https://doi.org/10.1051/epjconf/202429610005
Small-x structure of oxygen and neon isotopes as seen by the Large Hadron Collider
1 Department of Physics, University of Jyvaskyla, 40014, Finland
2 Institut für Theoretische Physik, Universität Heidelberg, Philosophenweg 16, 69120, Germany
3 Physics Department, Brookhaven National Laboratory, Bldg. 510A, Upton, NY 11973, USA
4 Fakultät für Physik, Universität Bielefeld, D-33615 Bielefeld, Germany
* e-mail: prasingh@jyu.fi
Published online: 26 June 2024
Results on collisions of 16O nuclei performed at the Relativistic Heavy Ion Collider (RHIC) have been presented for the first time at Quark Matter 2023 by the STAR collaboration. 16O+16O collisions are also expected to take place in the near future at the Large Hadron Collider (LHC) at much higher beam energies. We explore the potential of beam-energy-dependent studies for this system to probe small-x dynamics and QCD evolution. We perform 3 + 1D IP-Glasma simulations to predict the rapidity dependence of the initial geometry of light-ion collisions, focusing on 16O+16O and 20Ne+20Ne collisions at √SNN = 70 GeV and 7 TeV. The choice of 20Ne is motivated by its strongly elongated geometry, which may respond differently to the effect of the highenergy evolution compared to the more spherical 16O. We find that smearing induced by soft gluon production at high energy causes mild variations in the initial-state eccentricities as a function of the collision energy. These effects could be resolved in future experiments and deserve further investigation.
© The Authors, published by EDP Sciences, 2024
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
