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. 2023 Jul 10;83(7):587. doi: 10.1140/epjc/s10052-023-11630-8

CMS pythia  8 colour reconnection tunes based on underlying-event data

A Tumasyan 1,181, W Adam 2, J W Andrejkovic 2, T Bergauer 2, S Chatterjee 2, K Damanakis 2, M Dragicevic 2, A Escalante Del Valle 2, R Frühwirth 2,182, M Jeitler 2,182, N Krammer 2, L Lechner 2, D Liko 2, I Mikulec 2, P Paulitsch 2, F M Pitters 2, J Schieck 2,182, R Schöfbeck 2, D Schwarz 2, S Templ 2, W Waltenberger 2, C-E Wulz 2,182, M R Darwish 3,183, E A De Wolf 3, T Janssen 3, T Kello 3,184, A Lelek 3, H Rejeb Sfar 3, P Van Mechelen 3, S Van Putte 3, N Van Remortel 3, E S Bols 4, J D’Hondt 4, M Delcourt 4, H El Faham 4, S Lowette 4, S Moortgat 4, A Morton 4, D Müller 4, A R Sahasransu 4, S Tavernier 4, W Van Doninck 4, D Vannerom 4, D Beghin 5, B Bilin 5, B Clerbaux 5, G De Lentdecker 5, L Favart 5, A K Kalsi 5, K Lee 5, M Mahdavikhorrami 5, I Makarenko 5, L Moureaux 5, S Paredes 5, L Pétré 5, A Popov 5, N Postiau 5, E Starling 5, L Thomas 5, M Vanden Bemden 5, C Vander Velde 5, P Vanlaer 5, T Cornelis 6, D Dobur 6, J Knolle 6, L Lambrecht 6, G Mestdach 6, M Niedziela 6, C Rendón 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Iaydjiev 11, M Misheva 11, M Rodozov 11, M Shopova 11, G Sultanov 11, A Dimitrov 12, T Ivanov 12, L Litov 12, B Pavlov 12, P Petkov 12, A Petrov 12, T Cheng 13, T Javaid 13,188, M Mittal 13, L Yuan 13, M Ahmad 14, G Bauer 14, C Dozen 14, Z Hu 14, J Martins 14,189, Y Wang 14, K Yi 14,190,191, E Chapon 15, G M Chen 15,188, H S Chen 15,188, M Chen 15, F Iemmi 15, A Kapoor 15, D Leggat 15, H Liao 15, Z-A Liu 15,192, V Milosevic 15, F Monti 15, R Sharma 15, J Tao 15, J Thomas-Wilsker 15, J Wang 15, H Zhang 15, J Zhao 15, A Agapitos 16, Y An 16, Y Ban 16, C Chen 16, A Levin 16, Q Li 16, X Lyu 16, Y Mao 16, S J Qian 16, D Wang 16, J Xiao 16, H Yang 16, M Lu 17, Z You 17, X Gao 18,184, H Okawa 18, Y Zhang 18, Z Lin 19, M Xiao 19, C Avila 20, A Cabrera 20, C Florez 20, J Fraga 20, J Mejia Guisao 21, F Ramirez 21, J D Ruiz Alvarez 21, D Giljanovic 22, N Godinovic 22, D Lelas 22, I Puljak 22, Z Antunovic 23, M Kovac 23, T Sculac 23, V Brigljevic 24, D Ferencek 24, D Majumder 24, M Roguljic 24, A Starodumov 24,193, T Susa 24, A Attikis 25, K Christoforou 25, A Ioannou 25, G Kole 25, M Kolosova 25, S Konstantinou 25, J Mousa 25, C Nicolaou 25, F Ptochos 25, P A Razis 25, H Rykaczewski 25, H Saka 25, M Finger 26,193, M Finger Jr 26,193, A Kveton 26, E Ayala 27, E Carrera Jarrin 28, A A Abdelalim 29,194,195, S Khalil 29,195, M A Mahmoud 30, Y Mohammed 30, S Bhowmik 31, R K Dewanjee 31, K Ehataht 31, M Kadastik 31, S Nandan 31, C Nielsen 31, J Pata 31, M Raidal 31, L Tani 31, C Veelken 31, P Eerola 32, H Kirschenmann 32, K Osterberg 32, M Voutilainen 32, S Bharthuar 33, E Brücken 33, F Garcia 33, J Havukainen 33, M S Kim 33, R Kinnunen 33, T Lampén 33, K Lassila-Perini 33, S Lehti 33, T Lindén 33, M Lotti 33, L Martikainen 33, M Myllymäki 33, J Ott 33, H Siikonen 33, E Tuominen 33, J Tuominiemi 33, P Luukka 34, H Petrow 34, T Tuuva 34, C Amendola 35, M Besancon 35, F Couderc 35, M Dejardin 35, D Denegri 35, J L Faure 35, F Ferri 35, S Ganjour 35, P Gras 35, G Hamel de Monchenault 35, P Jarry 35, B Lenzi 35, E Locci 35, J Malcles 35, J Rander 35, A Rosowsky 35, MÖ Sahin 35, A Savoy-Navarro 35,196, M Titov 35, G B Yu 35, S Ahuja 36, F Beaudette 36, M Bonanomi 36, A Buchot Perraguin 36, P Busson 36, A Cappati 36, C Charlot 36, O Davignon 36, B Diab 36, G Falmagne 36, S Ghosh 36, R Granier de Cassagnac 36, A Hakimi 36, I Kucher 36, J Motta 36, M Nguyen 36, C Ochando 36, P Paganini 36, J Rembser 36, R Salerno 36, U Sarkar 36, J B Sauvan 36, Y Sirois 36, A Tarabini 36, A Zabi 36, A Zghiche 36, J-L Agram 37,197, J Andrea 37, D Apparu 37, D Bloch 37, G Bourgatte 37, J-M Brom 37, E C Chabert 37, C Collard 37, D Darej 37, J-C Fontaine 37,197, U Goerlach 37, C Grimault 37, A-C Le Bihan 37, E Nibigira 37, P Van Hove 37, E Asilar 38, S Beauceron 38, C Bernet 38, G Boudoul 38, C Camen 38, A Carle 38, N Chanon 38, D Contardo 38, P Depasse 38, H El Mamouni 38, J Fay 38, S Gascon 38, M Gouzevitch 38, B Ille 38, I B Laktineh 38, H Lattaud 38, A Lesauvage 38, M Lethuillier 38, L Mirabito 38, S Perries 38, K Shchablo 38, V Sordini 38, L Torterotot 38, G Touquet 38, M Vander Donckt 38, S Viret 38, I Lomidze 39, T Toriashvili 39,198, Z Tsamalaidze 39,193, V Botta 40, L Feld 40, K Klein 40, M Lipinski 40, D Meuser 40, A Pauls 40, N Röwert 40, J Schulz 40, M Teroerde 40, A Dodonova 41, D Eliseev 41, M Erdmann 41, P Fackeldey 41, B Fischer 41, T Hebbeker 41, K Hoepfner 41, F Ivone 41, L Mastrolorenzo 41, M Merschmeyer 41, A Meyer 41, G Mocellin 41, S Mondal 41, S Mukherjee 41, D Noll 41, A Novak 41, A Pozdnyakov 41, Y Rath 41, H Reithler 41, A Schmidt 41, S C Schuler 41, A Sharma 41, L Vigilante 41, S Wiedenbeck 41, S Zaleski 41, C Dziwok 42, G Flügge 42, W Haj Ahmad 42,199, O Hlushchenko 42, T Kress 42, A Nowack 42, O Pooth 42, D Roy 42, A Stahl 42,200, T Ziemons 42, A Zotz 42, H Aarup Petersen 43, M Aldaya Martin 43, P Asmuss 43, S Baxter 43, M Bayatmakou 43, O Behnke 43, A Bermúdez Martínez 43, S Bhattacharya 43, A A Bin Anuar 43, F Blekman 43, K Borras 43,201, D Brunner 43, A Campbell 43, A Cardini 43, C Cheng 43, F Colombina 43, S Consuegra Rodríguez 43, G Correia Silva 43, V Danilov 43, M De Silva 43, L Didukh 43, G Eckerlin 43, D Eckstein 43, L I Estevez Banos 43, O Filatov 43, E Gallo 43,202, A Geiser 43, A Giraldi 43, A Grohsjean 43, M Guthoff 43, A Jafari 43,203, N Z Jomhari 43, A Kasem 43,201, M Kasemann 43, H Kaveh 43, C Kleinwort 43, R Kogler 43, D Krücker 43, W Lange 43, K Lipka 43, W Lohmann 43,204, R Mankel 43, I-A Melzer-Pellmann 43, M Mendizabal Morentin 43, J Metwally 43, A B Meyer 43, M Meyer 43, J Mnich 43, A Mussgiller 43, A Nürnberg 43, Y Otarid 43, D Pérez Adán 43, D Pitzl 43, A Raspereza 43, B Ribeiro Lopes 43, J Rübenach 43, A Saggio 43, A Saibel 43, M Savitskyi 43, M Scham 43,205, V Scheurer 43, S Schnake 43, P Schütze 43, C Schwanenberger 43,202, M Shchedrolosiev 43, R E Sosa Ricardo 43, D Stafford 43, N Tonon 43, M Van De Klundert 43, F Vazzoler 43, R Walsh 43, D Walter 43, Q Wang 43, Y Wen 43, K Wichmann 43, L Wiens 43, C Wissing 43, S Wuchterl 43, R Aggleton 44, S Albrecht 44, S Bein 44, L Benato 44, P Connor 44, K De Leo 44, M Eich 44, F Feindt 44, A Fröhlich 44, C Garbers 44, E Garutti 44, P Gunnellini 44, M Hajheidari 44, J Haller 44, A Hinzmann 44, G Kasieczka 44, R Klanner 44, T Kramer 44, V Kutzner 44, J Lange 44, T Lange 44, A Lobanov 44, A Malara 44, A Mehta 44, A Nigamova 44, K J Pena Rodriguez 44, M Rieger 44, O Rieger 44, P Schleper 44, M Schröder 44, J Schwandt 44, J Sonneveld 44, H Stadie 44, G Steinbrück 44, A Tews 44, I Zoi 44, J Bechtel 45, S Brommer 45, M Burkart 45, E Butz 45, R Caspart 45, T Chwalek 45, W De Boer 45, A Dierlamm 45, A Droll 45, K El Morabit 45, N Faltermann 45, M Giffels 45, J O Gosewisch 45, A Gottmann 45, F Hartmann 45,200, C Heidecker 45, U Husemann 45, P Keicher 45, R Koppenhöfer 45, S Maier 45, M Metzler 45, S Mitra 45, Th Müller 45, M Neukum 45, G Quast 45, K Rabbertz 45, J Rauser 45, D Savoiu 45, M Schnepf 45, D Seith 45, I Shvetsov 45, H J Simonis 45, R Ulrich 45, J Van Der Linden 45, R F Von Cube 45, M Wassmer 45, M Weber 45, S Wieland 45, R Wolf 45, S Wozniewski 45, S Wunsch 45, G Anagnostou 46, G Daskalakis 46, A Kyriakis 46, A Stakia 46, M Diamantopoulou 47, D Karasavvas 47, P Kontaxakis 47, C K Koraka 47, A Manousakis-Katsikakis 47, A Panagiotou 47, I Papavergou 47, N Saoulidou 47, K Theofilatos 47, E Tziaferi 47, K Vellidis 47, E Vourliotis 47, G Bakas 48, K Kousouris 48, I Papakrivopoulos 48, G Tsipolitis 48, A Zacharopoulou 48, K Adamidis 49, I Bestintzanos 49, I Evangelou 49, C Foudas 49, P Gianneios 49, P Katsoulis 49, P Kokkas 49, N Manthos 49, I Papadopoulos 49, J Strologas 49, M Csanád 50, K Farkas 50, M M A Gadallah 50,206, S Lökös 50,207, P Major 50, K Mandal 50, G Pásztor 50, A J Rádl 50, O Surányi 50, G I Veres 50, M Bartók 51,208, G Bencze 51, C Hajdu 51, D Horvath 51,209,210, F Sikler 51, V Veszpremi 51, S Czellar 52, D Fasanella 52, F Fienga 52, J Karancsi 52,208, J Molnar 52, Z Szillasi 52, D Teyssier 52, P Raics 53, Z L Trocsanyi 53,211, B Ujvari 53, T Csorgo 54,212, F Nemes 54,212, T Novak 54, S Bansal 55, S B Beri 55, V Bhatnagar 55, G Chaudhary 55, S Chauhan 55, N Dhingra 55,213, R Gupta 55, A Kaur 55, H Kaur 55, M Kaur 55, P Kumari 55, M Meena 55, K Sandeep 55, J B Singh 55, A K Virdi 55, A Ahmed 56, A Bhardwaj 56, B C Choudhary 56, M Gola 56, S Keshri 56, A Kumar 56, M Naimuddin 56, P Priyanka 56, K Ranjan 56, A Shah 56, M Bharti 57,214, R Bhattacharya 57, S Bhattacharya 57, D Bhowmik 57, S Dutta 57, S Dutta 57, B Gomber 57,215, M Maity 57,216, P Palit 57, P K Rout 57, G Saha 57, B Sahu 57, S Sarkar 57, M Sharan 57, P K Behera 58, S C Behera 58, P Kalbhor 58, J R Komaragiri 58,217, D Kumar 58,217, A Muhammad 58, L Panwar 58,217, R Pradhan 58, P R Pujahari 58, A Sharma 58, A K Sikdar 58, P C Tiwari 58,217, K Naskar 59,218, T Aziz 60, S Dugad 60, M Kumar 60, G B Mohanty 60, S Banerjee 61, R Chudasama 61, M Guchait 61, S Karmakar 61, S Kumar 61, G Majumder 61, K Mazumdar 61, S Mukherjee 61, S Bahinipati 62,219, C Kar 62, P Mal 62, T Mishra 62, V K Muraleedharan Nair Bindhu 62,220, A Nayak 62,220, P Saha 62, N Sur 62, S K Swain 62, D Vats 62,220, A Alpana 63, S Dube 63, B Kansal 63, A Laha 63, S Pandey 63, A Rastogi 63, S Sharma 63, H Bakhshiansohi 64,221, E Khazaie 64, M Zeinali 64,222, S Chenarani 65,223, S M Etesami 65, M Khakzad 65, M Mohammadi Najafabadi 65, M Grunewald 66, M Abbrescia 67, R Aly 67,194, C Aruta 67, A Colaleo 67, D Creanza 67, N De Filippis 67, M De Palma 67, A Di Florio 67, A Di Pilato 67, W Elmetenawee 67, F Errico 67, L Fiore 67, A Gelmi 67, M Gul 67, G Iaselli 67, M Ince 67, S Lezki 67, G Maggi 67, M Maggi 67, I Margjeka 67, V Mastrapasqua 67, S My 67, S Nuzzo 67, A Pellecchia 67, A Pompili 67, G Pugliese 67, D Ramos 67, A Ranieri 67, G Selvaggi 67, L Silvestris 67, F M Simone 67, Ü Sözbilir 67, R Venditti 67, P Verwilligen 67, G Abbiendi 68, C Battilana 68, D Bonacorsi 68, L Borgonovi 68, L Brigliadori 68, R Campanini 68, P Capiluppi 68, A Castro 68, F R Cavallo 68, C Ciocca 68, M Cuffiani 68, G M Dallavalle 68, T Diotalevi 68, F Fabbri 68, A Fanfani 68, P Giacomelli 68, L Giommi 68, C Grandi 68, L Guiducci 68, S Lo Meo 68,224, L Lunerti 68, S Marcellini 68, G Masetti 68, F L Navarria 68, A Perrottas 68, F Primavera 68, A M Rossi 68, T Rovelli 68, G P Siroli 68, S Albergo 69,225, S Costa 69,225, A Di Mattia 69, R Potenza 69, A Tricomi 69,225, C Tuve 69, G Barbagli 70, A Cassese 70, R Ceccarelli 70, V Ciulli 70, C Civinini 70, R D’Alessandro 70, E Focardi 70, G Latino 70, P Lenzi 70, M Lizzo 70, M Meschini 70, S Paoletti 70, R Seidita 70, G Sguazzoni 70, L Viliani 70, L Benussi 71, S Bianco 71, D Piccolo 71, M Bozzo 72, F Ferro 72, R Mulargia 72, E Robutti 72, S Tosi 72, A Benaglia 73, G Boldrini 73, F Brivio 73, F Cetorelli 73, F De Guio 73, M E Dinardo 73, P Dini 73, S Gennai 73, A Ghezzi 73, P Govoni 73, L Guzzi 73, M T Lucchini 73, M Malberti 73, S Malvezzi 73, A Massironi 73, D Menasce 73, L Moroni 73, M Paganoni 73, D Pedrini 73, B S Pinolini 73, S Ragazzi 73, N Redaelli 73, T Tabarelli de Fatis 73, D Valsecchi 73,200, D Zuolo 73, S Buontempo 74, F Carnevali 74, N Cavallo 74, A De Iorio 74, F Fabozzi 74, A O M Iorio 74, L Lista 74,226, S Meola 74,200, P Paolucci 74,200, B Rossi 74, C Sciacca 74, P Azzi 75, N Bacchetta 75, D Bisello 75, P Bortignon 75, A Bragagnolo 75, R Carlin 75, P Checchia 75, T Dorigo 75, U Dosselli 75, F Gasparini 75, U Gasparini 75, G Grosso 75, S Y Hoh 75, L Layer 75,227, E Lusiani 75, M Margoni 75, A T Meneguzzo 75, J Pazzini 75, P Ronchese 75, R Rossin 75, F Simonetto 75, G Strong 75, M Tosi 75, H Yarar 75, M Zanetti 75, P Zotto 75, A Zucchetta 75, G Zumerle 75, C Aimè 76, A Braghieri 76, S Calzaferri 76, D Fiorina 76, P Montagna 76, S P Ratti 76, V Re 76, C Riccardi 76, P Salvini 76, I Vai 76, P Vitulo 76, P Asenov 77,228, G M Bilei 77, D Ciangottini 77, L Fanò 77, M Magherini 77, G Mantovani 77, V Mariani 77, M Menichelli 77, F Moscatelli 77,228, A Piccinelli 77, M 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S Kim 89, B Ko 89, J S H Lee 89, Y Lee 89, J A Merlin 89, I C Park 89, Y Roh 89, M S Ryu 89, D Song 89, I J Watson 89, S Yang 89, S Ha 90, H D Yoo 90, M Choi 91, H Lee 91, Y Lee 91, I Yu 91, T Beyrouthy 92, Y Maghrbi 92, K Dreimanis 93, V Veckalns 93, M Ambrozas 94, A Carvalho Antunes De Oliveira 94, A Juodagalvis 94, A Rinkevicius 94, G Tamulaitis 94, N Bin Norjoharuddeen 95, Z Zolkapli 95, J F Benitez 96, A Castaneda Hernandez 96, M León Coello 96, J A Murillo Quijada 96, A Sehrawat 96, L Valencia Palomo 96, G Ayala 97, H Castilla-Valdez 97, E De La Cruz-Burelo 97, I Heredia-De La Cruz 97,229, R Lopez-Fernandez 97, C A Mondragon Herrera 97, D A Perez Navarro 97, R Reyes-Almanza 97, A Sánchez Hernández 97, S Carrillo Moreno 98, C Oropeza Barrera 98, F Vazquez Valencia 98, I Pedraza 99, H A Salazar Ibarguen 99, C Uribe Estrada 99, J Mijuskovic 100,230, N Raicevic 100, D Krofcheck 101, P H Butler 102, A Ahmad 103, M I Asghar 103, A Awais 103, M I M Awan 103, H R Hoorani 103, W A Khan 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PMCID: PMC10333420  PMID: 37440247

