Centrality and pseudorapidity dependence of the transverse energy flow in pPb collisions at sqrt(s_NN) = 5.02 TeV
Christopher Bruner, Michael Murray (for the CMS Collaboration)

TL;DR
This paper measures the distribution of transverse energy as a function of pseudorapidity in pPb collisions at 5.02 TeV, revealing centrality dependence and differences from event generator predictions.
Contribution
It provides the first detailed measurement of transverse energy distribution in pPb collisions across pseudorapidity and compares centrality dependence with model predictions.
Findings
Transverse energy per participant pair is comparable to peripheral PbPb collisions.
Centrality dependence is stronger on the lead side than the proton side.
Significant discrepancies between data and event generator predictions.
Abstract
The almost hermetic coverage of CMS is used to measure the distribution of transverse energy as a function of pseudo-rapidity for pPb collisions at TeV. For minimum bias collisions reaches 23 GeV which implies an per participant pair comparable to that of peripheral PbPb collisions at TeV. The centrality dependence of transverse energy production has been studied using centrality measures defined in three different angular regions. There is a strong auto-correlation between and the range used to define centrality %both for data and the EPOS-LHC and HIJING event generators. The centrality dependence of the data is much stronger for values on the lead side than the proton side and shows significant differences from that predicted by either event generator.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsHigh-Energy Particle Collisions Research · Particle physics theoretical and experimental studies · Quantum Chromodynamics and Particle Interactions
