Evidence for Nonlinear Gluon Effects in QCD and Their Mass Number Dependence at STAR

Resource type
Authors/contributors
Title
Evidence for Nonlinear Gluon Effects in QCD and Their Mass Number Dependence at STAR
Abstract
The STAR Collaboration reports measurements of back-to-back azimuthal correlations of di-π0s produced at forward pseudorapidities (2.6<η<4.0) in p+p, p+Al, and p+Au collisions at a center-of-mass energy of 200 GeV. We observe a clear suppression of the correlated yields of back-to-back π0 pairs in p+Al and p+Au collisions compared to the p+p data. The observed suppression of back-to-back pairs as a function of transverse momentum suggests nonlinear gluon dynamics arising at high parton densities. The larger suppression found in p+Au relative to p+Al collisions exhibits a dependence of the saturation scale Q2s on the mass number A. A linear scaling of the suppression with A1/3 is observed with a slope of −0.09±0.01.
Publication
Physical Review Letters
Publisher
American Physical Society
Date
2022-08-22
Volume
129
Issue
9
Pages
092501
Journal Abbr
Phys. Rev. Lett.
Citation Key
starcollaborationEvidenceNonlinearGluon2022
Accessed
9/16/22, 4:36 PM
Library Catalog
APS
Extra
3 citations (Crossref) [2023-10-31]
Citation
STAR Collaboration. (2022). Evidence for Nonlinear Gluon Effects in QCD and Their Mass Number Dependence at STAR. Physical Review Letters, 129(9), 092501. https://doi.org/10.1103/PhysRevLett.129.092501