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dc.contributor.authorWalt, Marina
dc.contributor.authorHelenius, Ilkka
dc.contributor.authorVogelsang, Werner
dc.date.accessioned2019-11-26T12:41:53Z
dc.date.available2019-11-26T12:41:53Z
dc.date.issued2019
dc.identifier.citationWalt, M., Helenius, I., & Vogelsang, W. (2019). Open-source QCD analysis of nuclear parton distribution functions at NLO and NNLO. <i>Physical Review D</i>, <i>100</i>(9), Article 096015. <a href="https://doi.org/10.1103/PhysRevD.100.096015" target="_blank">https://doi.org/10.1103/PhysRevD.100.096015</a>
dc.identifier.otherCONVID_33624289
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/66528
dc.description.abstractWe present new sets of nuclear parton distribution functions (nPDFs) at next-to-leading order and next-to-next-to-leading order. Our analyses are based on deeply inelastic scattering data with charged-lepton and neutrino beams on nuclear targets. In addition, a set of proton baseline PDFs is fitted within the same framework with the same theoretical assumptions. The results of this global QCD analysis are compared to existing nPDF sets and to the fitted cross sections. Also, the uncertainties resulting from the limited constraining power of the included experimental data are presented. The published work is based on an open-source tool, xfitter, which has been modified to be applicable also for a nuclear PDF analysis. The required extensions of the code are discussed as well.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.othernonperturbative effects in field theory
dc.subject.othernuclear matter
dc.subject.othernucleon distribution
dc.subject.othernucleus-neutrino interactions
dc.subject.otherparticle interactions
dc.subject.otherperturbation theory
dc.subject.otherQCD in nuclear reactions
dc.subject.otherquantum chromodynamics
dc.subject.otherquantum field theory
dc.titleOpen-source QCD analysis of nuclear parton distribution functions at NLO and NNLO
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201911265018
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.numberinseries9
dc.relation.volume100
dc.type.versionpublishedVersion
dc.rights.copyright© Authors, 2019
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber308301
dc.subject.ysohiukkasfysiikka
dc.subject.ysoydinfysiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p14759
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.100.096015
dc.relation.funderResearch Council of Finlanden
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundinginformationThis work was supported in part by the Bundesministerium für Bildung und Forschung (BMBF) Grant No. 5P18VTCA1, Carl Zeiss Foundation and by the Academy of Finland, Project No. 308301.
dc.type.okmA1


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