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dc.contributor.authorALICE Collaboration
dc.date.accessioned2023-09-07T07:41:19Z
dc.date.available2023-09-07T07:41:19Z
dc.date.issued2023
dc.identifier.citationALICE Collaboration. (2023). Enhanced Deuteron Coalescence Probability in Jets. <i>Physical Review Letters</i>, <i>131</i>, Article 042301. <a href="https://doi.org/10.1103/PhysRevLett.131.042301" target="_blank">https://doi.org/10.1103/PhysRevLett.131.042301</a>
dc.identifier.otherCONVID_184278198
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/88939
dc.description.abstractThe transverse-momentum (pT) spectra and coalescence parameters B2 of (anti)deuterons are measured in p-p collisions at √s=13  TeV for the first time in and out of jets. In this measurement, the direction of the leading particle with the highest pT in the event (pT lead > 5 GeV /c) is used as an approximation for the jet axis. The event is consequently divided into three azimuthal regions, and the jet signal is obtained as the difference between the toward region, that contains jet fragmentation products in addition to the underlying event (UE), and the transverse region, which is dominated by the UE. The coalescence parameter in the jet is found to be approximately a factor of 10 larger than that in the underlying event. This experimental observation is consistent with the coalescence picture and can be attributed to the smaller average phase space distance between nucleons in the jet cone as compared with the underlying event. The results presented in this Letter are compared to predictions from a simple nucleon coalescence model, where the phase-space distributions of nucleons are generated using PYTHIA8 with the Monash 2013 tuning, and to predictions from a deuteron production model based on ordinary nuclear reactions with parametrized energy-dependent cross sections tuned on data. The latter model is implemented in PYTHIA8.3. Both models reproduce the observed large difference between in-jet and out-of-jet coalescence parameters, although the almost flat trend of the B2Jet is not reproduced by the models, which instead give a decreasing trend.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review Letters
dc.rightsCC BY 4.0
dc.titleEnhanced Deuteron Coalescence Probability in Jets
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202309074972
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.issn0031-9007
dc.relation.volume131
dc.type.versionpublishedVersion
dc.rights.copyright© 2023 CERN, for the ALICE Collaboration
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber824093
dc.relation.grantnumber824093
dc.relation.grantnumber346327
dc.relation.grantnumber346328
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/824093/EU//STRONG-2020
dc.subject.ysohiukkasfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevLett.131.042301
dc.relation.funderEuropean Commissionen
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderEuroopan komissiofi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramRIA Research and Innovation Action, H2020en
jyx.fundingprogramCentre of Excellence, AoFen
jyx.fundingprogramCentre of Excellence, AoFen
jyx.fundingprogramRIA Research and Innovation Action, H2020fi
jyx.fundingprogramHuippuyksikkörahoitus, SAfi
jyx.fundingprogramHuippuyksikkörahoitus, SAfi
dc.type.okmA1


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