Abstract

New 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.

Introduction

Monte Carlo (MC) event generators, such as pythia  8  [1], are indispensable tools for measurements at the LHC proton–proton (pp) collider. To provide an accurate description of high-energy collisions, both the hard scattering and the so-called underlying event (UE) are computed for each simulated event. In the hard scattering process, two initial partons interact with a large exchange of transverse momentum, pT>O(GeV) (we use natural units with c=1 throughout the paper). The UE represents additional activity occurring at lower energy scales that accompany the hard scattering. It consists of multiple-parton interactions (MPIs), initial- and final-state radiation (ISR and FSR), and beam-beam remnants (BBR). According to Quantum Chromodynamics (QCD), strong interactions are affected by colour charges that are carried by quarks and gluons. All of the coloured partons produced by these components are finally combined to form colourless hadrons through the hadronisation process.

Particularly relevant for the characterisation of the UE are the MPIs, which consist of additional 2-to-2 parton–parton interactions occurring within the single collision event. With increasing collision energy, the interaction probability for partons with small longitudinal momentum fractions also increases, which enhances MPI contributions.

The pythia  8 generator regularises the cross sections of the primary hard scattering processes and MPIs with respect to the perturbative 2-to-2 parton–parton differential cross section through an energy-dependent dampening parameter pT0, which depends on the centre-of-mass energy s. The energy dependence of the pT0 parameter in pythia  8 is described with a power law function of the form

pT0(s)=pT0refss0ϵ, 1

where pT0ref is the value of pT0 at a reference energy s0, and ϵ is a tunable parameter that determines the energy dependence. At a given s, the mean number of additional interactions from MPI depends on pT0, the parton distribution functions (PDFs), and the overlap of the matter distributions of the two colliding hadrons [2].

To track the colour information during the development of the parton shower, partons are represented and also connected by colour lines. Quarks and antiquarks are represented by colour lines with arrows pointing in the direction of the colour flow, and gluons are represented by a pair of colour lines with opposite arrows. Rules for colour propagation are shown in Fig. 1. Because each MPI system adds coloured partons to the final state, a dense net of colour lines that overlap with the coloured parton fields of the hard scattering and with each other is created. Parton shower algorithms, in general, use the leading colour (LC) approximation [3, 4] in which each successively emitted parton is colour connected only to its parent emitters in the limit of infinite number of colours. Colour reconnection (CR) models allow colour lines to be formed between partons also from different interactions and thus allow different colour topologies compared with a simple LC approach.

Fig. 1.

Fig. 1

Rules for colour flow for quark-gluon vertices. Figure is taken from Ref. [5]. Quark-gluon vertices are shown in black with Feynman diagrams and colour connection lines are shown with coloured lines

The CR was first included in minimum-bias (MB) simulations (see Sect. 4.1) to reproduce the increase of average transverse momentum pT of charged particles as a function of the measured multiplicity of the charged particles, Nch, and also to describe the dNch/dη distribution [6, 7]. The pseudorapidity is defined as η=-ln[tan(θ/2)], where the polar angle θ is defined with respect to the anticlockwise-beam direction. Introducing correlations between partons, including those also resulting from MPIs, generally changes the number of charged particles in an event and allows a more realistic simulation of Nch, and pT vs Nch distributions than in an event scenario without CR [7].

The CR effects are also important for processes occurring at larger scales in pp collisions. For example, in tt¯ events, the inclusion of CR effects can lead to a significant improvement in the description of UE variables [8]. The effects of CR may become more prominent in precision measurements, such as the top quark mass mt. Uncertainties in mt related to CR are usually estimated from comparing the prediction of a given model with and without CR, which might underestimate their effect [9]. A better way to approach the uncertainty estimation would be to consider a variety of CR models and variations of their parameters [10] that probe the effects of the underlying soft physics of pp collisions on the relevant observable.

Various phenomenological models for CR have been developed and are included in pythia  8. In these models, the general idea is to determine the partonic configuration that reproduces the minimal total string length. In the Lund string fragmentation model [11] used in pythia  8, the confining colour field between two partons is approximated by a one-dimensional string stretched between the partons according to the colour flow. The fragmentation of a string with a probability given by the fragmentation function produces a set of hadrons. Thus, the colour flow of an event determines the string configuration and therefore hadronic production.

None of the MPI processes or the CR models are completely determined from first principles, and they all include free parameters. A specified set of such parameters that is adjusted to better fit some aspects of the data is referred to as a “tune”. It is possible to derive a tune that describes the data at a particular s. However, such a model, without energy dependence, will be biased and cannot provide any reliable information about other s. Thus, whenever the collision energy (s) has changed, additional constraints on the models must be applied using the information obtained from the new measurements. This is not a straightforward procedure since no single tune can describe all the data with the same precision. The default CMS pythia  8 tune CUETP8M1 for 7TeV  [12] was derived using the inputs from the 0.9, 1.96 and 7TeV measurements, and it describes the data at 7TeV quite well. The default CMS pythia  8 tune CP5, where CP stands for “CMS pythia  8 ” for 13TeV  [13] was derived using the inputs from the 1.96, 7 and 13TeV measurements. The CUETP8M1 describes data at 7TeV better than CP5, but the overall performance of CP5 is much better than CUETP8M1 when 13TeV data are also included.

