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    Calculating the Jet Quenching Parameter

    Hong Liu1, Krishna Rajagopal1,2, and Urs Achim Wiedemann3,4

    • 1Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
    • 2Nuclear Science Division, MS 70R319, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
    • 3Department of Physics and Astronomy, University of Stony Brook, New York 11794, USA
    • 4RIKEN-BNL Research Center, Brookhaven National Laboratory, Upton, New York 11973-5000, USA

    Phys. Rev. Lett. 97, 182301 – Published 3 November, 2006

    DOI: https://doi.org/10.1103/PhysRevLett.97.182301

    Abstract

    Models of medium-induced radiative parton energy loss account for the strong suppression of high-pT hadron spectra in sNN=200  GeV Au-Au collisions at BNL RHIC in terms of a single “jet quenching parameter” q^. We observe that q^ can be given a model-independent, nonperturbative, quantum field theoretic definition in terms of the short-distance behavior of a particular lightlike Wilson loop. We then use the anti–de Sitter/conformal-field-theory correspondence to obtain a strong-coupling calculation of q^ in hot N=4 supersymmetric QCD, finding q^SYM=26.69αSYMNcT3 in the limit in which both Nc and 4παSYMNc are large. Thus, at strong coupling q^ is not proportional to the entropy density s, or to some “number density of scatterers” since, unlike the number of degrees of freedom, q^ does not grow like Nc2.

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