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dc.contributor.authorIsaksen, Johannes Hamre
dc.contributor.authorTywoniuk, Konrad
dc.date.accessioned2022-04-08T09:14:59Z
dc.date.available2022-04-08T09:14:59Z
dc.date.created2021-12-02T16:23:55Z
dc.date.issued2021
dc.identifier.issn1126-6708
dc.identifier.urihttps://hdl.handle.net/11250/2990721
dc.description.abstractWe study hard 1 → 2 final-state parton splittings in the medium, and put special emphasis on calculating the Wilson line correlators that appear in these calculations. As partons go through the medium their color continuously rotates, an effect that is encapsulated in a Wilson line along their trajectory. When calculating observables, one typically has to calculate traces of two or more medium-averaged Wilson lines. These are usually dealt with in the literature by invoking the large-Nc limit, but exact calculations have been lacking in many cases. In our work, we show how correlators of multiple Wilson lines appear, and develop a method to calculate them numerically to all orders in Nc. Initially, we focus on the trace of four Wilson lines, which we develop a differential equation for. We will then generalize this calculation to a product of an arbitrary number of Wilson lines, and show how to do the exact calculation numerically, and even analytically in the large-Nc limit. Color sub-leading corrections, that are suppressed with a factor \( {N}_c^{-2} \) relative to the leading scaling, are calculated explicitly for the four-point correlator and we discuss how to extend this method to the general case. These results are relevant for high-pT jet processes and initial stage physics at the LHC.en_US
dc.language.isoengen_US
dc.publisherSpringeren_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleWilson line correlators beyond the large-Ncen_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2021 The Author(s)en_US
dc.source.articlenumber125en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.doi10.1007/JHEP11(2021)125
dc.identifier.cristin1963730
dc.source.journalJournal of High Energy Physics (JHEP)en_US
dc.identifier.citationJournal of High Energy Physics (JHEP). 2021, 2021, 125.en_US
dc.source.volume2021en_US
dc.source.issue11en_US


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Navngivelse 4.0 Internasjonal
Except where otherwise noted, this item's license is described as Navngivelse 4.0 Internasjonal