# Deciphering the $z_g$ distribution in ultrarelativistic heavy ion   collisions

**Authors:** Paul Caucal, Edmond Iancu, Gregory Soyez

arXiv: 1907.04866 · 2020-01-08

## TL;DR

This paper introduces a new perturbative QCD-based model for jet evolution in quark-gluon plasma, successfully explaining jet quenching observables and predicting a change in jet substructure ratios at high transverse momentum.

## Contribution

It develops a combined model of medium-induced and vacuum-like parton emissions, implemented as a Monte Carlo generator, to better understand jet quenching phenomena.

## Key findings

- Good agreement with LHC data on $R_{AA}$ and $z_g$ distributions
- Energy loss increases with jet transverse momentum due to more vacuum-like emissions
- Predicted change in $z_g$ ratio behavior at high transverse momentum

## Abstract

Within perturbative QCD, we develop a new picture for the parton shower generated by a jet propagating through a dense quark-gluon plasma. This picture combines in a simple, factorised, way multiple medium-induced parton branchings and standard vacuum-like emissions, with the phase-space for the latter constrained by the presence of the medium. We implement this picture as a Monte Carlo generator that we use to study two phenomenologically important observables: the jet nuclear modification factor $R_{AA}$ and the $z_g$ distribution reflecting the jet substructure. In both cases, the outcome of our Monte Carlo simulations is in good agreement with the LHC measurements. We provide basic analytic calculations that help explaining the main features observed in the data. We find that the energy loss by the jet is increasing with the jet transverse momentum, due to a rise in the number of partonic sources via vacuum-like emissions. This is a key element in our description of both $R_{AA}$ and the $z_g$ distribution. For the latter, we identify two main nuclear effects: incoherent jet energy loss and hard medium-induced emissions. As the jet transverse momentum increases, we predict a qualitative change in the ratio between the $z_g$ distributions in PbPb and pp collisions: from increasing at small $z_g$, this ratio becomes essentially flat, or even slightly decreasing.

## Full text

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## Figures

61 figures with captions in the complete paper: https://tomesphere.com/paper/1907.04866/full.md

## References

71 references — full list in the complete paper: https://tomesphere.com/paper/1907.04866/full.md

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Source: https://tomesphere.com/paper/1907.04866