of weakly coupled plasma at some constant T (see Ref.…”
Section: Introduction and Conclusionsupporting
confidence: 90%
“…The conclusion that we reach is consistent with conclusions (also qualitative) reached by analyzing the quenching of a beam of gluons by strongly coupled N ¼ 4 SYM plasma [12]. In a different sense, weak-coupling analyses of the quenching of a high energy parton by a slab of weakly coupled plasma at some constant T (see Ref.…”
Section: Introduction and Conclusionsupporting
confidence: 90%
“…Similar quenching was also observed in isolated photon+jet pairs [15]. While these results constrain the mechanism of parton energy loss [17,18], further understanding requires the measurement of the p T dependence of the observed effects. The goal of this analysis is to characterize possible modifications of dijet event properties as a function of centrality and leading jet transverse momentum in PbPb collisions.…”
Section: Introductionsupporting
confidence: 72%
“…There is a minimum possible initial opening angle, corresponding to the maximum possible x stop for jets with a given initial energy [145] that was computed holographically in refs. [131,137,141] and is given by…”
Section: Jhep03(2017)135mentioning
confidence: 99%