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dc.contributor.authorCMS Collaboration
dc.date.accessioned2023-08-16T16:10:33Z
dc.date.available2023-08-16T16:10:33Z
dc.date.issued2023-07-10
dc.identifier.citationTumasyan, A., Adam, W., Andrejkovic, J.W. et al. CMS PYTHIA 8 colour reconnection tunes based on underlying-event data. Eur. Phys. J. C 83, 587 (2023). https://doi.org/10.1140/epjc/s10052-023-11630-8en_US
dc.identifier.urihttps://hdl.handle.net/1808/34742
dc.description.abstractNew sets of parameter tunes for two of the colour reconnection models, quantum chromodynamics-inspired and gluon-move, implemented in the PYTHIA 8 event generator, are obtained based on the default CMS PYTHIA 8 underlying-event tune, CP5. Measurements sensitive to the underlying event performed by the CMS experiment at centre-of-mass energies √𝑠=7 and 13TeV, and by the CDF experiment at 1.96TeV are used to constrain the parameters of colour reconnection models and multiple-parton interactions simultaneously. The new colour reconnection tunes are compared with various measurements at 1.96, 7, 8, and 13TeV including measurements of the underlying-event, strange-particle multiplicities, jet substructure observables, jet shapes, and colour flow in top quark pair (tt¯) events. The new tunes are also used to estimate the uncertainty related to colour reconnection modelling in the top quark mass measurement using the decay products of tt¯ events in the semileptonic channel at 13TeV.en_US
dc.publisherSpringerOpenen_US
dc.rights© CERN for the benefit of the CMS collaboration 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleCMS PYTHIA 8 colour reconnection tunes based on underlying-event dataen_US
dc.typeArticleen_US
kusw.kuauthorAbreu, A.
kusw.kuauthorAnguiano, J.
kusw.kuauthorBaldenegro Barrera, C.
kusw.kuauthorBaringer, P.
kusw.kuauthorBean, A.
kusw.kuauthorBylinkin, A.
kusw.kuauthorFlowers, Z.
kusw.kuauthorIsidori, T.
kusw.kuauthorKhalil, S.
kusw.kuauthorKing, J.
kusw.kuauthorKrintiras, G.
kusw.kuauthorKropivnitskaya, A.
kusw.kuauthorLazarovits, M.
kusw.kuauthorLe Mahieu, C.
kusw.kuauthorLindsey, C.
kusw.kuauthorMarquez, J.
kusw.kuauthorMinafra, N.
kusw.kuauthorMurray, M.
kusw.kuauthorNickel, M.
kusw.kuauthorRogan, C.
kusw.kuauthorRoyon, C.
kusw.kuauthorSalvatico, R.
kusw.kuauthorSanders, S.
kusw.kuauthorSchmitz, E.
kusw.kuauthorSmith, C.
kusw.kuauthorWang, Q.
kusw.kuauthorWarner, Z.
kusw.kuauthorWilliams, J.
kusw.kuauthorWilson, G.
dc.identifier.doi10.1140/epjc/s10052-023-11630-8en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.identifier.pmidPMC10333420en_US
dc.rights.accessrightsopenAccessen_US


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© CERN for the benefit of the CMS collaboration 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.
Except where otherwise noted, this item's license is described as: © CERN for the benefit of the CMS collaboration 2023. This article is licensed under a Creative Commons Attribution 4.0 International License.