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  4. J/ψ Production at Low p[subscript T] in Au + Au and Cu + Cu Collisions at √s[subscript NN] = 200 GeV with the STAR Detector

J/ψ Production at Low p[subscript T] in Au + Au and Cu + Cu Collisions at √s[subscript NN] = 200 GeV with the STAR Detector

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Author(s)
Stevens, Justin
•
van Nieuwenhuizen, Gerrit J
Date Issued
August 2014
Journal
Physical Review C
Publisher
American Physical Society
Citation
Adamczyk, L., J. K. Adkins, G. Agakishiev, M. M. Aggarwal, Z. Ahammed, I. Alekseev, J. Alford, et al. “J/ψ Production at Low p[subscript T] in Au + Au and Cu + Cu Collisions at √s[subscript NN] = 200 GeV with the STAR Detector.” Phys. Rev. C 90, no. 2 (August 2014). © 2014 American Physical Society
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Final published version
Abstract
The J/ψ p[subscript T] spectrum and nuclear modification factor (R[subscript AA]) are reported for p[subscript T] < 5GeV/c and |y| < 1 from 0% to 60% central Au + Au and Cu + Cu collisions at √s[subscript NN] = 200 GeV at STAR. A significant suppression of p[subscript T]-integrated J/ψ production is observed in central Au + Au events. The Cu + Cu data are consistent with no suppression, although the precision is limited by the available statistics. R[subscript AA] in Au + Au collisions exhibits a strong suppression at low transverse momentum and gradually increases with p[subscript T]. The data are compared to high-p[subscript T] STAR results and previously published BNL Relativistic Heavy Ion Collider results. Comparing with model calculations, it is found that the invariant yields at low p[subscript T] are significantly above hydrodynamic flow predictions but are consistent with models that include color screening and regeneration.
MIT Department
Massachusetts Institute of Technology. Laboratory for Nuclear Science
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/91210
DOI of Published Version
https://doi.org/10.1103/PhysRevC.90.024906
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