First Direct Measurement of Jets in $\sqrt{s_{NN}}=200$ GeV Heavy Ion Collisions by STAR
Sevil Salur
TL;DR
The paper develops and applies multiple jet-reconstruction techniques to central Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV, aiming to access unbiased jet kinematics amidst a large heavy-ion background. By combining STAR's TPC and EMC data with cone and sequential-recombination algorithms and event-by-event background corrections, it assesses energy resolution and systematic biases using Pythia-based simulations embedded in real events. The corrected jet spectra are compared to $p+p$ results scaled by $N_{Binary}$, finding consistency within substantial systematic uncertainties for the least-biased selections, suggesting the feasibility of full jet reconstruction in heavy ion environments. The study highlights dependence on $p_{T}$ thresholds and fragmentation modeling, underscoring the need for further calibration and cross-checks, particularly ahead of higher-energy LHC measurements.
Abstract
We present the first measurement of reconstructed jets in ultra-relativistic heavy ion collisions. Utilizing the large coverage of the STAR Time Projection Chamber and Electromagnetic Calorimeter, we apply several modern jet reconstruction algorithms and background subtraction techniques and explore their systematic uncertainties in heavy ion events. The differential spectrum for inclusive jet production in central Au+Au collisions at $\sqrt {s_{NN}}= 200$ GeV is presented. In order to assess the jet reconstruction biases, this spectrum is compared with the jet cross section measured in $\sqrt{s}=200$ GeV p+p collisions scaled by the number of binary N-N collisions to account for nuclear geometric effects.