This paper presents results from two tunes, which make use of the QCD-inspired [14] and the gluon-move [9] CR models. The new CR tunes presented are based on the default CMS pythia  8 tune CP5. Along with the CP5 tune, which is derived from the MPI-based CR model, the performance of the new CR tunes (CP5-CR1 and CP5-CR2 defined below) is studied using several observables. These tunes can be used for the evaluation of the uncertainties due to CR effects, and deepening the understanding of the CR mechanism.

The paper is organised as follows. In Sect. 2, the different colour reconnection models implemented in pythia  8 and used in this study are introduced. In Sect. 3, the tuning strategy is explained in detail and the parameters of the new tunes are presented. Section 4 shows a selection of validation plots related to observables measured at s=1.96, 7, 8, and 13TeV by various experiments compared with the predictions of the new tunes. In Sect. 5 a study of the uncertainty in the top quark mass mt measurement because of the CR modelling is presented before summarising the results in Sect. 6.

Colour reconnection models

The MPI-based CR model was the only CR model implemented in pythia  8 until pythia 8.2, which was released with two additional CR models. The models implemented in pythia 8.2, referred to as the “MPI-based”, “QCD-inspired”, and “gluon-move” CR models, are briefly described in the following:

  • MPI-based model (CP5): The simplest model [6, 15] implemented in MC event generators introduces only one tunable parameter. In this model, the partons are classified according to the MPI system to which they belong. Each parton interaction is originally a 22 scattering. For an MPI system with a hardness scale pT of the 22 interaction, a CR probability is defined as:
    P=pTRec2(pTRec2+pT2), 2
    with pTRec=rpT0, where r is a tunable parameter and pT0 is the energy-dependent dampening parameter defined in Eq. (1). The parameter pT0 avoids a divergence of the partonic cross section at low pT. According to Eq. (2), MPI systems at high pT would tend to escape from the interaction point, without being colour reconnected to the hard scattering system. Colour fields originating from a low-pT MPI system would instead more likely exchange colour. Once the systems to be connected are determined, partons of low-pT systems are added to strings defined by the highest pT system to achieve a minimal total string length.
  • QCD-inspired model (CP5-CR1): The QCD-inspired model [14] implemented in pythia  8 adds the QCD colour rules on top of the minimisation of the string length. The model constructs all pairs of QCD dipoles allowed to be reconnected by QCD colour rules that determine the colour compatibility of two strings. This is done iteratively until none of the allowed reconnection possibilities result in a shortening of the total string length. It uses a simple picture to causally connect the produced strings in spacetime through a string length measure λ to determine favoured reconnections. The default parametrisation for λ is
    λ=ln1+2E1m0+ln1+2E2m0, 3
    where E1 and E2 represent the energies of the coloured partons in the rest frame of the QCD dipole, and m0 is a constant with the dimension of energy [14]. In addition, the QCD-inspired model allows us to create junction structures. A junction is a topological structure and is formed when three colour lines meet at a single point. The presence of junctions reduces the number of colour lines that need to be connected to the beam remnant, which in turn can affect the number of particles produced in a collision. Since the QCD-inspired CR model allows for different color topologies beyond LC, it can successfully describe the baryon production measured at the CMS experiment [14, 16], which is not the case for previously available pythia  8 tunes.
  • Gluon-move model (CP5-CR2): In this scheme [9], final-state gluons are identified along with all the colour-connected pairs of partons. Then an iterative process starts. The difference between string lengths when a final-state gluon belonging to two connected partons is moved to another connected two-parton system is calculated. The gluon is moved to the string for which the move gives the largest reduction in total string length. This procedure can be repeated for all or a fraction of the gluons in the final state, which is controlled by the pythia  8 parameter ColourReconnection:fracGluon. In this scheme, quarks would not be reconnected, i.e. they would remain in the same position without any colour exchange. To improve this picture, the flip mechanism of the gluon-move model can be included. The flip mechanism basically allows reconnection of two different string systems, i.e. a quark can connect to a different antiquark. Junctions (Y-shaped three-quark configurations) are allowed to take part in the flip step as well, but no considerable differences are expected due to the limitation of the junction formation in this model. The flip mechanism has not been extensively studied and its effect on diffractive events is not known. For this reason the flip mechanism is switched off in pythia  8 and not used in this paper. The main free parameters of the gluon-move model account for the lower limit of the string length allowed for colour reconnection, the fraction of gluons allowed to move, and the lower limit of the allowed reduction of the string lengths.

In addition to these models, the effects of early resonance decay (ERD) [9] in top quark decays are also studied. With this option, top quark decay products are allowed to participate directly in CR. Normally the ERD option is switched off in pythia  8 but in Sect. 4.5 we investigate the ERD effects.

Usually, MPI and CR effects are investigated and constrained using fits to measurements sensitive to the UE in hadron collisions. The UE measurements have been performed at various collision energies by ATLAS, CMS, and CDF Collaborations [1721]. The measurements are typically performed by studying the multiplicity and the scalar pT sum of the charged particles (pTsum), measured as a function of the pT of the leading charged particle in the event, pTmax.

Different regions of the plane transverse to the direction of the beams are defined by the direction of the leading charged particle. A sketch of the different regions is shown in Fig. 2. A “toward” region includes mainly the products of the hard scattering, whereas the “away” region includes the recoiling objects belonging to the hard scattering. The two “transverse” regions contain the products of MPIs and are affected by contributions from ISR and FSR.

Fig. 2.

Fig. 2

The schematic description of the result of a typical hadron-hadron collision. The “toward” region contains the “toward-side” jet, whereas the “away” region may contain an “away-side” jet

In Refs. [17, 18, 21], the transverse region is further subdivided into “transMIN” and “transMAX”, defined to be the regions with the minimum and maximum number of particles between the two transverse regions. This is done to disentangle contributions from MPI, ISR, and FSR. For events with large ISR or FSR, the transMAX region contains at least one “transverse-side” jet, whereas both the transMAX and transMIN regions contain particles from the MPI and BBR. Thus, the transMIN region is sensitive to MPI and BBR, whereas the difference between transMAX and transMIN (referred to as the transDIFF region) is sensitive to ISR and FSR.

The CMS Collaboration showed that a consistent description of the Nch and the pTsum distributions is not possible using only the pythia  8 hadronisation model without taking into account the CR effects [12]. In general, the largest difference between the predictions from tunes and the data is observed in the soft region (pT2--5GeV), where CR effects are expected to be more relevant.

The new CR models, QCD-inspired and gluon-move, were implemented in pythia 8.226 after tuning the model parameters to the existing data at s=7TeV and at lower centre-of-mass energies [9, 14]. The models were tuned to different data sets starting from different baseline tune settings. The model predictions, with their default parameter settings in pythia 8.226 and CP5, are given in Fig. 3 for Nch and pTsum densities measured by the CMS experiment at 13TeV  [17] in the transMIN and transMAX regions, and in Fig. 4 for the dNch/dη distribution measured by CMS at 13TeV  [22]. In these figures, the data points, shown in black, are well described by CP5. The predictions for CP5-“QCD-inspired” and CP5-“gluon-move” were obtained by replacing the MPI-based CR model in CP5 with the QCD-inspired and gluon-move CR model, respectively. As mentioned earlier, these models were tuned to data at 7TeV and at lower centre-of-mass energies. The comparisons show that the models must be retuned to describe the underlying soft physics of pp collisions at 13TeV.

Fig. 3.

Fig. 3

The charged-particle (left) and pTsum densities (right) in the transMIN (upper) and transMAX (lower) regions as functions of the pT of the leading charged particle, pTmax, measured by the CMS experiment at s=13TeV [17]. The predictions of the tunes CP5, CP5-“QCD-inspired”, and CP5-“gluon-move” using their default parameter settings in Refs. [9, 14], are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data where the model uncertainty is also included. The comparisons show that the models do not describe the data and need to be retuned

Fig. 4.

Fig. 4

The pseudorapidity of charged hadrons, dNch/dη, measured in |η|<2 by the CMS experiment at s=13TeV [23]. The predictions of the tunes CP5, CP5-“QCD-inspired”, and CP5-“gluon-move” using their default parameter settings in Refs. [9, 14], are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data where model uncertainty is also included. The comparisons show that the models need to be retuned in order to have a better agreement with the data

The new CMS colour reconnection tunes

A new set of event tunes, based on UE data from the CMS and CDF experiments, are derived using the QCD-inspired and the gluon-move CR models, as implemented in the pythia 8.226 event generator. Having tunes for different CR models allows a consistent way of evaluating systematic uncertainties because of colour reconnection effects in specific measurements. The Rivet  2.4.0 [24] routines used as inputs to the fits, as well as the centre-of-mass energy values and the names of the Rivet distributions, the x-axis ranges (fit ranges), and the relative importance (R) of the distributions are displayed in Table 1 for the tunes CP5-CR1 and CP5-CR2. The CP5 tune is used as a baseline for the CR tuning since it is the default pythia  8 tune for most of the new CMS analyses using data at s=13TeV published since 2017, and it has explicitly been tested against a large number of different final states (MB, QCD, top quark, and vector boson + jets) and observables [13].

Table 1.

List of input Rivet routines, centre-of-mass energy values, η ranges, names of distributions, fit ranges, and relative importance of the distributions used in the fits to derive the tunes CP5-CR1 and CP5-CR2

Rivet routine s [TeV ] |η| Distribution CP5-CR1 Fit range [GeV ] R CP5-CR2 Fit range [GeV ] R
CMS_2015_I1384119 [23] 13 <2.0 Nch versus η 1 1
CMS_2015_PAS_FSQ_15_007 [17] 13 <2.0 TransMIN pTsum 2–28 1 3–36 0.5
TransMAX pTsum 2–28 1 3–36 0.5
TransMIN Nch 2–28 1 3–36 0.1
TransMAX Nch 2–28 1 3–36 0.1
CMS_2012_PAS_FSQ_12_020 [18] 7 <0.8 TransMAX Nch 3–20 1 3–20 0.1
TransMIN Nch 3–20 1 3–20 0.1
TransMAX pTsum 3–20 1 3–20 0.1
TransMIN pTsum 3–20 1 3–20 0.1
CDF_2015_I1388868 [21] 2 <0.8 TransMIN Nch 2–15 1 2–15 0.1
TransMAX Nch 2–15 1 2–15 0.1
TransMIN pTsum 2–15 1 2–15 0.1
TransMAX pTsum 2–15 1 2–15 0.1

The parameters and their ranges in the fits are shown in Table 2. The minimum and maximum values of the parameters are first taken from pythia  8, then the ranges of the values are further limited using the Professor  1.4.0 software [25]. The ranges are chosen such that the sampled MC space does not destroy the definition of a particular observable in the fits.

Table 2.

The MPI and CR parameter ranges used in the tuning procedure

pythia  8 parameter Min–Max
MPI parameters
  MultipartonInteractions:pT0Ref 1.0–3.0
  MultipartonInteractions:ecmPow 0.0–0.3
  MultipartonInteractions:coreRadius 0.2–0.8
  MultipartonInteractions:coreFraction 0.2–0.8
QCD-inspired model
  ColourReconnection:m0 0.1–4.0
  ColourReconnection:junctionCorrection 0.01–10
  ColourReconnection:timeDilationPar 0–60
Gluon-move model
  ColourReconnection:m2lambda 0.2–8.0
  ColourReconnection:fracGluon 0.8–1.0

Tune CP5 uses the next-to-next-to-leading order (NNLO) NNPDF31_nnlo_as_0118 [26] PDF set, the strong coupling parameter αS value of 0.118 for ISR, FSR, and MPI, and the MPI-based CR model. It also uses a double-Gaussian functional form with two tunable parameters, coreRadius and coreFraction, to model the overlap of the matter distribution of the two colliding protons [6]. The tune parameters are documented in Ref. [13] and displayed in Table 3. Also in Figs. 11 and 12 in Ref. [13], predictions of the CP5 tune are compared with event shape observables measured at LEP. The results show that a value of αSFSR(mZ) 0.120 better describes the data compared with higher values of αSFSR(mZ) which generally overestimates the number of final-state partons. As concluded in the Ref. [13], LEP event shape observables are well described by MadGraph 5_amc@nlo  + pythia  8 with CP5.

