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dc.contributor.authorCasuga, Carlisle
dc.contributor.authorKarhunen, Mikko
dc.contributor.authorMäntysaari, Heikki
dc.date.accessioned2024-05-23T05:51:55Z
dc.date.available2024-05-23T05:51:55Z
dc.date.issued2024
dc.identifier.citationCasuga, C., Karhunen, M., & Mäntysaari, H. (2024). Inferring the initial condition for the Balitsky-Kovchegov equation. <i>Physical Review D</i>, <i>109</i>(5), Article 054018. <a href="https://doi.org/10.1103/PhysRevD.109.054018" target="_blank">https://doi.org/10.1103/PhysRevD.109.054018</a>
dc.identifier.otherCONVID_213715336
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/95088
dc.description.abstractWe apply Bayesian inference to determine the posterior likelihood distribution for the parameters describing the initial condition of the small-x Balitsky-Kovchegov evolution equation at leading logarithmic accuracy. The HERA structure function data is found to constrain most of the model parameters well. In particular, we find that the HERA data prefers an anomalous dimension γ≈1 unlike in previous fits where γ>1 which led to e.g. the unintegrated gluon distribution and the quark-target cross sections not being positive definite. The determined posterior distribution can be used to propagate the uncertainties in the non-perturbative initial condition when calculating any other observable in the Color Glass Condensate framework. We demonstrate this explicitly for the inclusive quark production cross section in proton-proton collisions and by calculating predictions for the nuclear modification factor for the F2 structure function in the EIC and LHeC/FCC-he kinematics.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review D
dc.rightsCC BY 4.0
dc.titleInferring the initial condition for the Balitsky-Kovchegov equation
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202405233852
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.numberinseries5
dc.relation.volume109
dc.type.versionpublishedVersion
dc.rights.copyright© 2024 the Authors
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber835105
dc.relation.grantnumber835105
dc.relation.grantnumber824093
dc.relation.grantnumber824093
dc.relation.grantnumber346567
dc.relation.grantnumber338263
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/835105/EU//YoctoLHC
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/824093/EU//STRONG-2020
dc.subject.ysohiukkasfysiikka
dc.subject.ysokvarkit
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p19627
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1103/PhysRevD.109.054018
dc.relation.funderEuropean Commissionen
dc.relation.funderEuropean Commissionen
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderEuroopan komissiofi
dc.relation.funderEuroopan komissiofi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
jyx.fundingprogramERC Advanced Granten
jyx.fundingprogramRIA Research and Innovation Action, H2020en
jyx.fundingprogramResearch costs of Academy Research Fellow, AoFen
jyx.fundingprogramAcademy Research Fellow, AoFen
jyx.fundingprogramERC Advanced Grantfi
jyx.fundingprogramRIA Research and Innovation Action, H2020fi
jyx.fundingprogramAkatemiatutkijan tutkimuskulut, SAfi
jyx.fundingprogramAkatemiatutkija, SAfi
jyx.fundinginformationH. M and C. C. are supported by the Research Council of Finland, the Centre of Excellence in Quark Matter and projects 338263 and 346567. C. C. also acknowledges the support of the Vilho, Yrjö, and Kalle Väisälä Foundation. This work was also supported under the European Union’s Horizon 2020 research and innovation programme by the European Research Council (ERC, Grant Agreement No. ERC-2018-ADG-835105 YoctoLHC) and by the STRONG-2020 project (Grant Agreement No. 824093).
dc.type.okmA1


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