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Jet quenching

David d'Enterria

TL;DR

This review discusses jet quenching as a powerful probe of hot, dense QCD matter created in high-energy nucleus-nucleus collisions. It surveys perturbative and nonperturbative approaches to parton energy loss (BDMPS-ASW, DGLV, HT, AMY, and AdS/CFT), and confronts them with experimental data from RHIC and expectations for the LHC, highlighting the extraction of transport coefficients such as $\hat{q}$ and the initial gluon density $dN^g/dy$. The article details how high-$p_T$ hadron suppression, di-hadron correlations, and full jet observables constrain the medium’s temperature, density, and dynamical evolution, including the path-length and color-factor dependences, and heavy-quark dynamics. It also emphasizes the role of jet reconstruction and photon-jet correlations in providing a more differential view of in-medium parton showers and fragmentation, thereby offering a pathway to quantitatively map the QGP properties and its response to energetic probes.

Abstract

We present a comprehensive review of the physics of hadron and jet production at large transverse momentum in high-energy nucleus-nucleus collisions. Emphasis is put on experimental and theoretical "jet quenching" observables that provide direct information on the (thermo)dynamical properties of hot and dense QCD matter.

Jet quenching

TL;DR

This review discusses jet quenching as a powerful probe of hot, dense QCD matter created in high-energy nucleus-nucleus collisions. It surveys perturbative and nonperturbative approaches to parton energy loss (BDMPS-ASW, DGLV, HT, AMY, and AdS/CFT), and confronts them with experimental data from RHIC and expectations for the LHC, highlighting the extraction of transport coefficients such as and the initial gluon density . The article details how high- hadron suppression, di-hadron correlations, and full jet observables constrain the medium’s temperature, density, and dynamical evolution, including the path-length and color-factor dependences, and heavy-quark dynamics. It also emphasizes the role of jet reconstruction and photon-jet correlations in providing a more differential view of in-medium parton showers and fragmentation, thereby offering a pathway to quantitatively map the QGP properties and its response to energetic probes.

Abstract

We present a comprehensive review of the physics of hadron and jet production at large transverse momentum in high-energy nucleus-nucleus collisions. Emphasis is put on experimental and theoretical "jet quenching" observables that provide direct information on the (thermo)dynamical properties of hot and dense QCD matter.

Paper Structure

This paper contains 47 sections, 35 equations, 36 figures, 3 tables.

Figures (36)

  • Figure 1: Examples of hard probes whose modifications in high-energy $AA$ collisions provide direct information on properties of QCD matter such as the transport coefficient ${\hat{q}}$, the initial gluon rapidity density $dN^g/dy$, and the critical temperature $T_{\hbox{\tiny{\it crit}}}$ and energy density $\varepsilon_{\hbox{\tiny{\it crit}}}$d'Enterria:2006su.
  • Figure 2: "Jet quenching" in a head-on nucleus-nucleus collision. Two quarks suffer a hard scattering: one goes out directly to the vacuum, radiates a few gluons and hadronises, the other goes through the dense plasma created (characterised by transport coefficient ${\hat{q}}$, gluon density $dN^g/dy$ and temperature $T$), suffers energy loss due to medium-induced gluonstrahlung and finally fragments outside into a (quenched) jet.
  • Figure 3: Diagrams for collisional (left) and radiative (right) energy losses of a quark of energy $E$ traversing a quark-gluon medium.
  • Figure 4: Stopping power, $-dE/dl$, for positive muons in copper as a function of $\beta\gamma = p/Mc$ (or momentum $p$). The solid curve indicates the total stopping power Yao:2006px.
  • Figure 5: Comparison of the average radiative and elastic energy losses of light-quarks (left) and light- and heavy-quarks (right) passing through the medium produced in central $AuAu$ collisions at RHIC energies as obtained by the AMY Qin:2007rn and DGLV Wicks:2005gt models (see later).
  • ...and 31 more figures