Dissecting the role of initial collision geometry for jet quenching observables in relativistic heavy ion collisions
arXiv:1005.0645 · doi:10.1103/PhysRevC.82.024902
Abstract
The observation of large azimuthal anisotropy or for hadrons above GeV/ in Au+Au collisions at GeV has been a longstanding challenge for jet quenching models based on perturbative QCD (pQCD). Using a simple jet absorption model, we seek to clarify the situation by exploring in detail how the calculated varies with choices of the collision geometry as well as choices of the path length dependence and thermalization time in the energy loss formula. Besides the change of eccentricity due to distortion from gluon saturation or event-by-event fluctuation, we find that the is also sensitive to the centrality dependence of multiplicity and the relative size between the matter profile and the jet profile. We find that the calculated for the naive quadratic path length dependence of energy loss, even including eccentricity fluctuation and the gluon saturation, is not enough to describe the experimental data at high ( 6 GeV/) in Au+Au collisions. However, it can match the full centrality dependence of data if higher power path length dependence of energy loss is allowed. We also find that the calculated is sensitive to the assumption of the early time dynamics but generally increases with , opposite to what one expects for elliptic flow. This study attests to the importance of confining the initial geometry, possibly by combining jet quenching with elliptic flow and other jet quenching observables, for proper interpretation of the experimental data.
20 pages, 28 figures
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