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. 2016 Mar 17;76:155. doi: 10.1140/epjc/s10052-016-3988-x

Event generator tunes obtained from underlying event and multiparton scattering measurements

V Khachatryan 1, A M Sirunyan 1, A Tumasyan 1, W Adam 2, E Asilar 2, T Bergauer 2, J Brandstetter 2, E Brondolin 2, M Dragicevic 2, J Erö 2, M Friedl 2, R Frühwirth 2, V M Ghete 2, C Hartl 2, N Hörmann 2, J Hrubec 2, M Jeitler 2, V Knünz 2, A König 2, M Krammer 2, I Krätschmer 2, D Liko 2, T Matsushita 2, I Mikulec 2, D Rabady 2, B Rahbaran 2, H Rohringer 2, J Schieck 1, R Schöfbeck 2, J Strauss 2, W Treberer-Treberspurg 2, W Waltenberger 2, C-E Wulz 2, V Mossolov 3, N Shumeiko 3, J Suarez Gonzalez 3, S Alderweireldt 4, T Cornelis 4, E A De Wolf 4, X Janssen 4, A Knutsson 4, J Lauwers 4, S Luyckx 4, M Van De Klundert 4, H Van Haevermaet 4, P Van Mechelen 4, N Van Remortel 4, A Van Spilbeeck 4, S Abu Zeid 5, F Blekman 5, J D’Hondt 5, N Daci 5, I De Bruyn 5, K Deroover 5, N Heracleous 5, J Keaveney 5, S Lowette 5, L Moreels 5, A Olbrechts 5, Q Python 5, D Strom 5, S Tavernier 5, W Van Doninck 5, P Van Mulders 5, G P Van Onsem 5, I Van Parijs 5, P Barria 6, H Brun 6, C Caillol 6, B Clerbaux 6, G De Lentdecker 6, G Fasanella 6, L Favart 6, A Grebenyuk 6, G Karapostoli 6, T Lenzi 6, A Léonard 6, T Maerschalk 6, A Marinov 6, L Perniè 6, A Randle-conde 6, T Seva 6, C Vander Velde 6, R Yonamine 6, P Vanlaer 6, R Yonamine 6, F Zenoni 6, F Zhang 6, V Adler 7, K Beernaert 7, L Benucci 7, A Cimmino 7, S Crucy 7, D Dobur 7, A Fagot 7, G Garcia 7, M Gul 7, J Mccartin 7, A A Ocampo Rios 7, D Poyraz 7, D Ryckbosch 7, S Salva 7, M Sigamani 7, M Tytgat 7, W Van Driessche 7, E Yazgan 7, N Zaganidis 7, S Basegmez 8, C Beluffi 8, O Bondu 8, S Brochet 8, G Bruno 8, A Caudron 8, L Ceard 8, G G Da Silveira 8, C Delaere 8, D Favart 8, L Forthomme 8, A Giammanco 8, J Hollar 8, A Jafari 8, P Jez 8, M Komm 8, V Lemaitre 8, A Mertens 8, M Musich 8, C Nuttens 8, L Perrini 8, A Pin 8, K Piotrzkowski 8, A Popov 8, L Quertenmont 8, M Selvaggi 8, M Vidal Marono 8, N Beliy 9, G H Hammad 9, W L Aldá Júnior 10, F L Alves 10, G A Alves 10, L Brito 10, M Correa Martins Junior 10, M Hamer 10, C Hensel 10, A Moraes 10, M E Pol 10, P Rebello Teles 10, E Belchior Batista Das Chagas 11, W Carvalho 11, J Chinellato 11, A Custódio 11, E M Da Costa 11, D De Jesus Damiao 11, C De Oliveira Martins 11, S Fonseca De Souza 11, L M Huertas Guativa 11, H Malbouisson 11, D Matos Figueiredo 11, C Mora Herrera 11, L Mundim 11, H Nogima 11, W L Prado Da Silva 11, A Santoro 11, A Sznajder 11, E J Tonelli Manganote 11, A Vilela Pereira 11, S Ahuja 12, C A Bernardes 12, A De Souza Santos 12, S Dogra 12, T R Fernandez Perez Tomei 12, E M Gregores 12, P G Mercadante 12, C S Moon 12, S F Novaes 12, Sandra S Padula 12, D Romero Abad 12, J C Ruiz Vargas 12, A Aleksandrov 13, R Hadjiiska 13, P Iaydjiev 13, M Rodozov 13, S Stoykova 13, G Sultanov 13, M Vutova 13, A Dimitrov 14, I Glushkov 14, L Litov 14, B Pavlov 14, P Petkov 14, M Ahmad 14, J G Bian 15, G M Chen 15, H S Chen 15, M Chen 15, T Cheng 15, R Du 15, C H Jiang 15, R Plestina 15, F Romeo 15, S M Shaheen 15, A Spiezia 15, J Tao 15, C Wang 15, Z Wang 15, H Zhang 15, C Asawatangtrakuldee 16, Y Ban 16, Q Li 16, S Liu 16, Y Mao 16, S J Qian 16, D Wang 16, Z Xu 16, C Avila 17, A Cabrera 17, L F Chaparro Sierra 17, C Florez 17, J P Gomez 17, B Gomez Moreno 17, J C Sanabria 17, N Godinovic 18, D Lelas 18, I Puljak 18, P M Ribeiro Cipriano 18, Z Antunovic 19, M Kovac 19, V Brigljevic 20, K Kadija 20, J Luetic 20, S Micanovic 20, L Sudic 20, A Attikis 21, G Mavromanolakis 21, J Mousa 21, C Nicolaou 21, F Ptochos 21, P A Razis 21, H Rykaczewski 21, M Bodlak 22, M Finger 22, M Finger Jr 22, A A Abdelalim 23, A Awad 23, A Mahrous 23, Y Mohammed 23, A Radi 23, B Calpas 24, M Kadastik 24, M Murumaa 24, M Raidal 24, A Tiko 24, C Veelken 24, P Eerola 25, J Pekkanen 25, M Voutilainen 25, J Härkönen 26, V Karimäki 26, R Kinnunen 26, T Lampén 26, K Lassila-Perini 26, S Lehti 26, T Lindén 26, P Luukka 26, T Mäenpää 26, T Peltola 26, E Tuominen 26, J Tuominiemi 26, E Tuovinen 26, L Wendland 26, J Talvitie 27, T Tuuva 27, M Besancon 28, F Couderc 28, M Dejardin 28, D Denegri 28, B Fabbro 28, J L Faure 28, C Favaro 28, F Ferri 28, S Ganjour 28, A Givernaud 28, P Gras 28, G Hamel de Monchenault 28, P Jarry 28, E Locci 28, M Machet 28, J Malcles 28, J Rander 28, A Rosowsky 28, M Titov 28, A Zghiche 28, I Antropov 29, S Baffioni 29, F Beaudette 29, P Busson 29, L Cadamuro 29, E Chapon 29, C Charlot 29, T Dahms 29, O Davignon 29, N Filipovic 29, R Granier de Cassagnac 29, M Jo 29, S Lisniak 29, L Mastrolorenzo 29, P Miné 29, I N Naranjo 29, M Nguyen 29, C Ochando 29, G Ortona 29, P Paganini 29, P Pigard 29, S Regnard 29, R Salerno 29, J B Sauvan 29, Y Sirois 29, T Strebler 30, Y Yilmaz 29, A Zabi 29, J-L Agram 30, J Andrea 30, A Aubin 30, D Bloch 30, J-M Brom 30, M Buttignol 30, E C Chabert 30, N Chanon 30, C Collard 30, E Conte 30, X Coubez 30, J-C Fontaine 30, D Gelé 30, U Goerlach 30, C Goetzmann 30, A-C Le Bihan 30, J A Merlin 30, K Skovpen 30, P Van Hove 30, S Gadrat 31, S Beauceron 32, C Bernet 32, G Boudoul 32, E Bouvier 32, 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L Sonnenschein 36, D Teyssier 36, S Thüer 36, V Cherepanov 37, Y Erdogan 37, G Flügge 37, H Geenen 37, M Geisler 37, F Hoehle 37, B Kargoll 37, T Kress 37, Y Kuessel 37, A Künsken 37, J Lingemann 37, A Nehrkorn 37, A Nowack 37, I M Nugent 37, C Pistone 37, O Pooth 37, A Stahl 37, M Aldaya Martin 37, I Asin 38, N Bartosik 38, O Behnke 38, U Behrens 38, A J Bell 38, K Borras 38, A Burgmeier 38, A Campbell 38, S Choudhury 38, F Costanza 38, C Diez Pardos 38, G Dolinska 38, S Dooling 38, T Dorland 38, G Eckerlin 38, D Eckstein 38, T Eichhorn 38, G Flucke 38, E Gallo 38, J Garay Garcia 38, A Geiser 38, A Gizhko 38, P Gunnellini 38, J Hauk 38, M Hempel 38, H Jung 38, A Kalogeropoulos 38, O Karacheban 38, M Kasemann 38, P Katsas 38, J Kieseler 38, C Kleinwort 38, I Korol 38, W Lange 38, J Leonard 38, K Lipka 38, A Lobanov 38, W Lohmann 38, R Mankel 38, I Marfin 38, I-A Melzer-Pellmann 38, A B Meyer 38, G Mittag 38, J Mnich 38, A Mussgiller 38, S Naumann-Emme 38, A Nayak 38, E Ntomari 38, H Perrey 38, D Pitzl 38, R Placakyte 38, A Raspereza 38, B Roland 38, M Ö Sahin 38, P Saxena 38, T Schoerner-Sadenius 38, M Schröder 38, C Seitz 38, S Spannagel 38, K D Trippkewitz 38, R Walsh 38, C Wissing 38, V Blobel 39, M Centis Vignali 39, A R Draeger 39, J Erfle 39, E Garutti 39, K Goebel 39, D Gonzalez 39, M Görner 39, J Haller 39, M Hoffmann 39, R S Höing 39, A Junkes 39, R Klanner 39, R Kogler 39, N Kovalchuk 39, T Lapsien 39, T Lenz 39, I Marchesini 39, D Marconi 39, M Meyer 39, D Nowatschin 39, J Ott 39, F Pantaleo 39, T Peiffer 39, A Perieanu 39, N Pietsch 39, J Poehlsen 39, D Rathjens 39, C Sander 39, C Scharf 39, H Schettler 39, P Schleper 39, E Schlieckau 39, A Schmidt 39, J Schwandt 39, V Sola 39, H Stadie 39, G Steinbrück 39, H Tholen 39, D Troendle 39, E Usai 39, L Vanelderen 39, A Vanhoefer 39, B Vormwald 39, C Barth 40, C Baus 40, J Berger 40, C Böser 40, E Butz 40, T Chwalek 40, F Colombo 40, W De Boer 40, A Descroix 40, A Dierlamm 40, S Fink 40, F Frensch 40, R Friese 40, M Giffels 40, A Gilbert 40, D Haitz 40, F Hartmann 40, S M Heindl 40, U Husemann 40, I Katkov 40, A Kornmayer 40, P Lobelle Pardo 40, B Maier 40, H Mildner 40, M U Mozer 40, T Müller 40, Th Müller 40, M Plagge 40, G Quast 40, K Rabbertz 40, S Röcker 