Table 3.

The parameters obtained in the fits of the CP5-CR1 and CP5-CR2 tunes, compared with that of the CP5 tune. The upper part of the table displays the fixed input parameters of the tune, whereas the lower part shows the fitted tune parameters. The number of degrees of freedom (Ndof) and the goodness of fit divided by Ndof are also shown

pythia  8 parameter CP5 [13] CP5-CR1 CP5-CR2
PDF set NNPDF3.1 NNLO NNPDF3.1 NNLO NNPDF3.1 NNLO
αS(mZ) 0.118 0.118 0.118
SpaceShower:rapidityOrder On On On
MultipartonInteractions:ecmRef [GeV ] 7000 7000 7000
αSISR(mZ) value/order 0.118/NLO 0.118/NLO 0.118/NLO
αSFSR(mZ) value/order 0.118/NLO 0.118/NLO 0.118/NLO
αSMPI(mZ) value/order 0.118/NLO 0.118/NLO 0.118/NLO
αSME(mZ) value/order 0.118/NLO 0.118/NLO 0.118/NLO
StringZ:aLund 0.38
StringZ:bLund 0.64
StringFlav:probQQtoQ 0.078
StringFlav:probStoUD 0.2
SigmaTotal:zeroAXB Off Off Off
BeamRemnants:remnantMode 1
ColourReconnection:mode 1 2
MultipartonInteractions:pT0Ref [GeV ] 1.410 1.375 1.454
MultipartonInteractions:ecmPow 0.033 0.033 0.054
MultipartonInteractions:coreRadius 0.763 0.605 0.649
MultipartonInteractions:coreFraction 0.630 0.445 0.489
ColourReconnection:range 5.176
ColourReconnection:junctionCorrection 0.238
ColourReconnection:timeDilationPar 8.580
ColourReconnection:m0 1.721
ColourReconnection:m2lambda 4.917
ColourReconnection:fracGluon 0.993
Ndof 183 157 158
χ2/Ndof 1.04 2.37 0.89

The new tunes are obtained by constraining simultaneously the parameters controlling the contributions of the MPI and of each of the CR models. The strategy followed to obtain the CP5-CR1 and CP5-CR2 tunes is similar to that used for the CP5 tune, i.e. the same observables sensitive to MPI are considered to constrain the parameters. These are the Nch and average pTsum as functions of the leading charged particle transverse momentum pTmax, measured in the transMIN and transMAX regions by the CMS experiment at s=13TeV [17] and 7TeV  [19] and by the CDF experiment at 1.96TeV  [21]. The Nch as a function of η, measured by CMS at s=13TeV [22] is also used in the fit. In Ref. [17], the transMIN and transMAX regions are defined with respect to both the leading charged particles and the leading charged-particle jets as reference objects. The uncertainty in measurements using leading charged particles as reference objects is lower than the uncertainty in measurements using leading charged-particle jets as reference objects. This is one of the reasons why we choose to use leading charged particle observables instead of leading charged-particle jet observables in the fits. Another reason is that we want to use the same observables that were used to derive CP5, and CP5 was derived using leading charged particle observables in the fits. As a cross-check, we also derived another version of the CP5-CR1 tune using leading charged-particle jet observables, such as Nch and average pTsum, as functions of the transverse momentum of the leading charged-particle jets in the fits. The results showed that the use of leading charged-particle jet observables in the fits makes a very small difference, which is negligible when tune uncertainties are taken into account. As for CP5, the region with pTmax between 0.5 and 2.0 or 3.0GeV is excluded depending on the distribution from the fit, since this region is affected by diffractive processes whose free parameters are not considered in the tuning procedure.

The MPI-related parameters that are kept free in both the CP5-CR1 and CP5-CR2 tunes are:

  • MultipartonInteractions:pT0Ref, the parameter pT0ref included in the regularisation of the partonic QCD cross section as described in Eq. (1). It sets the lower cutoff scale for MPIs;

  • MultipartonInteractions:ecmPow, the exponent ϵ of the s dependence as shown in Eq. (1);

  • MultipartonInteractions:coreRadius, the width of the core when a double-Gaussian matter profile is assumed for the overlap distribution between the two colliding protons [6]. A double-Gaussian form identifies an inner, dense part, which is called core, and an outer, less dense part;

  • MultipartonInteractions:coreFraction, the fraction of quarks and gluons contained in the core when a double-Gaussian matter profile is assumed.

The tunable CR parameters in CP5-CR1 that are considered in the fit are:

  • ColourReconnection:m0, the variable that determines whether a possible reconnection is actually favoured in the λ measure in Eq. (3);

  • ColourReconnection:junctionCorrection, the multiplicative correction for junction formation, applied to the m0 parameter;

  • ColourReconnection:timeDilationPar, the parameter controlling the time dilation that forbids colour reconnection between strings that are not in causal contact.

More details on these parameters are reported in Ref. [1]. For the CP5-CR1 tune, the parameters related to the hadronisation, StringZ:aLund, StringZ:bLund, StringFlav:probQQtoQ, and StringFlav:probStoUD, proposed in Ref. [14], are also used as fixed inputs to the tune. The first two of these parameters govern the longitudinal fragmentation function used in the Lund string model in pythia  8, whereas the latter two are the probability of diquark over quark fragmentation, and the ratio of strange to light quark production, respectively.

For the optimisation of CP5-CR2, the following parameters are considered:

  • ColourReconnection:m2lambda, an approximate hadronic mass-square scale and the parameter used in the calculation of λ;

  • ColourReconnection:fracGluon, the probability that a given gluon will be moved. It thus gives the average fraction of gluons being considered.

The remaining parameters of pythia  8 are kept the same as in the CP5 tune.

The fits are performed using the Professor  1.4.0 software, which takes random values for each parameter in the defined multidimensional parameter space, and Rivet, which provides the data points and uncertainties, and produces the individual generator predictions for the considered observables. About 200 different choices of parameters are considered to build a random grid in the parameter space. For each choice of parameters, one million pp inelastic scattering events, including contributions from single-diffractive dissociation (SD), double-diffractive dissociation (DD), central diffraction (CD), and nondiffractive (ND) processes, are generated. The bin-by-bin envelopes of the different MC predictions are checked. After building the grid in the parameter space, Professor performs an interpolation of the bin values for the observables in the parameter space using a third-order polynomial function. We verified that the degree of the polynomial used for the interpolation does not affect the tune results significantly. The function fb(p) models the MC response of each bin b of the observable O as a function of the parameter vector p. The final step is the minimisation of the χ2 function given by:

χ2(p)=ObO(fb(p)-Rb)2Δb2, 4

where Rb is the data value for each bin b, and Δb2 expresses the total bin uncertainty of the data.

The χ2 is not a true χ2 function as explained in the following. Treating equally all distributions that are used as inputs to the fit for the CP5-CR2 tune results in a tune that describes the data poorly; in particular, it underestimates the dNch/dη distribution measured in data at s=13TeV by about 30%. This is because the χ2 definition treats all bins equally and the importance of dNch/dη may be lost because of its relatively low precision with respect to other observables. The dNch/dη distribution is one of the key observables that is sensitive to a number of processes and, therefore, increasing the importance of this observable in the fit is reasonable.

In Professor, this is done by using weights with a nonstandard χ2 definition. To keep the standard properties of a χ2 fit, we increase the total uncertainties of the other distributions. The total uncertainty in each bin is scaled up by 1/R with R (relative importance) values displayed in Table 1. Therefore, the total uncertainty of each bin of pTsum in the transMIN and transMAX regions at s=13TeV is scaled up by 2 and that of all other distributions by 10. These scale factors ensure that the distributions are well described after the tuning. For the CP5-CR1 model, a good description of the input observables is obtained without scaling, meaning that all distributions are considered equally important.

The experimental uncertainties used in the fit, in general, have bin-to-bin correlations. However, some of the bins of the UE distributions used in the fit, e.g. pTmax>10GeV, are dominated by statistical uncertainties, which are uncorrelated between bins. In the minimisation procedure, because the correlations between bins are not available for the input measurements, the experimental uncertainties are assumed to be uncorrelated between data points.

The parameters obtained from the CP5-CR1 and CP5-CR2 fits, as well as the value of the goodness of the fit are shown in Table 3. Uncertainties in the parameters of these tunes are discussed in Appendix B. In Ref. [13], the number of degrees of freedom (Ndof), defined as the sum of the number of bins of fit observables minus the number of fit parameters, for the tune CP5 is given as 63. However, this value of Ndof corresponds to the case when only 13TeV distributions are used. The value of Ndof for CP5 consistent with our calculation in this paper is 183. The tune CP5 was derived using two additional distributions in the fits; dNch/dη at 13TeV with NSD-enhanced selection and SD-enhanced selection. Since these two observables depend on modelling of single diffraction dissociation, which is not well understood, they are not included in the fits for CP5-CR tunes. Therefore, the Ndof values for CP5-CR tunes are lower than the Ndof of CP5. The slight difference in the Ndof values between the CP5-CR1 and CP5-CR2 tunes is due to the difference in the number of fit parameters used in each tune, which are 7 and 6 respectively. Although the fit ranges for the CP5-CR tunes differ slightly, as shown in Table 1, the sum of number of bins of fit observables is the same for both tunes.

A preliminary version of the CP5-CR2 tune was derived including several jet substructure observables [2729] in the fits. This tune, called CP5-CR2-j, has been used in the MC production in the CMS experiment. The CP5-CR2 and CP5-CR2-j tunes have very similar predictions in all final states discussed in this paper, because the tunes differ slightly only in the following parameters, where the listed values are for CP5-CR2-j:

  • MultipartonInteractions:ecmPow = 0.056,

  • MultipartonInteractions:coreRadius = 0.653,

  • MultipartonInteractions:coreFraction = 0.439,

  • ColourReconnection:m2lambda = 4.395,

  • MultipartonInteractions:fracGluon = 0.990.

The CP1 and CP2 are the two tunes in the CPX (X = 1–5) tune family [13] that use an LO PDF set [26]. We also derive CR tunes based on the CP1 and CP2 settings to study the effect of using a leading order (LO) PDF set with alternative CR models, although they are not used in precision measurements. We find that the predictions of the CR tunes based on CP1 and CP2 for the MB and UE observables are similar to the predictions of CR tunes based on CP5. However, CP1-CR1 (i.e. CP1 with the QCD-inspired colour reconnection model) has a different trend in particle multiplicity distributions compared with the predictions of other tunes discussed in this study. This different trend of CP1-CR1 cannot be attributed to the use of LO PDF set, because both CP1 and CP2 use the same LO PDF set and we do not see a different trend with CP2-CR1. The different trend observed with CP1-CR1 in the particle multiplicity distributions may become a collective effect rather than a single parameter effect, and could be an input for further tuning and development of the QCD-inspired model. Therefore, in Appendix A of this paper, we present the tune settings of the CR tunes based on CP1 and CP2, along with their predictions in the particle multiplicity distributions.

Performance of the tunes

In Figs. 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17, 18 we show the observables measured at centre-of-mass energies of 1.96, 7, 8, and 13TeV. The data points are shown in black, and are compared with simulations obtained from the pythia  8 event generator with the tunes CP5 (red), CP5-CR1 (blue), and CP5-CR2 (green). For simplicity, the tunes CP5-CR1 and CP5-CR2 will be referred to as CP5-CR when convenient. The lower panels show the ratios between each MC prediction and the data.

Fig. 5.

Fig. 5

The charged-particle (left) and pTsum (right) densities in the transMIN (upper) and transMAX (lower) regions, as functions of the pT of the leading charged particle, pTmax, measured by the CMS experiment at s=13TeV [17]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 6.

Fig. 6

The pseudorapidity of charged hadrons, dNch/dη, measured by the CMS experiment at s=13TeV [22]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 7.

Fig. 7

The mean charged-particle average transverse momentum as functions of charged-particle multiplicity in the transMAX (upper) and transMIN (lower) regions, measured by the ATLAS experiment at s=13TeV [18]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 8.

