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Υ Production in Heavy-Ion Collisions from the STAR Experiment

2017/02/18 by Zaochen Ye, Ye, Zaochen
Physics and Astronomy · #FOS: Physical sciences #High Energy Physics - Experiment (hep-ex) #High-Energy Particle Collisions Research #Nuclear Experiment (nucl-ex) #Particle physics theoretical and experimental studies #Quantum Chromodynamics and Particle Interactions #hep-ex #nucl-ex

paper · pdf · doi:10.48550/arxiv.1702.05651

Hard Probes 2016 proceedings

arxiv created 2017/02/18 · openalex publication_date 2017/02/18 · arxiv updated 2017/02/21 · openalex created_date 2019/06/27 · openalex updated_date 2026/07/28

Abstract

In these proceedings, we present recent results of Υ measurements in heavy-ion collisions from the STAR experiment at RHIC. Nuclear modification factors (RAA) for Υ(1S) and Υ(1S+2S+3S) in U+U collisions at \sqrtsNN = 193 GeV are measured through the di-electron channel and compared to those in Au+Au collisions at \sqrtsNN = 200 GeV and Pb+Pb collisions at \sqrtsNN = 2.76 TeV. The ratio between the Υ(2S+3S) and Υ(1S) yields in Au+Au collisions at \sqrtsNN = 200 GeV is measured in the di-muon channel and compared to those in p+p collisions and in Pb+Pb collisions at \sqrtsNN = 2.76 TeV. Prospects for future Υ measurements with the STAR experiment are also discussed.

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