Jet physics in heavy-ion collisions
Y. Mehtar-Tani, J. G. Milhano, K. Tywoniuk
TL;DR
This paper reviews the theoretical framework for jet modification in ultrarelativistic heavy-ion collisions, focusing on how a deconfined QCD medium induces radiation and decoheres color within perturbative QCD. It develops the LPM-based picture of radiative energy loss and an in-medium branching formalism, highlighting the roles of the transport coefficient $\\hat q$, the branching time $t_{br}$, and the decoherence parameter $\\Delta_{med}$, and discusses two main shower-modeling approaches: rate equations and vacuum-like evolution with medium-modified splitting kernels. It then connects these mechanisms to jet quenching observables—$R_{AA}$, di-jet asymmetry, and jet substructure—showing qualitative agreement with LHC data while outlining theoretical uncertainties and challenges. The goal is to provide a coherent, perturbative framework for extracting medium properties from jet measurements and guiding future theory and experiments in jet tomography of the QGP.
Abstract
Jets are expected to play a prominent role in the ongoing efforts to characterize the hot and dense QCD medium created in ultrarelativistic heavy ion collisions. The success of this program depends crucially on the existence of a full theoretical account of the dynamical effects of the medium on the jets that develop within it. By focussing on the discussion of the essential ingredients underlying such a theoretical formulation, we aim to set the appropriate context in which current and future developments can be understood.