Fig. 8

The charged-particle (left) and pTsum (right) densities in the transMIN (upper) and transMAX (lower) regions, as functions of the pT of the leading charged particle, pTmax, measured by the CMS experiment at s=7TeV [19]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 9.

Fig. 9

The charged-particle (upper left) and pTsum densities (upper right) in the transverse region, as functions of the pT of the leading charged particle, and average transverse momentum in the transverse region as functions of the leading charged particle pT (lower left) and of the charged particle multiplicity (lower right), measured by the ATLAS experiment at s=7TeV [20]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 10.

Fig. 10

The pseudorapidity of charged particles, dNch/dη, with at least one charged particle in |η|<2.4, measured by the CMS experiment at s=7TeV [31]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 11.

Fig. 11

The charged-particle (left) and pTsum densities (right) in the transMIN (upper) and transMAX (lower) regions, as functions of the pT of the leading charged particle, pTmax, measured by the CDF experiment at s=1.96TeV [21]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 12.

Fig. 12

The energy density as a function of pseudorapidity, in two different selections, in MB events (upper) and in events with a presence of a hard dijet system (lower), measured by the CMS experiment at s=13TeV [34]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 13.

Fig. 13

The pseudorapidity of charged particles, dNch/dη, measured by the CMS and TOTEM collaborations at s=8TeV [32] (upper) and measured by the TOTEM collaboration at s=7TeV [33] (lower). The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data. For the CMS-TOTEM measurement, at least one charged particle with pT>0 is required in 5.3<η<6.5 or -6.5<η<-5.3. For the TOTEM measurement, at least one charged particle with pT>40MeV is required in 5.3<|η|<6.4

Fig. 14.

Fig. 14

The strange particle production, Λ baryons (upper) and KS0 mesons (lower), as a function of rapidity, measured by the CMS experiment at s=7TeV [16]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 15.

Fig. 15

Ratios of particle yields, p/π, as a function of transverse momentum in minimum-bias events, measured by the CMS experiment at s=13TeV [39]. The predictions of the CP5 and CP5-CR tunes are compared with CMS data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 16.

Fig. 16

Average charged-hadron multiplicity, as a function of the jet pT, for jets with rapidity |y|<1, measured by the CMS experiment at s=7TeV [27]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 17.

Fig. 17

Distributions of F(z) for 25<pTjet<40GeV (upper) and 400<pTjet<500GeV (lower) for jets with pseudorapidity |ηjet|<1.2, measured by the ATLAS experiment at s=7TeV [28]. The predictions of the CP5 and CP5-CR tunes are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 18.

Fig. 18

Number of charged particles and pT flow in the transverse region of DY events, measured by the CMS experiment at s=13TeV in bins of Z boson pT  [44]. The plots show the predictions of pythia  8 with the CP5 and CP5-CR tunes, as well as MadGraph 5_amc@nlo with the CP5 tune compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

For the plots presented in Figs. 5, 6, 7, 8, 9, 10, 11, 12, 13, 14 in Sects. 4.1 and 4.2, inelastic events (i.e. ND, SD, DD, and CD) are simulated with pythia 8.226 and compared with data at different centre-of-mass energies. The rest of the plots are produced with pythia 8.235. An update to the description of the elastic scattering component in pythia 8.235 led to a slight decrease in the default ND cross section. The default ND cross section in pythia 8.226, which is 55.5\,mb at s=13TeV, is lowered to 55.1\,mb in pythia 8.235. Hence, to reproduce the conditions of pythia 8.226 in pythia 8.235 or in a newer version, one should set the ND cross section manually.

Underlying-event and minimum-bias observables

MB is a generic term used to describe events collected with a loose selection process that are dominated by relatively soft particles. Although these events generally correspond to inelastic scattering, including ND and SD+DD+CD processes, these contributions may vary depending on the trigger requirements used in the experiments. For example, a sample of non-single-diffractive-enhanced (NSD-enhanced) events is selected by suppressing the SD contribution at the trigger level.

The UE observables measured by the CMS experiment at s=13TeV [17], namely Nch density and the average pTsum in the transMIN and transMAX regions are well described by all tunes in the plateau region as shown in Fig. 5. The region up to 5 GeV of pTmax is highly sensitive to diffractive contributions [30]. There is a lack of measurements in this region where the tunes, in general, do not perform well. Although the optimisation of these components is beyond the scope of this study, we have extended the fit range to 2–3GeV as long as the data are well described. The rising part of the spectrum excluding the region up to 5GeV of the Nch density distributions is similarly described by all tunes, whereas in the pTsum density distributions the predictions of CP5 differ slightly from the predictions of the CR tunes. These show that the CP5 tune has a harder pT spectrum at low pTmax values. Through tuning the Nch and average pTsum density in the transMIN and transMAX regions, a satisfactory agreement is obtained for the same observables in the transDIFF region as well. Figure 6 shows the pseudorapidity distribution of charged hadrons in inelastic pp collisions measured by the CMS experiment at s=13TeV [22]. This observable is sensitive to the softer part of the MPI spectrum and well described by all tunes.

A crucial test for the performance of UE tunes, and of the CR simulation in particular, is the description of the average pT of the charged particles as a function of Nch. Comparisons of the mean average pT to the measurements by the ATLAS Collaboration at s=13TeV in the transMAX and transMIN regions [18] are displayed in Fig. 7. The tune CP5 describes the central values of the data perfectly for Nch>7, whereas the CR tunes show an almost constant discrepancy of 5–10% because of the harder pT spectrum predicted by the tune CP5 for low-pT particles. All CR tunes show a reasonable agreement with the data, confirming the accuracy of the parameters obtained for the new CR models. The improvement in the tuned CR models and their success in describing the data is seen by comparing Fig. 5 with Fig. 3, and Fig. 6 with Fig. 4. In these figures, CP5 tune predictions are also shown for easier comparison of CR tunes predictions with CP5.

In Fig. 8, charged-particle and pTsum densities measured by the CMS experiment at s=7TeV [19] in the transMIN and transMAX regions, as functions of pTmax, are compared with predictions from the tunes CP5 and CP5-CR. The data are reasonably well described for pTmax>5GeV.

In Fig. 9, charged particle and pTsum densities in the transverse region, as functions of pTmax, and the average pT in the transverse region as functions of pTmax and of the Nch, measured by the ATLAS experiment at s=7TeV [20], are compared with the predictions from the tunes CP5 and CP5-CR. The central values of the average pT in bins of the leading charged particle pT and of the Nch are consistent with the data points within 10%. A similar level of agreement as observed at 13TeV is achieved by the new tunes at 7TeV.

The performance of the new tunes is also checked at 7TeV using inclusive measurements of charged-particle pseudorapidity distributions. In Fig. 10, the CMS measurements for dNch/dη at 7TeV  [31] with at least one charged particle in |η|<2.4 are compared with predictions from the tunes CP5 and CP5-CR. The CP5 and CP5-CR1 have similar predictions, while CP5-CR2 predicts about 4% less charged particles than the first two tunes in all η bins of the measurement. Although all tunes provide a reasonable description of dNch/dη with deviations up to 10%, the data and MC simulation show different trends for |η|>1.2, where the trend for the data is not described well by the tunes. In the more central region, i.e. |η|<1.2, the shape of the predictions agrees well with the data but there is a difference in normalisation. For example, CP5 and CP5-CR1 predict 3–4% and CP5-CR2 predicts about 7% fewer charged particles in all bins for |η|<1.2 compared with the data.

In Fig. 11, charged-particle and pTsum densities measured as functions of pTmax at s=1.96TeV by the CDF experiment [21] in the transMIN and transMAX regions are compared with predictions from the tunes CP5 and CP5-CR, respectively. All predictions reproduce the UE observables within 10% at s=1.96, 7, and 13TeV.

We compare the new CMS tunes also with MB and UE data measured at forward pseudorapidities. The energy density, dE/dη, measured in MB events and in NSD events by the CMS experiment at s=13TeV, is shown in Fig. 12. The data are well described by CP5-CR2 within uncertainties and for all measured |η| bins. The predictions of CP5 and CP5-CR1 overestimate the data in 4.2<|η|<4.9.

The pseudorapidity of charged particles, dNch/dη, in the ranges |η|<2.2 and 5.3<|η|<6.4 measured by the CMS and TOTEM experiments at s=8TeV [32] is presented in Fig. 13. The events are required to have at least one charged particle in 5.3<η<6.5 or -6.5<η<-5.3 with pT>0. All tunes describe the data within the uncertainties. Additionally, Fig. 13 shows the pseudorapidity of charged particles, dNch/dη, in 5.3<|η|<6.4 in events with at least one charged particle with pT>40MeV, measured by the TOTEM experiment at s=7TeV [33]. Both CP5 and CP5-CR1 describe the data within the uncertainties, whereas CP5-CR2 underestimates the data by 15%.

Particle multiplicities

Figure 14 shows the strange particle production for Λ baryons and KS0 mesons as a function of rapidity (y) measured by the CMS experiment [16] in NSD events at s=7TeV. The rapidity is defined as y=12lnE+pLE-pL, where E is the particle energy and pL is the particle momentum along the anticlockwise-beam direction. It is shown in Ref. [14] that the new CR models might be beneficial for describing the ratios of strange particle multiplicities, for example Λ/ KS0 in pp collisions. We observe that all CP5 tunes, regardless of the CR model, describe particle production for KS0 mesons as a function of rapidity very well. However, they underestimate particle production for Λ versus rapidity by about 30%. Therefore, the ratio Λ/ KS0 is not perfectly described but this could be improved by different hadronisation models [35, 36]. Including these observables, as well as the recent measurements of baryon production from the ALICE and LHCb experiments [37, 38], could be beneficial in future tune derivations. This is discussed in Appendix C.

The multiplicities of identified particles are also investigated in simulated MB events (ND+SD+DD+CD). Figure 15 shows the ratio of proton over pion production, as a function of particle pT  [39]. All the tunes predict a similar trend, showing that the new CR models do not lead to a significant improvement in the description of the ratio of proton to pion production. However, it is known that this observable is strongly correlated with event particle multiplicity [3941] and not only CR, since also hadronisation and MPI play a key role in describing the ratios of particle yields.

Jet substructure observables

The number of charged particles contained in jets is an important observable that makes it possible to distinguish quark-initiated jets from gluon-initiated jets. The average number of charged hadrons with pT>500 MeV inside the jets measured by the CMS experiment as a function of the jet pT is shown in Fig. 16 [27]. The predictions of the CR tunes are comparable, and produce roughly 5% fewer charged particles than the CP5 tune. All predictions show a reasonable description of the data.

Figure 17 presents the distributions of F(z)=(1/Njet)(dNch/dz), where z is the longitudinal momentum fraction, and Nch is the charged-particle multiplicity in the jet, measured by the ATLAS experiment at s=7TeV [28]. The F(z) parameter is related to the fragmentation function and is presented for pTjet=25--40 GeV and pTjet=400--500 GeV. The CR tunes describe low-pTjet data better than CP5, and their predictions reasonably agree with the high-pTjet data, except for the last bin. The high-pTjet data are well described by the CP5 tune within the uncertainties, and its central values agree better with the predictions of the CP5 tune than with those of the CP5-CR tunes.

Drell–Yan events

Drell–Yan (DY) events [42, 43] with the Z boson decaying to μ+μ- were generated with pythia  8 and compared with CMS data at s=13TeV. Figure 18 shows the Nch and pT flow as a function of the Z boson pT (in the invariant μ+μ- mass window of 81–101GeV) in the region transverse to the boson momentum [44], which is expected to be dominated by the UE.

The CP5 tunes predict up to 15% too many charged particles at low Z boson pT, where additional effects, such as the intrinsic transverse momentum of the interacting partons (i.e. primordial kT) are expected to play a role. Higher-order corrections, as implemented in MadGraph 5_amc@nlo v2.4.2 [45] with FxFx merging [46], are necessary to describe the total pT flow. The impact of the different CR models is negligible in DY events.

