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dc.contributor.authorHuss, Alexander
dc.contributor.authorKurkela, Eero Aleksi
dc.contributor.authorMazeliauskas, Aleksas
dc.contributor.authorPaatelainen, Risto
dc.contributor.authorvan der Schee, Wilke
dc.contributor.authorWiedemann, Urs Achim
dc.date.accessioned2022-02-11T12:04:07Z
dc.date.available2022-02-11T12:04:07Z
dc.date.created2022-01-25T10:38:29Z
dc.date.issued2021-05
dc.identifier.citationHuss, A., Kurkela, A., Mazeliauskas, A., Paatelainen, R., van der Schee, W., Achim, U. (2021) Discovering Partonic Rescattering in Light Nucleus Collisions. Physical Review Letters, 126, 192301en_US
dc.identifier.issn0031-9007
dc.identifier.urihttps://hdl.handle.net/11250/2978470
dc.description.abstractWe demonstrate that oxygen-oxygen collisions at the LHC provide unprecedented sensitivity to parton energy loss in a system whose size is comparable to those created in very peripheral heavy-ion collisions. With leading and next-to-leading order calculations of nuclear modification factors, we show that the baseline in the absence of partonic rescattering is known with up to 2% theoretical accuracy in inclusive oxygen-oxygen collisions. Surprisingly, a Z-boson normalized nuclear modification factor does not lead to higher theoretical accuracy within current uncertainties of nuclear parton distribution functions. We study a broad range of parton energy loss models and we find that the expected signal of partonic rescattering can be disentangled from the baseline by measuring charged hadron spectra in the range 20 GeV < pT < 100 GeV.en_US
dc.language.isoengen_US
dc.publisherAmerican Physical Societyen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.subjectfysikken_US
dc.titleDiscovering Partonic Rescattering in Light Nucleus Collisionsen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.subject.nsiVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430en_US
dc.source.volume126en_US
dc.source.journalPhysical Review Lettersen_US
dc.identifier.doi10.1103/PhysRevLett.126.192301
dc.identifier.cristin1989239
dc.source.articlenumber192301en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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