The proton-$\Omega$ correlation function in Au + Au collisions at $\sqrt{s_{NN}}$ =200GeV
| dc.contributor.author | STAR Collaboration | |
| dc.date.accessioned | 2025-02-20T15:55:42Z | |
| dc.date.available | 2025-02-20T15:55:42Z | |
| dc.date.issued | 2019-03-10 | |
| dc.description.abstract | We present the first measurement of the proton-$\Omega$ correlation function in heavy-ion collisions for central (0-40%) and peripheral (40-80%) Au+Au collisions at $\sqrt{s_{NN}}$ =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-$\Omega$ correlation function are sensitive to the presence of a nucleon-$\Omega$ bound state. These predictions are based on the proton-$\Omega$ interaction extracted from (2+1)-flavor lattice QCD calculations at the physical point. The measured ratio of proton-$\Omega$ 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-$\Omega$ bound system with a binding energy of ∼ 27 MeV. | |
| dc.identifier.citation | STAR Collaboration. "The proton-$\Omega$ correlation function in Au + Au collisions at $\sqrt{s_{NN}}$ =200GeV." Physics Letters B, vol. 790, 2019-03-10, https://doi.org/10.1016/j.physletb.2019.01.055. | |
| dc.identifier.issn | 0370-2693 | |
| dc.identifier.other | BRITE 7228 | |
| dc.identifier.uri | https://hdl.handle.net/2022/32164 | |
| dc.language.iso | en | |
| dc.relation.isversionof | https://doi.org/10.1016/j.physletb.2019.01.055 | |
| dc.relation.isversionof | https://doi.org/10.1016/j.physletb.2019.01.055 | |
| dc.relation.journal | Physics Letters B | |
| dc.rights | This work may be protected by copyright unless otherwise stated. | |
| dc.title | The proton-$\Omega$ correlation function in Au + Au collisions at $\sqrt{s_{NN}}$ =200GeV |
Files
Collections
Can’t use the file because of accessibility barriers? Contact us