TY - JOUR
T1 - Evidence for Nonlinear Gluon Effects in QCD and Their Mass Number Dependence at STAR
AU - Abdallah, M. S.
AU - Aboona, B. E.
AU - Adam, J.
AU - Adamczyk, L.
AU - Kabana, S.
AU - (STAR Collaboration)
N1 - Publisher Copyright:
© 2022 American Physical Society.
PY - 2022/8/26
Y1 - 2022/8/26
N2 - 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 Qs2 on the mass number A. A linear scaling of the suppression with A1/3 is observed with a slope of -0.09±0.01.
AB - 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 Qs2 on the mass number A. A linear scaling of the suppression with A1/3 is observed with a slope of -0.09±0.01.
UR - https://www.scopus.com/pages/publications/85137263697
U2 - 10.1103/PhysRevLett.129.092501
DO - 10.1103/PhysRevLett.129.092501
M3 - Article
C2 - 36083674
AN - SCOPUS:85137263697
SN - 0031-9007
VL - 129
JO - Physical Review Letters
JF - Physical Review Letters
IS - 9
M1 - 092501
ER -