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dc.contributor.authorHelenius, Ilkka
dc.contributor.authorLajoie, John
dc.contributor.authorOsborn, Joseph D.
dc.contributor.authorPaakkinen, Petja
dc.contributor.authorPaukkunen, Hannu
dc.date.accessioned2019-07-30T04:55:44Z
dc.date.available2019-07-30T04:55:44Z
dc.date.issued2019
dc.identifier.citationHelenius, I., Lajoie, J., Osborn, J. D., Paakkinen, P., & Paukkunen, H. (2019). Nuclear gluons at RHIC in a multiobservable approach. <i>Physical Review D</i>, <i>100</i>(1), Article 014004. <a href="https://doi.org/10.1103/PhysRevD.100.014004" target="_blank">https://doi.org/10.1103/PhysRevD.100.014004</a>
dc.identifier.otherCONVID_32096342
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/65146
dc.description.abstractWe explore the possibility of measuring nuclear gluon distributions at the Relativistic Heavy-Ion Collider (RHIC) with √s=200 GeV proton-nucleus collisions. In addition to measurements at central rapidity, we consider also observables at forward rapidity, consistent with proposed upgrades to the experimental capabilities of STAR and sPHENIX. The processes we consider consist of Drell-Yan dilepton, dijet, and direct photon-jet production. The Drell-Yan process is found to be an efficient probe of gluons at small momentum fractions. In order to fully utilize the potential of Drell-Yan measurements we demonstrate how the overall normalization uncertainty present in the experimental data can be fixed using other experimental observables. An asset of the RHIC collider is its flexibility to run with different ion beams, and we outline how this ability could be taken advantage of to measure the A dependence of gluon distributions for which the current constraints are scarce.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofseriesPhysical Review D
dc.rightsCC BY 4.0
dc.subject.othergluonit
dc.subject.othernuclear gluons
dc.titleNuclear gluons at RHIC in a multiobservable approach
dc.typeresearch article
dc.identifier.urnURN:NBN:fi:jyu-201907303707
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries1
dc.relation.volume100
dc.type.versionpublishedVersion
dc.rights.copyright© The Authors, 2019.
dc.rights.accesslevelopenAccessfi
dc.type.publicationarticle
dc.relation.grantnumber308301
dc.subject.ysoydinfysiikka
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.100.014004
dc.relation.funderSuomen Akatemiafi
dc.relation.funderResearch Council of Finlanden
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundinginformationI. H. and H. P. acknowledge the support from the Academy of Finland, Project No. 308301. The work of P. P. has been supported by the Magnus Ehrnrooth Foundation. The Finnish IT Center for Science (CSC) is acknowledged for super-computing resources under the Project No. jyy2580. J. O. acknowledges support from the Margaret and Herman Sokol Faculty Awards of University of Michigan and the Office of Nuclear Physics in the Office of Science of the Department of Energy under Grant No. DE-SC0013393. J. L. acknowledges support from the Office of Nuclear Physics in the Office of Science of the Department of Energy under Grants No. DE-FG02-10ER41719 and DE-FG02-92ER40962.
dc.type.okmA1


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