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dc.contributor.authorALICE Collaboration
dc.date.accessioned2018-04-10T08:50:35Z
dc.date.available2018-04-10T08:50:35Z
dc.date.issued2018
dc.identifier.citationALICE Collaboration. (2018). Longitudinal asymmetry and its effect on pseudorapidity distributions in Pb–Pb collisions at √sNN = 2.76 TeV. <i>Physics Letters B</i>, <i>781</i>, 20-32. <a href="https://doi.org/10.1016/j.physletb.2018.03.051" target="_blank">https://doi.org/10.1016/j.physletb.2018.03.051</a>
dc.identifier.otherCONVID_27974883
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/57529
dc.description.abstractFirst results on the longitudinal asymmetry and its effect on the pseudorapidity distributions in Pb–Pb collisions at = 2.76 TeV at the Large Hadron Collider are obtained with the ALICE detector. The longitudinal asymmetry arises because of an unequal number of participating nucleons from the two colliding nuclei, and is estimated for each event by measuring the energy in the forward neutron-Zero-Degree-Calorimeters (ZNs). The effect of the longitudinal asymmetry is measured on the pseudorapidity distributions of charged particles in the regions , and by taking the ratio of the pseudorapidity distributions from events corresponding to different regions of asymmetry. The coefficients of a polynomial fit to the ratio characterise the effect of the asymmetry. A Monte Carlo simulation using a Glauber model for the colliding nuclei is tuned to reproduce the spectrum in the ZNs and provides a relation between the measurable longitudinal asymmetry and the shift in the rapidity () of the participant zone formed by the unequal number of participating nucleons. The dependence of the coefficient of the linear term in the polynomial expansion, , on the mean value of is investigated.
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofseriesPhysics Letters B
dc.subject.otherhiukkasfysiikka
dc.subject.otherparticle physics
dc.titleLongitudinal asymmetry and its effect on pseudorapidity distributions in Pb–Pb collisions at √sNN = 2.76 TeV
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201804051928
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.date.updated2018-04-05T12:15:06Z
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.format.pagerange20-32
dc.relation.issn0370-2693
dc.relation.numberinseries0
dc.relation.volume781
dc.type.versionpublishedVersion
dc.rights.copyright© 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by SCOAP3.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.subject.ysohiukkasfysiikka
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1016/j.physletb.2018.03.051
dc.type.okmA1


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© 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by
SCOAP3.
Ellei muuten mainita, aineiston lisenssi on © 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license. Funded by SCOAP3.