40, F Roscher 40, G Sieber 40, H J Simonis 40, F M Stober 40, R Ulrich 40, J Wagner-Kuhr 40, S Wayand 40, M Weber 40, T Weiler 40, S Williamson 40, C Wöhrmann 40, R Wolf 40, G Anagnostou 41, G Daskalakis 41, T Geralis 41, V A Giakoumopoulou 41, A Kyriakis 41, D Loukas 41, A Psallidas 41, I Topsis-Giotis 41, A Agapitos 42, S Kesisoglou 42, A Panagiotou 42, N Saoulidou 42, E Tziaferi 42, I Evangelou 43, G Flouris 43, C Foudas 43, P Kokkas 43, N Loukas 43, N Manthos 43, I Papadopoulos 43, E Paradas 43, J Strologas 43, G Bencze 44, C Hajdu 44, A Hazi 44, P Hidas 44, D Horvath 44, F Sikler 44, V Veszpremi 44, G Vesztergombi 44, A J Zsigmond 44, N Beni 45, S Czellar 45, J Karancsi 45, J Molnar 45, Z Szillasi 45, M Bartók 45, A Makovec 46, P Raics 46, Z L Trocsanyi 46, B Ujvari 46, P Mal 47, K Mandal 47, D K Sahoo 47, N Sahoo 47, S K Swain 47, S Bansal 47, S B Beri 48, V Bhatnagar 48, R Chawla 48, R Gupta 48, U Bhawandeep 48, A K Kalsi 48, A Kaur 48, M Kaur 48, R Kumar 48, A Mehta 48, M Mittal 48, J B Singh 48, G Walia 48, Ashok Kumar 49, A Bhardwaj 49, B C Choudhary 49, R B Garg 49, A Kumar 49, S Malhotra 49, M Naimuddin 49, N Nishu 49, K Ranjan 49, R Sharma 49, V Sharma 49, S Bhattacharya 50, K Chatterjee 50, S Dey 50, S Dutta 50, Sa Jain 50, N Majumdar 50, A Modak 50, K Mondal 50, S Mukherjee 50, S Mukhopadhyay 50, A Roy 50, D Roy 50, S Roy Chowdhury 50, S Sarkar 50, M Sharan 50, A Abdulsalam 51, R Chudasama 51, D Dutta 51, V Jha 51, V Kumar 51, A K Mohanty 51, L M Pant 51, P Shukla 51, A Topkar 51, T Aziz 52, S Banerjee 52, S Bhowmik 52, R M Chatterjee 52, R K Dewanjee 52, S Dugad 52, S Ganguly 52, S Ghosh 52, M Guchait 52, A Gurtu 52, G Kole 52, S Kumar 52, B Mahakud 52, M Maity 52, G Majumder 52, K Mazumdar 52, S Mitra 52, G B Mohanty 52, B Parida 52, T Sarkar 52, N Sur 52, B Sutar 52, N Wickramage 52, S Chauhan 52, S Dube 52, A Kapoor 52, K Kothekar 52, S Sharma 53, H Bakhshiansohi 54, H Behnamian 54, S M Etesami 54, A Fahim 54, R Goldouzian 54, M Khakzad 54, M Mohammadi Najafabadi 54, M Naseri 54, S Paktinat Mehdiabadi 54, F Rezaei Hosseinabadi 54, B Safarzadeh 54, M Zeinali 54, M Felcini 55, M Grunewald 55, M Abbrescia 56, C Calabria 56, C Caputo 56, A Colaleo 56, D Creanza 56, L Cristella 56, N De Filippis 56, M De Palma 56, L Fiore 56, G Iaselli 56, G Maggi 56, G Miniello 56, M Maggi 56, S My 56, S Nuzzo 56, A Pompili 56, G Pugliese 56, R Radogna 56, A Ranieri 56, G Selvaggi 56, L Silvestris 56, R Venditti 56, P Verwilligen 56, G Abbiendi 57, C Battilana 57, A C Benvenuti 57, D Bonacorsi 57, S Braibant-Giacomelli 57, L Brigliadori 57, R Campanini 57, P Capiluppi 57, A Castro 57, F R Cavallo 57, S S Chhibra 57, G Codispoti 57, M Cuffiani 57, G M Dallavalle 57, F Fabbri 57, A Fanfani 57, D Fasanella 57, P Giacomelli 57, C Grandi 57, L Guiducci 57, S Marcellini 57, G Masetti 57, A Montanari 57, F L Navarria 57, A Perrotta 57, A M Rossi 57, F Primavera 57, T Rovelli 57, G P Siroli 57, N Tosi 57, R Travaglini 57, G Cappello 58, M Chiorboli 58, S Costa 58, A Di Mattia 58, F Giordano 58, R Potenza 58, A Tricomi 58, C Tuve 58, G Barbagli 59, V Ciulli 59, C Civinini 59, R D’Alessandro 59, E Focardi 59, S Gonzi 59, V Gori 59, P Lenzi 59, M Meschini 59, S Paoletti 59, G Sguazzoni 59, A Tropiano 59, L Viliani 59, L Benussi 60, S Bianco 60, F Fabbri 60, D Piccolo 60, F Primavera 60, V Calvelli 61, F Ferro 61, M Lo Vetere 61, M R Monge 61, E Robutti 61, S Tosi 61, L Brianza 62, M E Dinardo 62, S Fiorendi 62, S Gennai 62, R Gerosa 62, A Ghezzi 62, P Govoni 62, S Malvezzi 62, R A Manzoni 62, B Marzocchi 62, D Menasce 62, L Moroni 62, M Paganoni 62, D Pedrini 62, S Ragazzi 62, N Redaelli 62, T Tabarelli de Fatis 62, S Buontempo 63, N Cavallo 63, S Di Guida 63, M Esposito 63, F Fabozzi 63, A O M Iorio 63, G Lanza 63, L Lista 63, S Meola 63, M Merola 63, P Paolucci 63, C Sciacca 63, F Thyssen 63, P Azzi 64, N Bacchetta 64, L Benato 64, D Bisello 64, A Boletti 64, A Branca 64, R Carlin 64, P Checchia 64, M Dall’Osso 64, T Dorigo 64, U Dosselli 64, S Fantinel 64, F Fanzago 64, F Gasparini 64, U Gasparini 64, A Gozzelino 64, K Kanishchev 64, S Lacaprara 64, M Margoni 64, A T Meneguzzo 64, J Pazzini 64, N Pozzobon 64, P Ronchese 64, F Simonetto 64, E Torassa 64, M Tosi 64, M Zanetti 64, P Zotto 64, A Zucchetta 64, A Braghieri 64, A Magnani 64, P Montagna 64, S P Ratti 65, V Re 65, C Riccardi 65, P Salvini 65, I Vai 65, P Vitulo 65, L Alunni Solestizi 66, G M Bilei 66, D Ciangottini 66, L Fanò 66, P Lariccia 66, G Mantovani 66, M Menichelli 66, A Saha 66, A Santocchia 66, K Androsov 67, P Azzurri 67, G Bagliesi 67, J Bernardini 67, T Boccali 67, R Castaldi 67, M A Ciocci 67, R Dell’Orso 67, S Donato 67, G Fedi 67, F Fiori 67, L Foà 67, A Giassi 67, M T Grippo 67, F Ligabue 67, T Lomtadze 67, L Martini 67, A Messineo 67, F Palla 67, A Rizzi 67, A Savoy-Navarro 67, A T Serban 67, P Spagnolo 67, R Tenchini 67, G Tonelli 67, A Venturi 67, P G Verdini 67, L Barone 68, F Cavallari 68, G D’imperio 68, D Del Re 68, M Diemoz 68, S Gelli 68, C Jorda 68, E Longo 68, F Margaroli 68, P Meridiani 68, G Organtini 68, R Paramatti 68, F Preiato 68, S Rahatlou 68, C Rovelli 68, F Santanastasio 68, P Traczyk 68, N Amapane 69, R Arcidiacono 69, S Argiro 69, M Arneodo 69, R Bellan 69, C Biino 69, N Cartiglia 69, M Costa 69, R Covarelli 69, A Degano 69, N Demaria 69, L Finco 69, B Kiani 69, C Mariotti 69, S Maselli 69, E Migliore 69, V Monaco 69, E Monteil 69, M M Obertino 69, L Pacher 69, N Pastrone 69, M Pelliccioni 69, G L Pinna Angioni 69, F Ravera 69, A Potenza 69, A Romero 69, M Ruspa 69, R Sacchi 69, A Solano 69, A Staiano 69, S Belforte 70, V Candelise 70, M Casarsa 70, F Cossutti 70, G Della Ricca 70, B Gobbo 70, C La Licata 70, M Marone 70, A Schizzi 70, A Zanetti 70, T A Kropivnitskaya 71, S K Nam 71, D H Kim 72, G N Kim 72, M S Kim 72, M S Kim 72, D J Kong 72, S Lee 72, Y D Oh 72, A Sakharov 72, D C Son 72, J A Brochero Cifuentes 73, H Kim 73, T J Kim 73, S Song 74, S Choi 75, Y Go 75, D Gyun 75, B Hong 75, H Kim 75, Y Kim 75, B Lee 75, K Lee 75, K S Lee 75, S Lee 75, S Lee 75, S K Park 75, Y Roh 75, H D Yoo 76, M Choi 77, H Kim 77, J H Kim 77, J S H Lee 77, I C Park 77, G Ryu 77, M S Ryu 77, Y Choi 78, J Goh 78, D Kim 78, E Kwon 78, J Lee 78, I Yu 78, V Dudenas 78, A Juodagalvis 79, J Vaitkus 79, I Ahmed 79, Z A Ibrahim 80, J R Komaragiri 80, M A B Md Ali 80, F Mohamad Idris 80, W A T Wan Abdullah 80, M N Yusli 80, W A T Wan Abdullah 80, E Casimiro Linares 80, H Castilla-Valdez 81, E De La Cruz-Burelo 81, I Heredia-De La Cruz 81, A Hernandez-Almada 81, R Lopez-Fernandez 81, A Sanchez-Hernandez 81, S Carrillo Moreno 82, F Vazquez Valencia 82, I Pedraza 83, H A Salazar Ibarguen 83, A Morelos Pineda 84, D Krofcheck 85, P H Butler 86, A Ahmad 87, 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166, A Ledovskoy 166, H Li 166, C Lin 166, C Neu 166, T Sinthuprasith 166, X Sun 166, Y Wang 166, E Wolfe 166, J Wood 166, F Xia 166, C Clarke 167, R Harr 167, P E Karchin 167, C Kottachchi Kankanamge Don 167, P Lamichhane 167, J Sturdy 167, D A Belknap 167, D Carlsmith 168, M Cepeda 168, S Dasu 168, L Dodd 168, S Duric 168, B Gomber 168, M Grothe 168, R Hall-Wilton 168, M Herndon 168, A Hervé 168, P Klabbers 168, A Lanaro 168, A Levine 168, K Long 168, R Loveless 168, A Mohapatra 168, I Ojalvo 168, T Perry 168, G A Pierro 168, G Polese 168, T Ruggles 168, T Sarangi 168, A Savin 168, A Sharma 168, N Smith 168, W H Smith 168, D Taylor 168, N Woods 168; CMS Collaboration169
PMCID: PMC4946872  PMID: 27471433

