Jet radiation in a longitudinally expanding medium
Paul Caucal, Edmond Iancu, Gregory Soyez

TL;DR
This paper extends a perturbative QCD-based jet evolution model to an expanding quark-gluon plasma, showing that key factorization properties hold and providing predictions consistent with LHC data, especially at high transverse momenta.
Contribution
It introduces a modified Monte Carlo framework for jet evolution in a longitudinally expanding medium, maintaining the factorization between vacuum-like and medium-induced emissions.
Findings
Scaling relation maps expanding medium to an effective static one.
Small numerical violations of scaling due to vacuum-like emissions.
Predictions for R_{AA} and fragmentation functions align with LHC measurements.
Abstract
In a series of previous papers, we have presented a new approach, based on perturbative QCD, for the evolution of a jet in a dense quark-gluon plasma. In the original formulation, the plasma was assumed to be homogeneous and static. In this work, we extend our description and its Monte Carlo implementation to a plasma obeying Bjorken longitudinal expansion. Our key observation is that the factorisation between vacuum-like and medium-induced emissions, derived in the static case, still holds for an expanding medium, albeit with modified rates for medium-induced emissions and transverse momentum broadening, and with a modified phase-space for vacuum-like emissions. We highlight a scaling relation valid for the energy spectrum of medium-induced emissions, through which the case of an expanding medium is mapped onto an effective static medium. We find that scaling violations due to…
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