Top quark observables

Jet substructure in tt¯ events

A study of the UE in tt¯ events [8] also estimated the effects of the CR on the top quark decay products by investigating the differences between predictions using pythia  8 with the ERD off and on options. In Ref.  [8], in addition to the QCD-inspired and gluon-move models, predictions of the rope hadronisation model [47, 48] are also compared with the data. In the rope hadronisation model, overlapping strings are treated to act coherently as a “rope”. The interactions between overlapping strings are described by an interaction potential inspired by the phenomenology of superconductors [35, 36, 4752]. The ERD off and on options allow the CR to take place before or after the top quark decay, respectively. In particular, the ERD option allows the top quark decay products to be colour reconnected with the partons from MPI systems. Ref. [8] showed that these different models and options produce similar predictions for UE observables in tt¯ events. However, some jet-shape distributions in tt¯ events display a more significant effect [53], e.g. in the number of charged particles in jets. In the following, we investigate how the pythia  8 CR tunes describe the CMS tt¯ jet substructure data [53]. In the CMS measurement, jets reconstructed using the anti-kT algorithm [54] with a distance parameter of R=0.4 as implemented in FASTJET 3.1 [55] are used. Jets with pT>30GeV within |η|<2 are selected. Jet pairs (j1 and j2) are required to be far from each other in η-ϕ space, ΔR(j1,j2)=(ηj1-ηj2)2-(ϕj1-ϕj2)2>0.8. Jet substructure observables are calculated from jet constituents with pT>1GeV, e.g. in the plateau region of high track finding efficiency and low misidentification rate. Here we focus on two variables, (i) λ00(N), which is the number of charged particles with pT>1GeV in the jet, and (ii) the separation between two groomed subjets, ΔRg, that are shown in Fig. 19 for gluon jets and inclusive jets, respectively. A “groomed jet” refers to a jet with soft and wide-angle radiation removed by a dedicated grooming algorithm [56, 57].

Fig. 19.

Fig. 19

Distributions of the particle multiplicity in gluon jets (upper) and the angle ΔRg between two groomed subjets in inclusive jets (lower) measured by the CMS experiment in tt¯ events at s=13TeV [53]. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

The compatibility of data and MC predictions is evaluated using a measure defined as χ2=ΔTC-1Δ, where Δ is the difference vector between measured and predicted values, and C is the total covariance matrix of the measurement. Since the measured distribution is normalised to unity, its covariance matrix is singular, i.e. not invertible. To render C invertible, the vector entry and matrix row/column corresponding to one measured bin need to be discarded; we choose to remove the last bin. The results are displayed in Table 4 for all jets inclusively as well as for each jet flavour separately. We observe that none of the tunes describe the λ00(N) data well for all jet flavours. As concluded in Ref. [53], flavour-dependent improvements in the nonperturbative physics modelling may be required for a better description of the data. The angle between the groomed subjets, on the other hand, is infrared and collinear safe and can be described very well by an increase in the αSFSR(mZ), which corresponds to a decrease in the FSR renormalisation scale μRFSR. Table 4 shows the results obtained by varying μRFSR by factors of 0.5 and 2.

Table 4.

The χ2 values and the numbers of degrees of freedom (Ndof) for the comparison of tt¯ data with the predictions of the different pythia  8 tunes, for the distributions of the charged-particle multiplicity λ00, the angle between the groomed subjets ΔRg at s = 13TeV  [53], and the pull angle measured in the ATLAS analysis of the colour flow at 8TeV  [58]. The FSR up and down entries denote variations of the renormalisation scale in the αSFSR(mZ) by factors of 0.5 and 2, respectively

Charged-particle multiplicity λ00 Angle between groomed subjets ΔRg Pull angle ϕ(j1,j2)
χ2 Ndof χ2 Ndof χ2 Ndof
Tune Incl. Bottom Light Gluon Incl. Bottom Light Gluon
CP5 18.4 26.6 30.7 11.8 8 28.2 18.3 10.6 8.1 10 4.7 3
CP5 ERD 19.6 28.7 32.2 12.2 8 26.9 15.0 10.7 8.7 10 2.4 3
CP5 FSR up 28.4 43.7 33.0 14.6 8 13.3 4.2 5.8 5.7 10 5.9 3
CP5 FSR down 15.0 19.7 44.0 11.6 8 59.6 39.2 33.1 22.6 10 4.1 3
CP5-CR1 14.3 28.4 29.5 4.1 8 34.6 13.4 24.4 23.6 10 3.9 3
CP5-CR1 ERD 11.7 24.4 27.8 3.8 8 32.7 13.4 21.1 27.0 10 1.4 3
CP5-CR2 14.1 23.8 38.3 8.1 8 34.3 22.3 21.3 11.7 10 5.2 3
CP5-CR2 ERD 11.0 16.9 38.6 7.1 8 35.3 24.8 16.1 13.1 10 9.3 3

Pull angle in tt¯ events

Figure 20 displays the normalised tt¯ differential cross section for the jet pull angle [59] defined using the jets originating from the decay of a W boson in tt¯ events, as measured by the ATLAS experiment [58]. The observable is shown for the case where only the charged constituents of the jet are used in the calculation. The data are compared with predictions from POWHEG v2 [60]+pythia  8 using the CP5 tunes or the corresponding CR tunes. The χ2 values are calculated as described in Sect. 4.5.1 and are shown in the last column of Table 4. The pull angle is particularly sensitive to the setting of the ERD option. With ERD turned off, the decay products of the W boson in tt¯ events are not included in CR, and the predictions using the tunes with the various CR models are similar to each other. With ERD enabled, CR now modifies the pull angle between the two jets, which is observed in Fig. 20. The predictions of each tune also show significant changes when ERD is enabled. For both the nominal and CP5-CR1 (QCD-inspired) tunes, the prediction with ERD improves the description of the data, and the difference between the predictions with or without ERD is larger for the CP5-CR1-based tune. We observe the opposite for the CP5-CR2-based (gluon-move) tunes, for which the choice without ERD is preferable. This picture might be different if the flip mechanism had been added in the tuning of the gluon-move model. The move step in the gluon-move model is more restrictive because it allows only gluons to move between the string end-points. The inclusion of the flip mechanism would also allow the string end-points to be mixed with each other and, therefore, could further reduce the total string length in an event. However, as indicated earlier, the effect of the flip mechanism on diffractive events is not well understood and, therefore, this mechanism is not used in this paper.

Fig. 20.

Fig. 20

Normalised tt¯ differential cross section for the pull angle between jets from the W boson in top quark decays, calculated from the charged constituents of the jets, measured by the ATLAS experiment using s=8TeV data [58] to investigate colour flow. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Overall, the QCD-inspired model with ERD provides the best description of the jet pull angle. The differences between the predictions using the different tunes observed here indicate that the inclusion of observables, such as the jet pull angle and other jet substructure observables, could be beneficial in future tune derivations.

Uncertainty in the top quark mass due to colour reconnection

The top quark mass has been measured with high precision using the 7, 8, and 13TeV  tt¯ data at the LHC  [10, 6173]. The most precise value of mt=172.44±0.13(stat)±0.47(syst) GeV was measured by the CMS Collaboration combining 7 and 8TeV data [67]. To further improve the precision of mt measurements, a complete analysis of the systematic uncertainties in the measurement is crucial. One of the dominant systematic uncertainties is due to the modelling of CR in top quark decays [67]. The procedure for estimating this uncertainty used for the LHC Run 1 (years 2009–2013) analyses at s=7 and 8TeV was based on a comparison of two values of mt, calculated by using predictions with the same UE tune with and without CR effects. In Ref. [67], this is done using the tune “Perugia 2011” with and without CR effects included. The “Perugia 2011” tunes family is the updated version of the “Perugia (Tevatron)” tunes family and also takes into account lessons learned from LHC MB and UE data at 0.9 and 7TeV  [74]. The new CMS tunes, presented in Sect. 2, which use different CR models, can be used to give a better evaluation of the CR uncertainty. In particular, the uncertainty is now calculated by comparing results for mt values obtained from different realistic CR models, such as CP5, CP5-CR1, and CP5-CR2.

Additionally, one can also estimate the effects of the CR on the top quark decay products by investigating the differences between predictions using pythia  8 with the option ERD off and on, which was done for the UE observables [8].

A determination of mt using a kinematic reconstruction of the decay products in semileptonic tt¯ events at s=13TeV is reported in Ref. [10]. In these events, one of the W bosons from the top quark decays into a muon or electron and a neutrino, and the other into a quark–antiquark pair. In this analysis, mt and the jet energy scale factor were determined simultaneously through a joint-likelihood fit to the selected events. The results with the QCD-inspired and gluon-move models were also compared. The pythia  8 CUETP8M2T4 [75] UE tune was used, and the parameters of the CR models were tuned to UE and MB data at s=13TeV [10]. They found that the gluon-move model results in a 0.31GeV shift from the mt value obtained with the default simulation. This shift, which is larger than the shifts caused by the other CR models, is assumed to be the uncertainty due to the modelling of CR in the measured mt. It is much larger than the shift, 0.01GeV, due to the CR modelling in the Run 1 measurement [67]. This is the largest source of uncertainty in the measured mt, where the total uncertainty is 0.62GeV  [10]. Similar studies using single top quark final states are reported in Refs. [71, 76].

We compare the mt and W boson mass values obtained with different tune configurations based on our new tunes in Table 5. Top quark candidates are constructed by a Rivet routine in a sample of simulated semileptonic tt¯ events. Events must contain exactly one lepton with pT>30GeV and |η|<2.1. Leptons are “dressed” with the surrounding photons within a cone of ΔR=0.1 and are required to yield an invariant mass window of 5GeV centred at 80.4GeV, when combined with a neutrino in the event. The events must also contain at least four jets, reconstructed with the anti-kT algorithm, with pT>30GeV within |η|<2.4. At least two of the jets are required to originate from the fragmentation of bottom quarks, and at least two other jets, referred to as light-quark jets, must not originate from bottom quarks. One jet originating from a bottom quark is combined with the lepton and neutrino to form a leptonically decaying top quark candidate, whereas the other jet originating from a bottom quark is combined with two other jets to form a hadronically decaying top quark candidate. The difference in the invariant mass window of the two top quark candidates is required to be less than 20GeV, and the invariant mass of the two light-quark jets is within a window of 10GeV centred at 80.4GeV. If more than one combination of jets satisfy these criteria when combined with the lepton and neutrino, then only one combination is chosen based on how similar the invariant masses of the two top quark candidates are to each other and on how close the invariant mass of the light-quark jets is to 80.4GeV. The invariant mass of the hadronically decaying top quark candidates constructed in this way for each of the different tune configurations is shown in Fig. 21. The top quark and W boson mass values are obtained from these hadronically decaying top quark candidates by fitting a Gaussian function within an 8GeV mass window around the corresponding mass peak. Table 5 also contains the differences from the nominal mt and mW values (Δmt, and ΔmW) and the difference in Δmthyb, a quantity that was introduced in Ref. [67] to incorporate both an in situ jet scale factor determined from the reconstructed mW as well as prior knowledge about the jet energy scale in a hybrid approach to extract mt. Here, Δmthyb is approximated as Δmt-0.5ΔmW. From Table 5, we observe that the largest deviation from the predictions of CP5 is CP5-CR2 ERD (0.32GeV) similar to the largest shift found in Ref. [10] using CUETP8M2T4. However, CP5-CR2 ERD is not able to describe the available colour flow data, and can therefore be excluded from the list of modelling uncertainties.

Table 5.

The top quark mass (mt) and W mass (mW) extracted by a fit to the predictions of the different pythia  8 tunes, along with the differences from the nominal mt value (Δmt), mW value (ΔmW), and Δmthyb which represents an estimation of the mt uncertainty considering the shift in mW included with a weight of 0.5. The uncertainties in the mt and mW values correspond to the uncertainty in the fitted mt and mW

Tune mt [GeV ] Δmt [GeV ] mW [GeV ] ΔmW [GeV ] Δmthyb [GeV ]
CP5 171.93±0.02 79.76±0.02
CP5 ERD 172.18±0.03 0.25 80.15±0.02 0.40 0.05
CP5-CR1 171.97±0.02 0.04 79.74±0.02 -0.02 0.05
CP5-CR1 ERD 172.01±0.03 0.08 79.98±0.02 0.23 -0.04
CP5-CR2 171.91±0.02 -0.02 79.85±0.02 0.10 -0.07
CP5-CR2 ERD 172.32±0.03 0.39 79.90±0.02 0.14 0.32

Fig. 21.

