Observation of strong nuclear suppression in exclusive 𝐽/𝜓 photoproduction in Au+Au ultraperipheral collisions at RHIC

We report a measurement of exclusive 𝐽/𝜓 and 𝜓⁡(2⁢𝑠) photoproduction in Au+Au ultraperipheral collisions at √𝑠NN=200 GeV using the STAR detector. For the first time, (i) the 𝜓⁡(2⁢𝑠) photoproduction in midrapidity at the Relativistic Heavy-Ion Collider has been experimentally measured; (ii) nuclear s...

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Hauptverfasser: Abdulhamid, Muhammad Ibrahim (VerfasserIn) , Deppner, Ingo Martin (VerfasserIn) , Herrmann, Norbert (VerfasserIn) , Leung, Yue (VerfasserIn) , Söhngen, Yannick (VerfasserIn)
Körperschaft: STAR Collaboration (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 31 July, 2024
In: Physical review letters
Year: 2024, Jahrgang: 133, Heft: 5, Pages: 1-9
ISSN:1079-7114
DOI:10.1103/PhysRevLett.133.052301
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevLett.133.052301
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevLett.133.052301
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Verfasserangaben:M.I. Abdulhamid, I.M. Deppner, N. Herrmann, Y.H. Leung, Y. Söhngen (STAR Collaboration)
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Zusammenfassung:We report a measurement of exclusive 𝐽/𝜓 and 𝜓⁡(2⁢𝑠) photoproduction in Au+Au ultraperipheral collisions at √𝑠NN=200 GeV using the STAR detector. For the first time, (i) the 𝜓⁡(2⁢𝑠) photoproduction in midrapidity at the Relativistic Heavy-Ion Collider has been experimentally measured; (ii) nuclear suppression factors are measured for both the coherent and incoherent 𝐽/𝜓 production. At average photon-nucleon center-of-mass energy of 25.0 GeV, the coherent and incoherent 𝐽/𝜓 cross sections of Au nuclei are found to be 71 ±10% and 36 ±7%, respectively, of that of free protons. The stronger suppression observed in the incoherent production provides a new experimental handle to study the initial-state parton density in heavy nuclei. Data are compared with theoretical models quantitatively.
Beschreibung:Gesehen am 11.07.2025
Beschreibung:Online Resource
ISSN:1079-7114
DOI:10.1103/PhysRevLett.133.052301