We report measurements of Υ meson production in p + p, d + Au, and Au + Au collisions using the STAR detector at RHIC. We compare the Υ yield to the measured cross section in p + p collisions in order to quantify any modiﬁcations of the yield in cold nuclear matter using d + Au data and in hot nuclear matter using Au + Au data separated into three centrality classes. Our p + p measurement is based on three times the statistics of our previous result. We obtain a nuclear modiﬁcation factor for Υ (1S + 2S + 3S) in the rapidity range | y| < 1 in d + Au collisions of RdAu = 0.79 ± 0.24(stat.) ± 0.03(syst.) ± 0.10(p + p syst.). A comparison with models including shadowing and initial state parton energy loss indicates the presence of additional cold-nuclear matter suppression. Similarly, in the top 10% most-central Au + Au collisions, we measure a nuclear modiﬁcation factor of RAA = 0.49 ± 0.1(stat.) ± 0.02(syst.) ± 0.06(p + p syst.), which is a larger suppression factor than that seen in cold nuclear matter. Our results are consistent with complete suppression of excited-state Υ mesons in Au + Au collisions. The additional suppression in Au + Au is consistent with the level expected in model calculations that include the presence of a hot, deconﬁned Quark–Gluon Plasma. However, understanding the suppression seen in d + Au is still needed before any deﬁnitive statements about the nature of the suppression in Au + Au can be made.
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We thank the RHIC Operations Group and RCF at BNL, the NERSC Center at LBNL, the KISTI Center in Korea, and the Open Science Grid consortium for providing resources and support. This work was supported in part by the Offices of NP and HEP within the U.S. DOE Office of Science, the U.S. NSF, CNRS/IN2P3, FAPESP–CNPq of Brazil, the Ministry of Education and Science of the Russian Federation, NNSFC, CAS, MoST and MoE of China, the Korean Research Foundation, GA and MSMT of the Czech Republic, FIAS of Germany, DAE, DST, and CSIR of India, the National Science Centre of Poland, National Research Foundation (NRF-2012004024), the Ministry of Science, Education and Sports of the Republic of Croatia, and RosAtom of Russia.
A corrigendum to this article was published: 'Corrigendum to “Suppression of Υ production in d + Au and Au +Au collisions at √sNN = 200 GeV” [Phys. Lett. B 735 (2014) 127–137]', published in Physics Letters B, v. 743, p. 537-541, available at http://dx.doi.org/10.1016/j.physletb.2015.01.046.
This corrigendum is also available in UKnowledge at: http://uknowledge.uky.edu/physastron_facpub/348/
Adkins, James K.; Fatemi, Renee; Korsch, Wolfgang; Ramachandran, Suvarna; Adamczyk, L.; Aggarwal, M. M.; Ahammed, Z.; Alekseev, I.; Alford, J.; Aparin, A.; Arkhipkin, D.; Aschenauer, E. C.; Averichev, G. S.; and Banerjee, A., "Suppression of Υ production in d + Au and Au + Au collisions at √sNN = 200 GeV" (2014). Physics and Astronomy Faculty Publications. 349.