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dc.contributor.authorCMS Collaboration
dc.date.accessioned2018-10-09T17:29:35Z
dc.date.available2018-10-09T17:29:35Z
dc.date.issued2018-09
dc.identifier.citationThe CMS collaboration, Coherent J/ψ photoproduction in ultra-peripheral PbPb collisions at √sNN= 2.76 TeV with the CMS experiment, Physics Letters B. (2017) 772: 489-511. https://doi.org/10.1016/j.physletb.2017.07.001en_US
dc.identifier.urihttp://hdl.handle.net/1808/26799
dc.description.abstractThe cross section for coherent J/ψ photoproduction accompanied by at least one neutron on one side of the interaction point and no neutron activity on the other side, Xn0n, is measured with the CMS experiment in ultra-peripheral PbPb collisions at √sNN= 2.76TeV. The analysis is based on a data sample corresponding to an integrated luminosity of 159 μb−1, collected during the 2011 PbPb run. The J/ψ mesons are reconstructed in the dimuon decay channel, while neutrons are detected using zero degree calorimeters. The measured cross section is dσcohXn0n/dy(J/ψ ) = 0.36 ± 0.04 (stat) ±0.04 (syst) mb in the rapidity interval 1.8 < |y| < 2.3. Using a model for the relative rate of coherent photoproduction processes, this Xn0nmeasurement gives a total coherent photoproduction cross section of dσcoh/dy(J/ψ ) = 1.82±0.22 (stat)±0.20 (syst)±0.19 (theo) mb. The data strongly disfavor the impulse approximation model prediction, indicating that nuclear effects are needed to describe coherent J/ψphotoproduction in γ + Pb interactions. The data are found to be consistent with the leading twist approximation, which includes nuclear gluon shadowing.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 licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.subjectCMSen_US
dc.subjectPhysicsen_US
dc.subjectHeavy ion collisionsen_US
dc.subjectUltra-peripheral collisionsen_US
dc.subjectUPCen_US
dc.subjectJ/Psien_US
dc.titleCoherent J/ψ photoproduction in ultra-peripheral PbPb collisions at √sNN= 2.76 TeV with the CMS experimenten_US
dc.typeArticleen_US
kusw.kuauthorBaringer, Philip S.
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doihttps://doi.org/10.1016/j.physletb.2017.07.001en_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
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