English

The Proton-$\Omega$ correlation function in Au+Au collisions at $\sqrt{s_{NN}}$=200 GeV

High Energy Physics - Experiment 2018-08-09 v1 Nuclear Experiment

Abstract

We present the first measurement of the proton-Ω\Omega correlation function in heavy-ion collisions for central (0-40%\%) and peripheral (40-80%\%) Au+Au collisions at \sqrtsNN\,\,=200 GeV by the STAR experiment at the Relativistic Heavy-Ion Collider (RHIC). Predictions for the ratio of peripheral collisions to central collisions for the proton-Ω\Omega correlation function are sensitive to the presence of a nucleon-Ω\Omega bound state. These predictions are based on the proton-Ω\Omega interaction extracted from (2+1)-flavor lattice QCD calculations at the physical point. The measured ratio of proton-Ω\Omega correlation function from peripheral (small system) to central (large system) collisions is less than unity for relative momentum smaller than 40 MeV/c. Comparison of our measured correlation ratio with the theoretical calculation slightly favors a proton-Ω\Omega bound system with a binding energy of \sim 27~MeV.

Keywords

Cite

@article{arxiv.1808.02511,
  title  = {The Proton-$\Omega$ correlation function in Au+Au collisions at $\sqrt{s_{NN}}$=200 GeV},
  author = {The STAR Collaboration},
  journal= {arXiv preprint arXiv:1808.02511},
  year   = {2018}
}

Comments

Submitted to Phys. Lett. B