Abstract

New sets of parameters (“tunes”) for the underlying-event (UE) modelling of the pythia8, pythia6 and herwig++ Monte Carlo event generators are constructed using different parton distribution functions. Combined fits to CMS UE proton–proton (pp) data at s=7TeV and to UE proton–antiproton (pp¯) data from the CDF experiment at lower s, are used to study the UE models and constrain their parameters, providing thereby improved predictions for proton–proton collisions at 13TeV. In addition, it is investigated whether the values of the parameters obtained from fits to UE observables are consistent with the values determined from fitting observables sensitive to double-parton scattering processes. Finally, comparisons are presented of the UE tunes to “minimum bias” (MB) events, multijet, and Drell–Yan (qq¯Z/γ lepton-antilepton+jets) observables at 7 and 8TeV, as well as predictions for MB and UE observables at 13TeV.

Introduction

Monte Carlo (MC) event generators of hadron–hadron collisions based on perturbative quantum chromodynamics (QCD) contain several components. The “hard-scattering” part of the event consists of particles resulting from the hadronization of the two partons (jets) produced in the hardest scattering, and in their associated hard initial- and final-state radiation (ISR and FSR). The underlying event (UE) consists of particles from the hadronization of beam-beam remnants (BBR), of multiple-parton interactions (MPI), and their associated ISR and FSR. The BBR include hadrons from the fragmentation of spectator partons that do not exchange any appreciable transverse momentum (pT) in the collision. The MPI are additional 2-to-2 parton-parton scatterings that occur within the same hadron–hadron collision, and are softer in transverse momentum (pT3GeV) than the hard scattering.

The perturbative 2-to-2 parton-parton differential cross section diverges like 1/p^T4, where p^T is the transverse momentum of the outgoing partons in the parton-parton center-of-mass (c.m.) frame. Usually, QCD MC models such as pythia  [15] regulate this divergence by including a smooth phenomenological cutoff pT0 as follows:

1/p^T41/(p^T2+pT02)2. 1

This formula approaches the perturbative result for large scales and is finite as p^T0. The divergence of the strong coupling αs at low p^T is also regulated through Eq. (1). The primary hard 2-to-2 parton-parton scattering process and the MPI are regulated in the same way through a single pT0 parameter. However, this cutoff is expected to have a dependence on the center-of-mass energy of the hadron–hadron collision s. In the pythia MC event generator this energy dependence is parametrized with a power-law function with exponent ϵ:

pT0(s)=pT0ref(s/s0)ϵ, 2

where s0 is a given reference energy and pT0ref is the value of pT0 at s0. At a given s, the amount of MPI depends on pT0, the parton distribution functions (PDF), and the overlap of the matter distributions (or centrality) of the two colliding hadrons. Smaller values of pT0 provide more MPI due to a larger MPI cross section. Table 1 shows the parameters in pythia6 [1] and pythia8 [5] that, together with the selected PDF, determine the energy dependence of MPI. Recently, in herwig++ [6, 7] the same formula has been adopted to provide an energy dependence to their MPI cutoff, which is also shown in Table 1. The QCD MC generators have other parameters that can be adjusted to control the modelling of the properties of the events, and a specified set of such parameters adjusted to fit certain prescribed aspects of the data is referred to as a “tune” [810].

