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dc.contributor.authorLappi, T.
dc.contributor.authorMäntysaari, H.
dc.contributor.authorRamnath, A.
dc.date.accessioned2021-11-08T10:40:14Z
dc.date.available2021-11-08T10:40:14Z
dc.date.issued2021
dc.identifier.citationLappi, T., Mäntysaari, H., & Ramnath, A. (2021). Finite Nc corrections in the Balitsky-Kovchegov equation at next-to-leading order. In <i>HardProbes2020 : 10th International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions</i> (Article 102). Sissa Medialab. POS Proceedings of Science, 387. <a href="https://doi.org/10.22323/1.387.0102" target="_blank">https://doi.org/10.22323/1.387.0102</a>
dc.identifier.otherCONVID_101764810
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/78534
dc.description.abstractWe study the finite-Nc corrections to the next-to-leading order (NLO) Balitsky--Kovchegov (BK) equation. This contains correlators of six Wilson lines, which we express in terms of the two-point function using the Gaussian approximation. Numerically, the effects of these finite-Nc corrections on the NLO BK equation are found to be smaller than the expected 1/Nc^2 ∼ 10 percent. Corrections may be large for individual correlators, but have less of an influence on the shape of the amplitude as a function of the dipole size. There is an even smaller effect on the evolution speed as a function of rapidity.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherSissa Medialab
dc.relation.ispartofHardProbes2020 : 10th International Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions
dc.relation.ispartofseriesPOS Proceedings of Science
dc.rightsCC BY-NC-ND 4.0
dc.titleFinite Nc corrections in the Balitsky-Kovchegov equation at next-to-leading order
dc.typeconferenceObject
dc.identifier.urnURN:NBN:fi:jyu-202111085557
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/ConferencePaper
dc.type.coarhttp://purl.org/coar/resource_type/c_5794
dc.description.reviewstatuspeerReviewed
dc.relation.issn1824-8039
dc.type.versionpublishedVersion
dc.rights.copyright© 2021 the Authors
dc.rights.accesslevelopenAccessfi
dc.relation.conferenceInternational Conference on Hard and Electromagnetic Probes of High-Energy Nuclear Collisions
dc.relation.grantnumber314764
dc.relation.grantnumber321840
dc.relation.grantnumber681707
dc.relation.grantnumber681707
dc.relation.projectidinfo:eu-repo/grantAgreement/EC/H2020/681707/EU//CGCglasmaQGP
dc.subject.ysohiukkasfysiikka
dc.subject.ysokvanttiväridynamiikka
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p39318
dc.rights.urlhttps://creativecommons.org/licenses/by-nc-nd/4.0/
dc.relation.doi10.22323/1.387.0102
dc.relation.funderResearch Council of Finlanden
dc.relation.funderResearch Council of Finlanden
dc.relation.funderEuropean Commissionen
dc.relation.funderSuomen Akatemiafi
dc.relation.funderSuomen Akatemiafi
dc.relation.funderEuroopan komissiofi
jyx.fundingprogramPostdoctoral Researcher, AoFen
jyx.fundingprogramAcademy Project, AoFen
jyx.fundingprogramERC European Research Council, H2020en
jyx.fundingprogramTutkijatohtori, SAfi
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramERC European Research Council, H2020fi
jyx.fundinginformationThis work was supported by the Academy of Finland, projects 314764 (H. M.) and 321840 (T.L.), and by the National Research Foundation of South Africa (A. R.). A. R. and T. L. are supported by the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme (grant agreement No. ERC-2015-CoG-681707). The content of this article does not reflect the official opinion of the European Union and responsibility for the information and views expressed therein lies entirely with the authors. Computing resources from CSC – IT Center for Science in Espoo, Finland and from the Finnish Grid and Cloud Infrastructure (persistent identifier urn:nbn:fi:research-infras-2016072533) were used in this work.
dc.type.okmA4


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