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dc.contributor.authorCMS Collaboration
dc.date.accessioned2018-10-25T17:17:38Z
dc.date.available2018-10-25T17:17:38Z
dc.date.issued2017-07
dc.identifier.citationCMS Collaboration. "Suppression of ϒ(1S), ϒ(2S), and ϒ(3S) quarkonium states in PbPb collisions at √ sNN = 2.76 TeV”, Physics Letters B. (2017) 770: 357-379. https://doi.org/10.1016/j.physletb.2017.04.031en_US
dc.identifier.urihttp://hdl.handle.net/1808/27037
dc.description.abstractThe production yields of ϒ(1S), ϒ(2S), and ϒ(3S) quarkonium states are measured through their decays into muon pairs in the CMS detector, in PbPb and pp collisions at the centre-of-mass energy per nucleon pair of 2.76 TeV. The data correspond to integrated luminosities of 166 μb−1 and 5.4 pb−1 for PbPb and pp collisions, respectively. Differential production cross sections are reported as functions of ϒ rapidity y up to 2.4, and transverse momentum pT up to 20 GeV/c. A strong centrality-dependent suppression is observed in PbPb relative to pp collisions, by factors of up to ≈2 and 8, for the ϒ(1S) and ϒ(2S) states, respectively. No significant dependence of this suppression is observed as a function of y or pT. The ϒ(3S) state is not observed in PbPb collisions, which corresponds to a suppression for the centrality-integrated data by at least a factor of ≈7 at a 95% confidence level. The observed suppression is in agreement with theoretical scenarios modeling the sequential melting of quarkonium states in a quark gluon plasma.en_US
dc.publisherElsevieren_US
dc.rights© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.subjectCMSen_US
dc.subjectPhysicsen_US
dc.subjectHeavy ionsen_US
dc.subjectDimuonsen_US
dc.subjectBottomoniaen_US
dc.titleSuppression of ϒ(1S), ϒ(2S), and ϒ(3S) quarkonium states in PbPb collisions at √ sNN = 2.76 TeVen_US
dc.typeArticleen_US
kusw.kuauthorBaringer, Philip, S.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1016/j.physletb.2017.04.031en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.rights.accessrightsopenAccessen_US


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© 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license
(http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3
Except where otherwise noted, this item's license is described as: © 2017 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3