Table 1.

Parameters in pythia6 [1], pythia8 [5], and herwig++ [6, 7] MC event generators that, together with some chosen PDF, determine the energy dependence of MPI

Parameter pythia6 pythia8 herwig++
MPI cutoff, pT0ref, at s=s0 PARP(82) MultipartonInteractions:pT0Ref MPIHandler:pTmin0
Reference energy, s0 PARP(89) MultipartonInteractions:ecmRef MPIHandler:ReferenceScale
Exponent of s dependence, ϵ PARP(90) MultipartonInteractions:ecmPow MPIHandler:Power

In addition to hard-scattering processes, other processes contribute to the inelastic cross section in hadron–hadron collisions: single-diffraction dissociation (SD), double-diffraction dissociation (DD), and central-diffraction (CD). In SD and DD events, one or both beam particles are excited into high-mass color-singlet states (i.e.  into some resonant N), which then decay. The SD and DD processes correspond to color-singlet exchanges between the beam hadrons, while CD corresponds to double color-singlet exchange with a diffractive system produced centrally. For non-diffractive processes (ND), color is exchanged, the outgoing remnants are no longer color singlets, and this separation of color generates a multitude of quark–antiquark pairs that are created via vacuum polarization. The sum of all components except SD corresponds to non single-diffraction (NSD) processes.

Minimum bias (MB) is a generic term that refers to events selected by requiring minimal activity within the detector. This selection accepts a large fraction of the overall inelastic cross section. Studies of the UE are often based on MB data, but it should be noted that the dominant particle production mechanisms in MB collisions and in the UE are not exactly the same. On the one hand, the UE is studied in collisions in which a hard 2-to-2 parton-parton scattering has occurred, by analyzing the hadronic activity in different regions of the event relative to the back-to-back azimuthal structure of the hardest particles emitted [11]. On the other hand, MB collisions are often softer and include diffractive interactions that, in the case of pythia, are modelled via a Regge-based approach [12].

The MPI are usually much softer than primary hard scatters, however, occasionally two hard 2-to-2 parton scatters can take place within the same hadron–hadron collision. This is referred to as double-parton scattering (DPS) [1316], and is typically described in terms of an effective cross section parameter, σeff, defined as:

σAB=σAσBσeff, 3

where σA and σB are the inclusive cross sections for individual hard scattering processes of generic type A and B, respectively, and σAB is the cross section for producing both scatters in the same hadron–hadron collision. If A and B are indistinguishable, as in four-jet production, a statistical factor of 1 / 2 must be inserted on the right-hand side of Eq. (3). Furthermore, σeff is assumed to be independent of A and B. However, σeff is not a directly observed quantity, but can be calculated from the overlap function of the two transverse profile distributions of the colliding hadrons, as implemented in any given MPI model.

The UE tunes have impact in both soft and hard particle production in a given pp collision. First, about half of the particles produced in a MB collision originate from the hadronization of partons scattered in MPI, and have their differential cross sections in pT regulated via Eq. (1), using the same pT0 cutoff used to tame the hardest 2-to-2 parton-parton scattering in the event. The tuning of the cross-section regularization affects therefore all (soft and hard) parton-parton scatterings and provides a prediction for the behavior of the ND cross section. Second, the UE tunes parametrize the distribution in the transverse overlap of the colliding protons and thereby the probability of two hard parton-parton scatters that is then used to estimate DPS-sensitive observables.

In this paper, we study the s dependence of the UE using recent CDF proton–antiproton data from the Fermilab Tevatron at 0.3, 0.9, and 1.96TeV [11], together with CMS pp data from the CERN LHC at s=7TeV [17]. The 0.3 and 0.9TeV data are from the “Tevatron energy scan” performed just before the Tevatron was shut down. Using the rivet (version 1.9.0) and professor (version 1.3.3) frameworks [18, 19], we construct: (i) new pythia8 (version 8.185) UE tunes using several PDF sets (CTEQ6L1 [20], HERAPDF1.5LO [21], and NNPDF2.3LO [22, 23]), (ii) new pythia6 (version 6.327) UE tunes (using CTEQ6L1 and HERAPDF1.5LO), and (iii) a new herwig++ (version 2.7.0) UE tune for CTEQ6L1. The rivet software is a tool for producing predictions of physics quantities obtained from MC event generators. It is used for generating sets of MC predictions with a different choice of parameters related to the UE simulation. The predictions are then included in the professor framework, which parametrizes the generator response and returns the set of tuned parameters that best fits the input measurements.

In addition, we construct several new CMS “DPS tunes” and investigate whether the values of the UE parameters determined from fitting the UE observables in a hard-scattering process are consistent with the values determined from fitting DPS-sensitive observables. The professor software also offers the possibility of extracting “eigentunes”, which provide an estimate of the uncertainties in the fitted parameters. The eigentunes consist of a collection of additional tunes, obtained through the covariance matrix of the data-theory fitting procedure, to determine independent directions in parameter space that provide a specific modification in the goodness of the fit, χ2 (Sect. 2). All of the CMS UE and DPS tunes are provided with eigentunes. In Sect. 4, predictions using the CMS UE tunes are compared to other UE measurements not used in determining the tunes, and we examine how well Drell–Yan, MB, and multijet observables can be predicted using the UE tunes. In Sect. 5, predictions of the new tunes are shown for UE observables at 13TeV, together with a comparison to the first MB distribution measured. Section 6 has a brief summary and conclusions. The appendices contain additional comparisons between the pythia6 and herwig++ UE tunes and the data, information about the tune uncertainties, and predictions for some MB and DPS observables at 13TeV.

The CMS UE tunes

Previous UE studies have used the charged-particle jet with largest pT [24, 25] or a Z boson [11, 26] as the leading (i.e. highest pT) objects in the event. The CDF and CMS data, used for the tunes, select the charged particle with largest pT in the event (pTmax) as the “leading object”, and use just the charged particles with pT>0.5GeV and |η|<0.8 to characterize the UE.

On an event-by-event basis, the leading object is used to define regions of pseudorapidity-azimuth (η-ϕ) space. The “toward” region relative to this direction, as indicated in Fig. 1, is defined by |Δϕ|<π/3 and |η|<0.8, and the “away” region by |Δϕ|>2π/3 and |η|<0.8. The charged-particle and the scalar-pT sum densities in the transverse region are calculated as the sum of the contribution in the two regions: “Transverse-1” (π/3<Δϕ<2π/3, |η|<0.8) and “Transverse-2” (π/3<-Δϕ<2π/3, |η|<0.8), divided by the area in η-ϕ space, ΔηΔϕ=1.6×2π/3. The transverse region is further separated into the “TransMAX” and “TransMIN” regions, also shown in Fig. 1. This defines on an event-by-event basis the regions with more (TransMAX) and fewer (TransMIN) charged particles (Nch), or greater (TransMAX) or smaller (TransMIN) scalar-pT sums (pTsum). The UE particle and pT densities are constructed by dividing by the area in η-ϕ space, where the TransMAX and TransMIN regions each have an area of ΔηΔϕ=1.6×2π/6. The transverse density (also referred to as “TransAVE”) is the average of the TransMAX and the TransMIN densities. For events with hard initial- or final-state radiation, the TransMAX region often contains a third jet, but both the TransMAX and TransMIN regions receive contributions from the MPI and beam-beam remnant components. The TransMIN region is very sensitive to the MPI and beam-beam remnant components of the UE, while “TransDIF” (the difference between TransMAX and TransMIN densities) is very sensitive to ISR and FSR [27].

Fig. 1.