Fig. 21

The invariant mass of hadronically decaying top quark candidates for different tune configurations. The coloured band and vertical bars represent the statistical uncertainty in the predictions

Summary and conclusion

New sets of parameters for two of the colour reconnection (CR) models implemented in the pythia  8 event generator, QCD-inspired and gluon-move, are obtained, based on the default CMS pythia  8 tune CP5. Measurements sensitive to underlying-event (UE) contributions performed at hadron-colliders at s=1.96, 7, and 13TeV are used to constrain the parameters for the CR and for the multiple-parton interactions simultaneously. Various measurements at 1.96, 7, 8, and 13TeV are used to evaluate the performance of the new tunes. The central values predicted by the new CR tunes for the UE and minimum-bias events describe the data significantly better than the CR models with their default parameters before tuning. The predictions of the new tunes achieve a reasonable agreement in many UE observables, including the ones measured at forward pseudorapidities. However, the models after tuning do not generally perform better than the CP5 tune for the observables presented in this study. Although the new CR tunes presented in this work are not intended to improve the description of the measurements of strange particle multiplicities for Λ baryons and KS0 mesons, we test the new tunes against them. We find that the new CR models, when tuned using only measurements that are sensitive to the UE, do not provide a better description of the distribution of strange particle production as a function of rapidity for Λ baryons. However, we observe that all CP5 tunes, irrespective of the CR model, describe particle production for KS0 as a function of rapidity well. Including these observables in the fits, along with the latest measurements of baryon/meson production, could be beneficial for future tune derivations.

The predictions of the new tunes for jet shapes and colour flow measurements done with top quark pair events are also compared with data. All tunes give similar predictions, but none of the tunes describe the jet shape distributions well. Some differences are also observed with respect to the colour flow data, which is particularly sensitive to the early resonance decay option in the CR models. The differences between the predictions using the different tunes observed here indicate that the inclusion of observables, such as the jet pull angle and other jet substructure observables, could be beneficial in tuning studies. A study of the uncertainty in the top quark mass measurement due to CR effects is also presented. The new CR tunes will play a role in the evaluation of systematic uncertainties associated with the modelling of colour reconnection.

Acknowledgements

We congratulate our colleagues in the CERN accelerator departments for the excellent performance of the LHC and thank the technical and administrative staffs at CERN and at other CMS institutes for their contributions to the success of the CMS effort. In addition, we gratefully acknowledge the computing centres and personnel of the Worldwide LHC Computing Grid and other centres for delivering so effectively the computing infrastructure essential to our analyses. Finally, we acknowledge the enduring support for the construction and operation of the LHC, the CMS detector, and the supporting computing infrastructure provided by the following funding agencies: BMBWF and FWF (Austria); FNRS and FWO (Belgium); CNPq, CAPES, FAPERJ, FAPERGS, and FAPESP (Brazil); MES and BNSF (Bulgaria); CERN; CAS, MoST, and NSFC (China); MINCIENCIAS (Colombia); MSES and CSF (Croatia); RIF (Cyprus); SENESCYT (Ecuador); MoER, ERC PUT and ERDF (Estonia); Academy of Finland, MEC, and HIP (Finland); CEA and CNRS/IN2P3 (France); BMBF, DFG, and HGF (Germany); GSRI (Greece); NKFIH (Hungary); DAE and DST (India); IPM (Iran); SFI (Ireland); INFN (Italy); MSIP and NRF (Republic of Korea); MES (Latvia); LAS (Lithuania); MOE and UM (Malaysia); BUAP, CINVESTAV, CONACYT, LNS, SEP, and UASLP-FAI (Mexico); MOS (Montenegro); MBIE (New Zealand); PAEC (Pakistan); MES and NSC (Poland); FCT (Portugal); MESTD (Serbia); MCIN/AEI and PCTI (Spain); MOSTR (Sri Lanka); Swiss Funding Agencies (Switzerland); MST (Taipei); MHESI and NSTDA (Thailand); TUBITAK and TENMAK (Turkey); NASU (Ukraine); STFC (United Kingdom); DOE and NSF (USA). Individuals have received support from the Marie-Curie programme and the European Research Council and Horizon 2020 Grant, contract Nos. 675440, 724704, 752730, 758316, 765710, 824093, 884104, and COST Action CA16108 (European Union); the Leventis Foundation; the Alfred P. Sloan Foundation; the Alexander von Humboldt Foundation; the Belgian Federal Science Policy Office; the Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture (FRIA-Belgium); the Agentschap voor Innovatie door Wetenschap en Technologie (IWT-Belgium); the F.R.S.-FNRS and FWO (Belgium) under the “Excellence of Science – EOS” – be.h project n. 30820817; the Beijing Municipal Science & Technology Commission, No. Z191100007219010; the Ministry of Education, Youth and Sports (MEYS) of the Czech Republic; the Hellenic Foundation for Research and Innovation (HFRI), Project Number 2288 (Greece); the Deutsche Forschungsgemeinschaft (DFG), under Germany’s Excellence Strategy – EXC 2121 “Quantum Universe” – 390833306, and under project number 400140256 – GRK2497; the Hungarian Academy of Sciences, the New National Excellence Program – ÚNKP, the NKFIH research grants K 124845, K 124850, K 128713, K 128786, K 129058, K 131991, K 133046, K 138136, K 143460, K 143477, 2020-2.2.1-ED-2021-00181, and TKP2021-NKTA-64 (Hungary); the Council of Science and Industrial Research, India; the Latvian Council of Science; the Ministry of Education and Science, project no. 2022/WK/14, and the National Science Center, contracts Opus 2021/41/B/ST2/01369 and 2021/43/B/ST2/01552 (Poland); the Fundação para a Ciência e a Tecnologia, grant CEECIND/01334/2018 (Portugal); the National Priorities Research Program by Qatar National Research Fund; MCIN/AEI/10.13039/501100011033, ERDF “a way of making Europe”, and the Programa Estatal de Fomento de la Investigación Científica y Técnica de Excelencia María de Maeztu, grant MDM-2017-0765 and Programa Severo Ochoa del Principado de Asturias (Spain); the Chulalongkorn Academic into Its 2nd Century Project Advancement Project, and the National Science, Research and Innovation Fund via the Program Management Unit for Human Resources & Institutional Development, Research and Innovation, grant B05F650021 (Thailand); the Kavli Foundation; the Nvidia Corporation; the SuperMicro Corporation; the Welch Foundation, contract C-1845; and the Weston Havens Foundation (USA).

Colour reconnection tunes with a leading-order PDF set

The list of input Rivet routines used as inputs for the fits, as well as the centre-of-mass energy values, the η ranges, the names of the distributions, the x-axis ranges, and the R values of the distributions are displayed in Table 6 for the tunes CP1-CR1 and CP1-CR2, and in Table 7 for the tunes CP2-CR1 and CP2-CR2. The baseline tunes CP1 and CP2 use the NNPDF31_lo_as_0130 [26] PDF set, with an αS(mZ) value of 0.130 for ISR, FSR, and MPI, and the MPI-based CR model. The parameters of the tunes are documented in Ref. [13] and displayed in Tables 8 and 9. The parameters obtained from the CP1-CR1, CP1-CR2, CP2-CR1, and CP2-CR2 fits, as well as the value of the goodness of the fits are displayed in Tables 8 and 9. The predictions of these new CR tunes for particle multiplicities are shown in Figs. 22, and 23. The CR tunes based on CP1 and CP2 describe MB and UE data as well as the CR tunes based on CP5, except for the different trend observed with CP1-CR1 in the particle multiplicity distributions.

Table 6.

List of input Rivet routines, centre-of-mass energy values, η ranges, names of distributions, fit ranges, and relative importance of the distributions used in the fits to derive the tunes CP1-CR1 and CP1-CR2

Rivet routine s [TeV ] |η| Distribution CP1-CR1 Fit range [GeV ] R CP1-CR2 Fit range [GeV ] R
CMS_2015_I1384119 13 <2.0 Nch versus η 1 1
CMS_2015_PAS_FSQ_15_007 13 <2.0 TransMIN pTsum 3–36 1 4–36 0.20
TransMAX pTsum 3–36 1 4–36 0.20
TransMIN Nch 3–36 1 4–36 0.20
TransMAX Nch 3–36 1 4–36 0.20
CMS_2012_PAS_FSQ_12_020 7 <0.8 TransMAX Nch 3–20 1 3–20 0.10
TransMIN Nch 3–20 1 3–20 0.10
TransMAX pTsum 3–20 1 3–20 0.10
TransMIN pTsum 3–20 1 3–20 0.10
CDF_2015_I1388868 2 <0.8 TransMIN Nch 2–15 1 2–15 0.10
TransMAX Nch 2–15 1 2–15 0.10
TransMIN pTsum 2–15 1 2–15 0.10
TransMAX pTsum 2–15 1 2–15 0.10

Table 7.

List of input Rivet routines, centre-of-mass energy values, η ranges, names of distributions, fit ranges, and relative importance of the distributions used in the fits to derive the tunes CP2-CR1 and CP2-CR2

Rivet routine s [TeV ] |η| Distribution CP2-CR1 Fit range [GeV ] R CP2-CR2 Fit range [GeV ] R
CMS_2015_I1384119 13 <2.0 Nch versus η 0.03 0.05
CMS_2015_PAS_FSQ_15_007 13 <2.0 TransMIN pTsum 5–24 1 5–24 1
TransMAX pTsum 5–24 0.17 5–24 0.25
TransMIN Nch 5–24 1 5–24 1
TransMAX Nch 5–24 0.17 5–24 0.25
CMS_2012_PAS_FSQ_12_020 7 <0.8 TransMAX Nch 5–20 0.07 5–20 0.25
TransMIN Nch 5–20 1 5–20 1
TransMAX pTsum 5–20 0.07 5–20 0.25
TransMIN pTsum 5–20 1 5–20 1
CDF_2015_I1388868 2 <0.8 TransMIN Nch 2–15 0.03 2–15 0.05
TransMAX Nch 2–15 0.03 2–15 0.05
TransMIN pTsum 2–15 0.03 2–15 0.05
TransMAX pTsum 2–15 0.03 2–15 0.05

Table 8.

The parameters obtained in the fits of the CP1-CR1 and CP1-CR2 tunes, compared with the ones of the tune CP1. The upper part of the table displays the fixed input parameters of the tune, while the lower part shows the fitted tune parameters. The number of degrees of freedom (Ndof) and the goodness of fit divided by the number of degrees of freedom are also shown

pythia  8 parameter CP1 [13] CP1-CR1 CP1-CR2
PDF set NNPDF3.1 LO NNPDF3.1 LO NNPDF3.1 LO
αS(mZ) 0.130 0.130 0.130
SpaceShower:rapidityOrder Off Off Off
MultipartonInteractions:ecmRef [GeV ] 7000 7000 7000
αSISR(mZ) value/order 0.1365/LO 0.1365/LO 0.1365/LO
αSFSR(mZ) value/order 0.1365/LO 0.1365/LO 0.1365/LO
αSMPI(mZ) value/order 0.130/LO 0.130/LO 0.130/LO
αSME(mZ) value/order 0.130/LO 0.130/LO 0.130/LO
StringZ:aLund 0.38
StringZ:bLund 0.64
StringFlav:probQQtoQ 0.078
StringFlav:probStoUD 0.2
SigmaTotal:zeroAXB Off Off Off
BeamRemnants:remnantMode 1
MultipartonInteractions:bProfile 2 2 2
ColourReconnection:mode 1 2
MultipartonInteractions:pT0Ref [GeV ] 2.400 1.984 2.385
MultipartonInteractions:ecmPow 0.154 0.113 0.165
MultipartonInteractions:coreRadius 0.544 0.746 0.587
MultipartonInteractions:coreFraction 0.684 0.569 0.533
ColourReconnection:range 2.633
ColourReconnection:junctionCorrection 8.382
ColourReconnection:timeDilationPar 31.070
ColourReconnection:m0 1.845
ColourReconnection:m2lambda 2.769
ColourReconnection:fracGluon 0.979
Ndof 183 157 150
χ2/Ndof 0.89 0.73 0.20

Table 9.

