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

  • (STAR Collaboration)

Producción científica: Contribución a una revistaArtículorevisión exhaustiva

24 Citas (Scopus)

Resumen

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.

Idioma originalInglés
Número de artículo092501
PublicaciónPhysical Review Letters
Volumen129
N.º9
DOI
EstadoPublicada - 26 ago. 2022

Huella

Profundice en los temas de investigación de 'Evidence for Nonlinear Gluon Effects in QCD and Their Mass Number Dependence at STAR'. En conjunto forman una huella única.

Citar esto