Fig. 1

Left Illustration of the azimuthal regions in an event defined by the Δϕ angle relative to the direction of the leading object [11]. Right Illustration of the topology of a hadron–hadron collision in which a hard parton–parton collision has occurred, and the leading object is taken to be the charged particle of largest pT in the event, pTmax

The new UE tunes are determined by fitting UE observables, and using only those parameters that are most sensitive to the UE data. Since it is not possible to tune all parameters of a MC event generator at once, the parameters that affect, for example, the parton shower, the fragmentation, and the intrinsic-parton pT are fixed to the values given by an initially established reference tune. The initial reference tunes used for pythia8 are Tune 4C [28] and the Monash Tune [29]. For pythia6, the reference tune is Tune Z2*lep [25], and for herwig++ it is Tune UE-EE-5C [30].

The PYTHIA8 UE tunes

Taking as the reference tune the set of parameters of pythia8 Tune 4C [28], we construct two new UE tunes, one using CTEQ6L1 (CUETP8S1-CTEQ6L1) and one using HERAPDF1.5LO (CUETP8S1-HERAPDF1.5LO). CUET (read as “cute”) stands for “CMS UE tune”, and P8S1 stands for pythia8 “Set 1”.

The tunes are extracted by varying the four parameters in Table 2 in fits to the TransMAX and TransMIN charged-particle and pTsum densities at three energies, for pp¯ collisions at s=0.9 and 1.96, and pp collisions at 7TeV. The measurements of TransAVE and TransDIF densities are not included in the fit, since they can be constructed from TransMAX and TransMIN. The new tunes use an exponentially-falling matter-overlap function between the two colliding protons of the form exp(−bexpPow), with b being the impact parameter of the collision. The parameters that are varied are expPow, the MPI energy-dependence parameters (Table 1) and the range, i.e. the probability, of color reconnection (CR). A small (large) value of the final-state CR parameter tends to increase (reduce) the final particle multiplicities. In pythia8, unlike in pythia6, only one parameter determines the amount of CR, which includes a pT dependence, as defined in Ref. [5].

Table 2.

The pythia8 parameters, tuning range, Tune 4C values [28], and best-fit values for CUETP8S1-CTEQ6L1 and CUETP8S1-HERAPDF1.5LO, obtained from fits to the TransMAX and TransMIN charged-particle and pTsum densities, as defined by the leading charged-particle pTmaxat s=0.9, 1.96, and 7TeV. The s=300GeV data are excluded from the fit

pythia8 Parameter Tuning range Tune 4C CUETP8S1 CUETP8S1
PDF CTEQ6L1 CTEQ6L1 HERAPDF1.5LO
MultipartonInteractions:pT0Ref [GeV] 1.0–3.0 2.085 2.101 2.000
MultipartonInteractions:ecmPow 0.0–0.4 0.19 0.211 0.250
MultipartonInteractions:expPow 0.4–10.0 2.0 1.609 1.691
ColourReconnection:range 0.0–9.0 1.5 3.313 6.096
MultipartonInteractions:ecmRef [GeV] 1800 1800a 1800a
χ2/dof 0.952 1.13

a Fixed at Tune 4C value

The generated inelastic events include ND and diffractive (DD+SD+CD) contributions, although the UE observables used to determine the tunes are sensitive to single-diffraction dissociation, central-diffraction, and double-diffraction dissociation only at very small pTmax values (e.g. pTmax<1.5GeV). The ND component dominates for pTmax values greater than 2.0GeV, since the cross section of the diffractive components rapidly decreases as a function of p^T. The fit is performed by minimizing the χ2 function:

χ2(p)=i(fi(p)-Ri)2Δi2, 4

where the sum runs over each bin i of every observable. The fi(p) functions correspond to the interpolated MC response for the simulated observables as a function of the parameter vector p, Ri is the value of the measured observable in bin i, and Δi is the total experimental uncertainty of Ri. We do not use the Tevatron data at s=300GeV, as we are unable to obtain an acceptable χ2 in a fit of the four parameters in Table 2. The χ2 per degree of freedom (dof) listed in Table 2 refers to the quantity χ2(p) in Eq. (4), divided by the number of dof in the fit. The eigentunes (Appendix A) correspond to the tunes in which the changes in the χ2 (Δχ2) of the fit relative to the best-fit value equals the χ2 value obtained in the tune, i.e. Δχ2 = χ2. For both tunes in Table 2, the fit quality is very good, with χ2/dof values very close to 1.

The contribution from CR changes in the two new tunes; it is large for the HERAPDF1.5LO and small for the CTEQ6L1 PDF. This is a result of the shape of the parton densities at small fractional momenta x, which is different for the two PDF sets. While the parameter pT0ref in Eq. (2) stays relatively constant between Tune 4C and the new tunes, the energy dependence ϵ tends to increase in the new tunes, as do the matter-overlap profile functions.

The pythia8 Monash Tune [29] combines updated fragmentation parameters with the NNPDF2.3LO PDF.

The NNPDF2.3LO PDF has a gluon distribution at small x that is different compared to CTEQ6L1 and HERAPDF1.5LO, and this affects predictions in the forward region of hadron–hadron collisions. Tunes using the NNPDF2.3LO PDF provide a more consistent description of the UE and MB observables in both the central and forward regions, than tunes using other PDF.

A new pythia8 tune CUETP8M1 (labeled with M for Monash) is constructed using the parameters of the Monash Tune and fitting the two MPI energy-dependence parameters of Table 1 to UE data at s=0.9, 1.96, and 7TeV. Varying the CR range and the exponential slope of the matter-overlap function freely in the minimization of the χ2 leads to suboptimal best-fit values. The CR range is therefore fixed to the value of the Monash Tune, and the exponential slope of the matter-overlap function expPow is set to 1.6, which is similar to the value determined in CUETP8S1-CTEQ6L1. The best-fit values of the two tuned parameters are shown in Table 3. Again, we exclude the 300GeV data, since we are unable to get a good χ2 in the fit. The parameters obtained for CUETP8M1 differ slightly from the ones of the Monash Tune. The obtained energy-dependence parameter ϵ is larger, while a very similar value is obtained for pT0ref.

Table 3.

The pythia8 parameters, tuning range, Monash values [29], and best-fit values for CUETP8M1, obtained from fits to the TransMAX and TransMIN charged-particle and pTsum densities, as defined by the leading charged-particle pTmaxat s=0.9, 1.96, and 7TeV. The s=300GeV data are excluded from the fit

pythia8 Parameter Tuning range Monash CUETP8M1
PDF NNPDF2.3LO NNPDF2.3LO
MultipartonInteractions:pT0Ref [GeV] 1.0–3.0 2.280 2.402
MultipartonInteractions:ecmPow 0.0–0.4 0.215 0.252
MultipartonInteractions:expPow 1.85 1.6a
ColourReconnection:range 1.80 1.80b
MultipartonInteractions:ecmRef [GeV] 7000 7000b
χ2/dof 1.54

a Fixed at CUETP8S1-CTEQ6L1 value

b Fixed at Monash Tune value

Figures 2, 3, 4 and 5 show the CDF data at 0.3, 0.9, and 1.96TeV, and the CMS data at 7TeV for charged-particle and pTsum densities in the TransMIN and TransMAX regions as a function of pTmax, compared to predictions obtained with the pythia8 Tune 4C and with the new CMS tunes: CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. Predictions from the new tunes cannot reproduce the s=300GeV data, but describe very well the data at the higher s=0.9, 1.96, and 7TeV. In particular, the description provided by the new tunes significantly improves relative to the old Tune 4C, which is likely due to the better choice of parameters used in the MPI energy dependence and the extraction of the CR in the retuning.

Fig. 2.

Fig. 2

CDF data at s=300GeV [11] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to pythia8 Tune 4C, CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. The ratios of MC events to data are given below each panel. The data at s=300GeV are not used in determining these tunes. The green bands in the ratios represent the total experimental uncertainties

Fig. 3.

Fig. 3

CDF data at s=900GeV [11] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to pythia8 Tune 4C, CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. The ratios of MC events to data are given below each panel. The green bands in the ratios represent the total experimental uncertainties

Fig. 4.

Fig. 4

CDF data at s=1.96TeV [11] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to pythia8 Tune 4C, CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. The ratios of MC events to data are given below each panel. The green bands in the ratios represent the total experimental uncertainties

Fig. 5.