The parameters obtained in the fits of the CP2-CR1 and CP2-CR2 tunes, compared with the ones of the tune CP2. The upper part of the table displays the fixed input parameters of the tune, while the lower part shows the fitted tune parameters. The number of degrees of freedom (Ndof) and the goodness of fit divided by the number of degrees of freedom are also shown

pythia  8 parameter CP2 [13] CP2-CR1 CP2-CR2
PDF set NNPDF3.1 LO NNPDF3.1 LO NNPDF3.1 LO
αS(mZ) 0.130 0.130 0.130
SpaceShower:rapidityOrder Off Off Off
MultipartonInteractions:ecmRef [GeV ] 7000 7000 7000
αSISR(mZ) value/order 0.130/LO 0.130/LO 0.130/LO
αSFSR(mZ) value/order 0.130/LO 0.130/LO 0.130/LO
αSMPI(mZ) value/order 0.130/LO 0.130/LO 0.130/LO
αSME(mZ) value/order 0.130/LO 0.130/LO 0.130/LO
StringZ:aLund 0.38
StringZ:bLund 0.64
StringFlav:probQQtoQ 0.078
StringFlav:probStoUD 0.2
SigmaTotal:zeroAXB Off Off Off
BeamRemnants:remnantMode 1
MultipartonInteractions:bProfile 2 2 2
ColourReconnection:mode 1 2
MultipartonInteractions:pT0Ref [GeV ] 2.306 2.154 2.287
MultipartonInteractions:ecmPow 0.139 0.119 0.146
MultipartonInteractions:coreRadius 0.376 0.538 0.514
MultipartonInteractions:coreFraction 0.327 0.599 0.525
ColourReconnection:range 2.323
ColourReconnection:junctionCorrection 0.761
ColourReconnection:timeDilationPar 13.080
ColourReconnection:m0 1.546
ColourReconnection:m2lambda 6.186
ColourReconnection:fracGluon 0.978
Ndof 183 117 118
χ2/Ndof 0.54 0.21 0.22

Fig. 22.

Fig. 22

The strange particle production, Λ baryons (left) and KS0 mesons (right), as a function of rapidity, measured by the CMS experiment at s=7TeV [16]. The predictions of the CP1 and CP1-CR tunes (upper) and CP2 and CP2-CR tunes (lower) are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Fig. 23.

Fig. 23

Ratios of particle yields, p/π, as a function of transverse momentum in MB events, measured by the CMS experiment at s=13TeV [39]. The predictions of the CP1 and CP1-CR tunes (left) and CP2 and CP2-CR tunes (right) are compared with data. The coloured band and error bars on the data points represent the total experimental uncertainty in the data

Parameter ranges and uncertainties in the tunes

The parameter ranges are chosen such that the sampled MC space does not destroy the definition of a particular observable in the fits. In Fig. 24, some sample histograms showing the range of variation available on the observable histograms are given for CP5-CR1. The results are similar for other observables used in the fits as well as for CP5-CR2.

Fig. 24.

Fig. 24

Sample histograms showing the range of variation available on the observable histograms are given for CP5-CR1

The CP5-CR1 and CP5-CR2 tunes were developed to evaluate the uncertainty in CP5 that results from different color reconnection models. The uncertainties in the parameters for these tunes were estimated using eigentunes provided by Professor. Eigentunes represent variations of the tuned parameters in the parameter space along the maximally independent directions. The magnitude of the variation corresponds to a change in the χ2 (Δχ2) equal to the χ2 of the fit. The choice of Δχ2, which is recommended by the Professor Collaboration, is based on empirical grounds since modifying it in equation Eq. (4) does not yield a statistically meaningful variation. Such a change, Δχ2=χ2, is considered reasonable for reflecting the combined statistical and systematic uncertainty in the model parameters, and results in variations similar in magnitude to the uncertainties in the fitted data points. However, this approach may result in uncertainties that do not fully encompass the data in every bin. If the uncertainties in the fitted data points are uncorrelated, their magnitudes will depend on the bin widths. For the data used in the fit, the uncertainties are mostly correlated between bins. However, for UE observables with high pTmax (pTmax10GeV) statistical uncertainties, which are uncorrelated between bins, dominate. This creates some dependence of the eigentunes on the bin widths of the data used in the fit, and leads to uncertainties in the tunes that are much larger and more asymmetric than those on the data points when all eigentunes are added in quadrature.

The number of eigentunes is equal to twice the number of free parameters used in the fit. For the QCD-inspired and gluon-move models, there are 14 and 12 eigentunes, respectively. However, using all 12 or 14 eigentunes to calculate the tune uncertainty for a given observable is computationally inefficient. Therefore, the “up” and “down” tune settings are calculated by comparing the positive and negative differences between each eigentune and the central prediction of the nominal tune for each bin of the observable. The upper and lower bounds of the uncertainty in each bin are defined by adding the positive differences in quadrature and taking the square root, and similarly for the negative differences. These “up” and “down” variations are then fit using the same procedure as in Sect. 3 to obtain new parameter sets that can be used to estimate the uncertainties in the nominal tune.

The predictions of the CP5-CR1 and CP5-CR2 tunes are compared with observables at 13TeV in Figs. 25, 26, 27, 28. The shaded bands in these figures correspond to the envelope of the predictions of the eigentunes of each tune. The parameters of the “up” and “down” tunes for CP5-CR1 and CP5-CR2 are given in Tables 10 and 11, respectively.

Fig. 25.

Fig. 25

The pseudorapidity of charged hadrons, dNch/dη, measured by the CMS experiment at s=13TeV [22]. The prediction of the CP5-CR1 tune is compared with data. The coloured band represents the tune uncertainties

Fig. 26.

Fig. 26

The charged-particle (left) and pTsum densities (right) in the transMIN (upper) and transMAX (lower) regions as functions of the pT of the leading charged particle, pTmax, measured by the CMS experiment at s=13TeV [17]. The predictions of the tunes CP5-CR1 are compared with data. The coloured band represents the tune uncertainties

Fig. 27.

Fig. 27

The pseudorapidity of charged hadrons, dNch/dη, measured by the CMS experiment at s=13TeV [22]. The prediction of the CP5-CR2 tune is compared with data. The coloured band represents the tune uncertainties

Fig. 28.

Fig. 28

The charged-particle (left) and pTsum densities (right) in the transMIN (upper) and transMAX (lower) regions as functions of the pT of the leading charged particle, pTmax, measured by the CMS experiment at s=13TeV [17]. The predictions of the tunes CP5-CR2 are compared with data. The coloured band represents the tune uncertainties

Table 10.

Parameters of the “up” and “down” variations of the CP5-CR1 tune

CP5-CR1
Down Up
MultipartonInteractions:pT0Ref [GeV ] 1.568 1.328
MultipartonInteractions:ecmPow 0.011 0.045
MultipartonInteractions:coreRadius 0.466 0.643
MultipartonInteractions:coreFraction 0.516 0.579
ColourReconnection:junctionCorrection 0.219 0.261
ColourReconnection:timeDilationPar 9.328 11.95
ColourReconnection:m0 1.786 1.529

Table 11.

Parameters of the “up” and “down” variations of the CP5-CR2 tune

CP5-CR2
Down Up
MultipartonInteractions:pT0Ref [GeV ] 1.565 1.361
MultipartonInteractions:ecmPow 0.057 0.075
MultipartonInteractions:coreRadius 0.576 0.760
MultipartonInteractions:coreFraction 0.704 0.623
ColourReconnection:m2lambda 3.202 2.837
ColourReconnection:fracGluon 0.979 0.988

The ColourReconnection:junctionCorrection parameter

The QCD-inspired model implemented in pythia  8 allows for the creation of string junctions when three color lines meet at a single point. The presence of these junctions can affect the number of particles produced in a collision and result in the production of additional gluons and quark–antiquark pairs. The junctionCorrection parameter in pythia  8 controls the strength of this effect and can impact various observables, including the charged particle pseudorapidity distribution.

The model predictions, with their default parameter settings in pythia 8.226 and CP5, are given in Fig. 29 for the dNch/dη distribution measured by the CMS experiment at 13TeV  [22], and in Fig. 30 for Nch and pTsum densities measured by CMS at 13TeV  [17] in the transMIN and transMAX regions. The predictions for CP5-“QCD-inspired” were obtained by replacing the MPI-based CR model in CP5 with the QCD-inspired model, where the default value of the junctionCorrection parameter is 1.2. The other predictions presented in the figures were obtained by setting the junctionCorrection parameter to 4.0 and to 0.05, respectively. These values were chosen arbitrarily to test how the prediction changes when a relatively high or low value is set for the junctionCorrection parameter. These comparisons demonstrate the sensitivity of the junctionCorrection parameter to these observables. According to Ref. [14], the junctionCorrection parameter is most sensitive to the baryon/meson ratio in pp collisions. The sensitivity of the junctionCorrection parameter to the production of Λ baryons and KS0 mesons, measured by the CMS experiment at s=7TeV [16], is shown in Fig. 31.

Fig. 29.

Fig. 29

The pseudorapidity of charged hadrons, dNch/dη, measured in |η|<2 by the CMS experiment at s=13TeV [23]. The red line shows the prediction of CP5-“QCD-inspired,” where the default value of the ColourReconnection:junctionCorrection parameter is 1.2. The predictions shown with the blue and green lines use 4.0 and 0.05 for the ColourReconnection:junctionCorrection parameter, respectively. These comparisons demonstrate the sensitivity of the ColourReconnection:junctionCorrection parameter to this observable

Fig. 30.

Fig. 30

The charged-particle (left) and pTsum densities (right) in the transMIN (upper) and transMAX (lower) regions as functions of the pT of the leading charged particle, pTmax, measured by the CMS experiment at s=13TeV [17]. The red line shows the prediction of CP5-“QCD-inspired,” where the default value of the ColourReconnection:junctionCorrection parameter is 1.2. The predictions shown with the blue and green lines use 4.0 and 0.05 for the ColourReconnection:junctionCorrection parameter, respectively. These comparisons demonstrate the sensitivity of the ColourReconnection:junctionCorrection parameter to these observables

Fig. 31.

Fig. 31

The strange particle production, Λ baryons (left) and KS0 mesons (right), as a function of rapidity, measured by the CMS experiment at s=7TeV [16]. The red line shows the prediction of CP5-“QCD-inspired,” where the default value of the ColourReconnection:junctionCorrection parameter is 1.2. The predictions shown with the blue and green lines use 4.0 and 0.05 for the ColourReconnection:junctionCorrection parameter, respectively. These comparisons demonstrate the sensitivity of the ColourReconnection:junctionCorrection parameter to these observables

We also derived a new version of CP5-CR1 by including the rapidity distributions of Λ baryons and KS0 mesons, as well as some recent baryon and meson measurements from ALICE and LHCb experiments [37, 38]. The new tune, named CP5-CR2-v2, resulted in a significant improvement in the description of the Λ rapidity distribution and reasonable agreement with the data for Λ/KS0, but it was not able to reproduce the dNch/dη at 13 TeV. The values of the parameters obtained in the fits of the CP5-CR1-v2 are presented in Table 12. The remaining parameters of pythia  8 are kept the same as in the CP5 tune.

Table 12.

The values of the parameters obtained in the fits of the CP5-CR1-v2

pythia  8 parameterCP5-CR1-v2
MultipartonInteractions:pT0Ref 1.260
MultipartonInteractions:ecmPow 0.042
MultipartonInteractions:coreRadius 0.750
MultipartonInteractions:coreFraction 0.567
ColourReconnection:m0 1.888
ColourReconnection:junctionCorrection 1.427
ColourReconnection:timeDilationPar 4.990

Data Availability

This manuscript has no associated data or the data will not be deposited. [Authors’ comment: Release and preservation of data used by the CMS Collaboration as the basis for publications is guided by the CMS policy as stated in https://cms-docdb.cern.ch/cgi-bin/PublicDocDB/RetrieveFile?docid=6032 &filename=CMSDataPolicyV1.2.pdf &version=2 CMS data preservation, re-use and open access policy.]

Declarations

Conflict of interest

The authors declare that they have no conflict of interest.

Footnotes

W. De Boer, P. Baillon, G. R. Snow: The author deceased.

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Data Availability Statement

This manuscript has no associated data or the data will not be deposited. [Authors’ comment: Release and preservation of data used by the CMS Collaboration as the basis for publications is guided by the CMS policy as stated in https://cms-docdb.cern.ch/cgi-bin/PublicDocDB/RetrieveFile?docid=6032 &filename=CMSDataPolicyV1.2.pdf &version=2 CMS data preservation, re-use and open access policy.]


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