Rapidity dependence of azimuthal correlations for p+p and d+Au at $\sqrt{s}=200$GeV
Xuan Li (for the STAR Collaboration)

TL;DR
This paper investigates how azimuthal correlations of particles produced in proton-proton and deuteron-gold collisions at 200 GeV vary with rapidity, providing insights into the nuclear gluon density at small Bjorken-x values.
Contribution
It presents new measurements of forward and mid-rapidity azimuthal correlations using STAR's electromagnetic calorimeters, probing the nuclear gluon density at intermediate x.
Findings
Preliminary results on $c0^{0}$-$c0^{0}$ correlations.
Analysis of $c0^{0}$ + jet-like azimuthal correlations.
Sensitivity to nuclear gluon density at small Bjorken-x.
Abstract
Forward di-jet production in d+Au collisions at RHIC provides sensitivity to Bjorken-x between 0.001 and 0.02 for the nuclear gluon density . The STAR experiment at RHIC has continuous azimuthal coverage with electromagnetic calorimeters for pseudo-rapidity from -1 to 4. We have measured forward+mid-rapidity and azimuthal correlations and forward+forward rapidity azimuthal correlations. Both analyses use the Forward Meson Spectrometer (FMS) triggered data in RHIC 2008 run p+p and d+Au collisions at =200 GeV. The end-cap electromagnetic calorimeter (EEMC) at STAR covers pseudo-rapidity from 1.07 to 2. This provides us sensitivity to the nuclear gluon density at intermediate x values. Preliminary results on the and + jet-like azimuthal correlations with both the FMS and the EEMC will be discussed.
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.