Fig. 5

CMS data at s=7TeV [17] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to pythia8 Tune 4C, and CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. The ratios of MC events to data are given below each panel. The green bands in the ratios represent the total experimental uncertainties

The PYTHIA6 UE tunes

The pythia6 Tune Z2lep [25] uses the improved fragmentation parameters from fits to the LEP e+e- data [31], and a double-Gaussian matter profile for the colliding protons but corresponds to an outdated CMS UE tune. It was constructed by fitting the CMS charged-particle jet UE data at 0.9 and 7TeV [24] using data on the TransAVE charged-particle and pTsum densities, since data on TransMAX, TransMIN, and TransDIF were not available at that time.

Starting with Tune Z2lep parameters, two new pythia6 UE tunes are constructed, one using CTEQ6L1 (CUETP6S1-CTEQ6L1) and one using HERAPDF1.5LO (CUETP6S1-HERAPDF1.5LO), with P6S1 standing for pythia6 “Set 1”. The tunes are constructed by fitting the five parameters shown in Table 4 to the TransMAX and TransMIN charged-particle and pTsum densities at s=0.3, 0.9, 1.96, and 7TeV. In addition to varying the MPI energy-dependence parameters (Table 1), we also vary the core-matter fraction PARP(83), which parametrizes the amount of matter contained within the radius of the proton core, the CR strength PARP(78), and the CR suppression PARP(77). The PARP(78) parameter reflects the probability for a given string to retain its color history, and therefore does not change the color and other string pieces, while the PARP(77) parameter introduces a pT dependence on the CR probability [1].

Table 4.

The pythia6 parameters, tuning range, Tune Z2lep values [31], and best-fit values for CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO, obtained from fits to the TransMAX and TransMIN charged-particle and pTsum densities as defined by the pTmax of the leading charged particle at s=0.3 , 0.9, 1.96, and 7TeV

pythia6 Parameter Tuning Range Tune Z2lep CUETP6S1 CUETP6S1
PDF CTEQ6L1 CTEQ6L1 HERAPDF1.5LO
PARP(82)-MPI cutoff [GeV] 1.6–2.2 1.921 1.910 1.946
PARP(90)-exponent of s dependence 0.18–0.28 0.227 0.248 0.250
PARP(77)-CR suppression 0.25–1.15 1.016 0.665 0.667
PARP(78)-CR strength 0.2–0.8 0.538 0.545 0.537
PARP(83)-matter fraction in core 0.1–1.0 0.356 0.822 0.490
PARP(89)-reference energy [GeV] 1800 1800a 1800a
χ2/dof 0.915 1.004

a Fixed at Tune Z2lep value

Inelastic events (ND+DD+SD+CD) are generated with pythia6. The best-fit values of the five parameters are shown in Table 4. The matter-core fraction is quite different in the two new pythia6 tunes. This is due to the fact that this parameter is very sensitive to the behaviour of the PDF at small x. Predictions obtained with pythia6 Tune Z2lep , CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO are compared in Appendix B to the UE data. The new pythia6 tunes significantly improve the description of the UE data relative to pythia6 Tune Z2lep at all considered energies, due to the better choice of parameters governing the MPI energy dependence.

The HERWIG++ UE tunes

Starting with the parameters of herwig++ Tune UE-EE-5C [30], we construct a new herwig++ UE tune, CUETHppS1, where Hpp stands for herwig++. This tune is obtained by varying the four parameters shown in Table 5 in the fit to TransMAX and TransMIN charged-particle and pTsum densities at the four s=0.3, 0.9, 1.96, and 7TeV. We set the MPI cutoff pT0 and the reference energy s0 to the Tune UE-EE-5C values, and vary the MPI c.m. energy extrapolation parameter in Table 1. We also vary the inverse radius that determines the matter overlap and the range of CR. The CR model in herwig++ is defined by two parameters, one (colourDisrupt) ruling the color structure of soft interactions (pT<pT0), and one (ReconnectionProbability) giving the probability of CR without a pT dependence for color strings. We include all four center-of-mass energies, although at each energy we exclude the first two pTmax bins. These first bins, e.g. for pTmax<1.5GeV, are sensitive to single-diffraction dissociation, central-diffraction, and double-diffraction dissociation, but herwig++ contains only the ND component.

Table 5.

The herwig++ parameters, tuning range, Tune UE-EE-5C values [30], and best-fit values for CUETHppS1, obtained from a fit to the TransMAX and TransMIN charged-particle and pTsum densities as a function of the leading charged-particle pTmaxat s=0.3 , 0.9, 1.96, and 7TeV

herwig++ Parameter Tuning range UE-EE-5C CUETHppS1
PDF CTEQ6L1 CTEQ6L1
MPIHandler:Power 0.1–0.5 0.33 0.371
RemnantDecayer:colourDisrupt 0.1–0.9 0.8 0.628
MPIHandler:InvRadius [GeV2] 0.5–2.7 2.30 2.255
ColourReconnector:ReconnectionProbability 0.1–0.9 0.49 0.528
MPIHandler:pTmin0 [GeV] 3.91 3.91a
MPIHandler:ReferenceScale [GeV] 7000 7000a
χ2/dof 0.463

a Fixed at Tune UE-EE-5C value

In Table 5, the parameters of the new CUETHppS1 are listed and compared to those from Tune UE-EE-5C. The parameters of the two tunes are very similar. The χ2/dof, also indicated in Table 5, is found to be 0.46, which is smaller than the value obtained for other CMS UE tunes. This is due to the fact that the first two bins as a function of pTmax, which have much smaller statistical uncertainties than the higher-pTmax bins, are excluded from the fit because they cannot be described by any reasonable fit-values. In Appendix C, predictions obtained with herwig++ Tune UE-EE-5C and CUETHppS1 are compared to the UE data. The two tunes are both able to reproduce the UE data at all energies. With the new CUETHppS1 tune, uncertainties can be estimated using the eigentunes (Appendix A).

In conclusion, both herwig++ tunes, as well as the new CMS pythia6 UE tunes reproduce the UE data at all four s. The pythia8 UE tunes, however, do not describe well the data at s=300GeV, which may be related to the modelling of the proton–proton overlap function. The pythia6 Tune Z2lep, and the new CMS UE tunes use a double-Gaussian matter distribution, while all the pythia8 UE tunes use a single exponential matter overlap. The herwig++ tune, on the other hand, uses a matter-overlap function that is related to the Fourier transform of the electromagnetic form factor with μ2 [7] playing the role of an effective inverse proton radius (i.e. the InvRadius parameter in Table 5). However, predictions from a tune performed with pythia8 using a double-Gaussian matter distribution were not able to improve the quality of the fit as a fit obtained without interleaved FSR in the simulation of the UE (as it is implemented in pythia6) did not show any improvement. Further investigations are needed to resolve this issue.

The CMS DPS tunes

Traditionally, σeff is determined by fitting the DPS-sensitive observables with two templates [3236] that are often based on distributions obtained from QCD MC models. One template is constructed with no DPS, i.e. just single parton scattering (SPS), while the other represents DPS production. This determines σeff from the relative amounts of SPS and DPS contributions needed to fit the data. Here we use an alternative method that does not require construction of templates from MC samples. Instead, we fit the DPS-sensitive observables directly and then calculate the resulting σeff from the model. For example, in pythia8, the value of σeff is calculated by multiplying the ND cross section by an enhancement or a depletion factor, which expresses the dependence of DPS events on the collision impact parameter. As expected, more central collisions have a higher probability of a second hard scattering than peripheral collisions. The enhancement/depletion factors depend on the UE parameters, namely, on the parameters that characterize the matter-overlap function of the two protons, which for bProfile=3 is determined by the exponential parameter expPow, on the MPI regulator pT0 in Eq. (2), and the range of the CR. pythia8 Tune 4C gives σeff 30.3 mb at s=7TeV.

In Sect. 2, we determined the MPI parameters by fitting UE data. Here we determine the MPI parameters by fitting to observables which involve correlations among produced objects in hadron–hadron collisions that are sensitive to DPS. Two such observables used in the fit, ΔS and ΔrelpT, are defined as follows:

ΔS=arccospT(object1)·pT(object2)|pT(object1)|×|pT(object2)|, 5
ΔrelpT=|pTjet1+pTjet2||pTjet1|+|pTjet2|, 6

where, for W+dijet production, object1 is the W boson and object2 is the dijet system. For four-jet production, object1 is the hard-jet pair and object2 is the soft-jet pair. For ΔrelpT in W+dijet production, jet1 and jet2 are the two jets of the dijet system, while in four-jet production, jet1 and jet2 refer to the two softer jets.

The pythia8 UE parameters are fitted to the DPS-sensitive observables measured by CMS in W+dijet [36] and in four-jet production [37]. After extracting the MPI parameters, the value of σeff in Eq. (3) can be calculated from the underlying MPI model. In pythia8, σeff depends primarily on the matter-overlap function and, to a lesser extent, on the value of pT0 in Eq. (2), and the range of the CR. We obtain two separate tunes for each channel: in the first one, we vary just the matter-overlap parameter expPow, to which the σeff value is most sensitive, and in the second one, the whole set of parameters is varied. These two tunes allow to check whether the value of σeff is stable relative to the choice of parameters.

The W+dijet and the four-jet channels are fitted separately. The fit to DPS-sensitive observables in the W+dijet channel gives a new determination of σeff which can be compared to the value measured through the template method in the same final state [36]. Fitting the same way to the observables in the four-jet final state provides an estimate of σeff for this channel.

Double-parton scattering in W+dijet production

To study the dependence of the DPS-sensitive observables on MPI parameters, we construct two W+dijet DPS tunes, starting from the parameters of pythia8 Tune 4C. In a partial tune only the parameter of the exponential distribution expPow is varied, and in a full tune all four parameters in Table 6 are varied. In a comparison of models with W+dijet events [36], it was shown that higher-order SPS contributions (not present in pythia) fill a similar region of phase-space as the DPS signal. When such higher-order SPS diagrams are neglected, the measured DPS contribution to the W+dijet channel can be overestimated (i.e. σeff underestimated). We therefore interface the LO matrix elements (ME) generated by MadGraph 5 (version 1.5.14) [38] with pythia8, and tune to the normalized distributions of the correlation observables in Eqs. (5) and (6). For this study, we produce MadGraph parton-level events with a W boson and up to four partons in the final state. The cross section is calculated using the CTEQ6L1 PDF with a matching scale for ME and parton shower (PS) jets set to 20 GeV. (In Sect. 4, we show that the CMS UE tunes can be interfaced to higher-order ME generators without additional tuning of MPI parameters). Figure 6 shows the CMS data [36] for the observables ΔS and ΔrelpT measured in W+dijet production, compared to predictions from MadGraph interfaced to pythia8 Tune 4C, to Tune 4C with no MPI, to the partial CDPSTP8S1-Wj, as well as to the full CDPSTP8S2-Wj (CDPST stands for “CMS DPS tune”). Table 6 gives the best-fit parameters and the resulting σeff values at s=7TeV. The uncertainties quoted for σeff are computed from the uncertainties of the fitted parameters given by the eigentunes. For Tune 4C, the uncertainty in σeff is not provided since no eigentunes are available for that tune. The resulting values of σeff are compatible with the value measured by CMS using the template method of σeff=20.6±0.8(stat)±6.6(syst)\,mb  [36].

Table 6.

The pythia8 parameters, tuning ranges, Tune 4C values [28] and best-fit values of CDPSTP8S1-Wj and CDPSTP8S2-Wj, obtained from fits to DPS observables in W+dijet production with the MadGraph event generator interfaced to pythia8. Also shown are the predicted values of σeff at s=7TeV, and the uncertainties obtained from the eigentunes

pythia8 Parameter Tuning range Tune 4C CDPSTP8S1-Wj CDPSTP8S2-Wj
PDF CTEQ6L1 CTEQ6L1 CTEQ6L1
MultipartonInteractions:pT0Ref [GeV] 1.0–3.0 2.085 2.085a 2.501
MultipartonInteractions:ecmPow 0.0–0.4 0.19 0.19a 0.179
MultipartonInteractions:expPow 0.4–10.0 2.0 1.523 1.120
ColourReconnection:range 0.0–9.0 1.5 1.5a 2.586
MultipartonInteractions:ecmRef [GeV] 1800 1800a 1800a
χ2/dof 0.118 0.09
Predicted σeff (in mb) 30.3 25.9-2.9+2.4 25.8-4.2+8.2

a Fixed at Tune 4C value

Fig. 6.

Fig. 6

CMS data at s=7TeV [36] for the normalized distributions of the correlation observables ΔS (left), and ΔrelpT (right) in the W+dijet channel, compared to MadGraph (MG) interfaced to: pythia8 Tune 4C, Tune 4C with no MPI, and the CMS pythia8 DPS partial CDPSTP8S1-Wj (top); and CDPSTP8S1-Wj, and CDPSTP8S2-Wj (bottom). The bottom panels of each plot show the ratios of these tunes to the data, and the green bands around unity represent the total experimental uncertainty

Double-parton scattering in four-jet production

Starting from the parameters of pythia8 Tune 4C, we construct two different four-jet DPS tunes. As in the W+dijet channel, in the partial tune just the exponential-dependence parameter, expPow, while in the full tune all four parameters of Table 7 are varied. We obtain a good fit to the four-jet data without including higher-order ME contributions. However, we also obtain a good fit when higher-order (real) ME terms are generated with MadGraph. In Figs. 7 and 8 the correlation observables ΔS and ΔrelpT in four-jet production [37] are compared to predictions obtained with pythia8 Tune 4C, Tune 4C without MPI, CDPSTP8S1-4j, CDPSTP8S2-4j, and MadGraph interfaced to CDPSTP8S2-4j. Table 7 gives the best-fit parameters and the resulting σeff values. The values of σeff extracted from the CMS pythia8 DPS tunes give the first determination of σeff in four-jet production at s=7TeV. The uncertainties quoted for σeff are obtained from the eigentunes.

Table 7.

The pythia8 parameters, tuning ranges, Tune 4C values [28] and best-fit values of CDPSTP8S1-4j and CDPSTP8S2-4j, obtained from fits to DPS observables in four-jet production. Also shown are the predicted values of σeff at s=7TeV, and the uncertainties obtained from the eigentunes

pythia8 Parameter Tuning range Tune 4C CDPSTP8S1-4j CDPSTP8S2-4j
PDF CTEQ6L1 CTEQ6L1 CTEQ6L1
MultipartonInteractions:pT0Ref [GeV] 1.0–3.0 2.085 2.085a 2.125
MultipartonInteractions:ecmPow 0.0–0.4 0.19 0.19a 0.179
MultipartonInteractions:expPow 0.4–10.0 2.0 1.160 0.692
ColourReconnection:range 0.0–9.0 1.5 1.5a 6.526
MultipartonInteractions:ecmRef [GeV] 1800 1800a 1800a
χ2/dof 0.751 0.428
Predicted σeff (in mb) 30.3 21.3-1.6+1.2 19.0-3.0+4.7

a Fixed at Tune 4C value

Fig. 7.

Fig. 7

Distributions of the correlation observables ΔS (left) and ΔrelpT (right) measured in four-jet production at s=7TeV [37] compared to pythia8 Tune 4C, Tune 4C with no MPI, and CDPSTP8S1-4j. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

Fig. 8.

Fig. 8

Distributions in the correlation observables ΔS (top) and ΔrelpT (bottom) measured in four-jet production at s=7TeV [37], compared to predictions of pythia8 using CDPSTP8S2-4j and of MadGraph (MG) interfaced to pythia8 using CDPSTP8S2-4j (left) and pythia8 using CUETP8M1 and herwig++ with CUETHppS1 (right). Also shown are the ratios of the predictions to the data. Predictions for CUETP8M1 (right) are shown with an error band corresponding to the total uncertainty obtained from the eigentunes (Appendix A). The green bands around unity represent the total experimental uncertainty

Validation of CMS tunes

Here we discuss the compatibility of the UE and DPS tunes. In addition, we compare the CMS UE tunes with UE data that have not been used in the fits, and we examine how well Drell–Yan and MB observables can be predicted from MC simulations using the UE tunes. We also show that the CMS UE tunes can be interfaced to higher-order ME generators without additional tuning of the MPI parameters.

Compatibility of UE and DPS tunes

The values of σeff obtained from simulations applying the CMS pythia8 UE and DPS tunes at s=7TeV and s=13TeV are listed in Table 8. The uncertainties, obtained from eigentunes are also quoted in Table 8. At s=7TeV, the CMS DPS tunes give values of σeff 20\,mb, while the CMS pythia8 UE tunes give slightly higher values in the range 26–29 mb as shown in Figs. 8 and  9. Figure 8 shows the CMS DPS-sensitive data for four-jet production at s=7TeV compared to predictions using CDPSTP8S2-4j, CUETP8M1, and CUETHppS1. Figure 9 shows ATLAS UE data at s=7TeV [39] compared to predictions obtained with various tunes: CDPSTP8S2-4j with uncertainty bands, CUETP6S1-CTEQ6L1, CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, CUETP8M1, and CUETHppS1. Predictions from pythia8 using CUETP8M1 describe reasonably well the DPS observables, but do not fit them as well as predictions using the DPS tunes. On the other hand, predictions using CDPSTP8S2-4j do not fit the UE data as well as the UE tunes do.

Table 8.

Values of σeff at s=7TeV and 13TeV for CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, CUETHppS1, and for CDPSTP8S1-4j and CDPSTP8S2-4j. At s=7TeV, also shown are the uncertainties in σeff obtained from the eigentunes

CMS tune σeff(mb) at 7TeV σeff(mb) at 13TeV
CUETP8S1-CTEQ6L1 27.8-1.3+1.2 29.9-2.8+1.6
CUETP8S1-HERAPDF1.5LO 29.1-2.0+2.2 31.0-2.6+3.8
CUETP8M1 26.0-0.2+0.6 27.9-0.4+0.7
CUETHppS1 15.2-0.6+0.5 15.2-0.6+0.5
CDPSTP8S1-4j 21.3-1.6+1.2 21.8-0.7+1.0
CDPSTP8S2-4j 19.0-3.0+4.7 22.7-5.2+10.0

Fig. 9.

Fig. 9

ATLAS data at s=7TeV [39] for charged-particle (left) and pTsum densities (right) with pT>0.5GeV and |η|<2.0 in the transverse (TransAVE) region compared to predictions of pythia8 using CDPSTP8S2-4j (left) and CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, plus herwig++ using CUETHppS1 (right). The predictions of CDPSTP8S2-4j are shown with an error band corresponding to the total uncertainty obtained from the eigentunes (Appendix A). The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

As discussed previously, the pythia8 tunes use a single exponential matter-overlap function, while the herwig++ tune uses a matter-overlap function that is related to the Fourier transform of the electromagnetic form factor. The CUETHppS1 gives a value of σeff 15\,mb, while UE and DPS tunes give higher values of σeff. It should be noted that σeff is a parton-level observable and its importance is not in the modelled value of σeff, but in what is learned about the transverse proton profile (and its energy evolution), and how well the models describe the DPS-sensitive observables. As can be seen in Fig. 8, predictions using CUETP8M1 describe the DPS-sensitive observables better than CUETHppS1, but not quite as well as the DPS tunes. We performed a simultaneous pythia8 tune that included both the UE data and DPS-sensitive observables, however, the quality of the resulting fit was poor. This confirms the difficulty of describing soft and hard MPI within the current pythia and herwig++ frameworks. Recent studies [40, 41] suggest the need for introducing parton correlation effects in the MPI framework in order to achieve a consistent description of both the UE and DPS observables.

Comparisons with other UE measurements

Figure 10 shows charged particle and pTsum densities [24, 42] at s=0.9, 2.76, and 7TeV with pT>0.5GeV and |η|<2.0 in the TransAVE region, as defined by the leading jet reconstructed by using just the charged particles (also called “leading track-jet”) compared to predictions using the CMS UE tunes. The CMS UE tunes describe quite well the UE measured using the leading charged particle as well as the leading charged-particle jet.

Fig. 10.

Fig. 10

CMS data on charged-particle (left) and pTsum (right) densities at s = 0.9 [24] (top), 2.76 [42] (middle), and 7TeV [24] (bottom) with pT>0.5GeV and |η|<2.0 in the transverse (TransAVE) region as defined by the leading charged-particle jet, as a function of the transverse momentum of the leading charged-particle jet. The data are compared to predictions of pythia6 using CUETP6S1-CTEQ6L1, pythia8 using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, and herwig++ using CUETHppS1. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

Tunes obtained from fits to UE data and combined with higher-order ME calculations [43] can also be cross-checked against the data. The CMS UE tunes can be interfaced to higher-order ME generators without spoiling their good description of the UE. In Fig. 11, the charged-particle and pTsum densities in the TransMIN and TransMAX regions as a function of pTmax, are compared to predictions obtained with MadGraph and powheg  [44, 45] interfaced to pythia8 using CUETP8S1-CTEQ6L1 and CUETP8M1. In MadGraph, up to four partons are simulated in the final state. The cross section is calculated with the CTEQ6L1 PDF. The ME/PS matching scale is taken to be 10GeV. The powheg predictions are based on next-to-leading-order (NLO) dijet using the CT10nlo PDF [46] interfaced to pythia8 based on CUETP8M1, and HERAPDF1.5NLO [21] interfaced to the pythia8 using CUETP8S1-HERAPDF1.5LO.

Fig. 11.

Fig. 11

CMS data at s=7TeV  [17] for particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions, as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to MadGraph (MG), interfaced to pythia8 using CUETP8S1-CTEQ6L1 and CUETP8M1, and to powheg (PH), interfaced to pythia8 using CUETP8S1-HERAPDF1.5LO and CUETP8M1. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

The poor agreement below pTmax=5GeV in Fig. 11 is not relevant as the minimum p^T for MadGraph and powheg is 5GeV. The agreement with the UE data in the plateau region of pTmax>5GeV is good. All these figures show that CMS UE tunes interfaced to higher-order ME generators do not spoil their good description of the UE data.

Predicting MB observables

The UE is studied in events containing a hard scatter, whereas most of the MB collisions are softer and can include diffractive scatterings. It is however interesting to see how well predictions based on the CMS UE tunes can describe the properties of MB distributions. Figure 12 shows predictions using CMS UE tunes for the ALICE [47] and TOTEM data [48] at s=7TeV for the charged-particle pseudorapidity distribution, dNch/dη, and for dE/dη [49] at s=7TeV. These observables are sensitive to single-diffraction dissociation, central-diffraction, and double-diffraction dissociation, which are modelled in pythia. Since herwig++ does not include a model for single-diffraction dissociation, central-diffraction, and double-diffraction dissociation, we do not show it here. Figure 13 shows predictions using the CMS UE tunes for the combined CMS+TOTEM data at s=8TeV [50] for the charged-particle pseudorapidity distribution, dNch/dη, for inelastic, non single-diffraction-enhanced, and single-diffraction-enhanced proton–proton collisions.

Fig. 12.

Fig. 12

ALICE data at s=7TeV [47] for the charged-particle pseudorapidity distribution, dNch/dη, in inclusive inelastic pp collisions (top left). TOTEM data at s=7TeV [48] for the charged-particle pseudorapidity distribution, dNch/dη, in inclusive inelastic pp collisions (pT>40MeV, Nchg1) (top right). CMS data at s=7TeV [50] for the energy flow dE/dη, in MB pp collisions. The data are compared to pythia6 using CUETP6S1-CTEQ6L1, and to pythia8 using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

Fig. 13.

Fig. 13

Combined CMS and TOTEM data at s=8TeV [50] for the charged-particle distribution dNch/dη, in inclusive inelastic (top left), NSD-enhanced (top right), and SD-enhanced (bottom) pp collisions. The data are compared to pythia6 using CUETP6S1-CTEQ6L1, and to pythia8 using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

The pythia8 event generator using the UE tunes describes the MB data better than pythia6 with the UE tune, which is likely due to the improved modelling of single-diffraction dissociation, central-diffraction, and double-diffraction dissociation in pythia8. Predictions with all the UE tunes describe fairly well MB observables in the central region (|η|<2), however, only predictions obtained with CUETP8M1 describe the data in the forward region (|η|>4). This is due to the PDF used in CUETP8M1. As can be seen in Fig. 14, the NNPDF2.3LO PDF at scales Q2 = 10 GeV2 (corresponding to hard scatterings with p^T 3 GeV) and small x, features a larger gluon density than in CTEQ6L1 and HERAPDF1.5LO, thereby contributing to more particles (and more energy) produced in the forward region. We have checked that increasing the gluon distribution in HERAPDF1.5LO at values below 10-5 improved the description of the charged-particle multiplicity measurements in the forward region.

Fig. 14.

Fig. 14

Comparison of gluon distributions in the proton for the CTEQ6L1, HERAPDF1.5LO, and NNPDF2.3LO PDF sets, at the Q2 = 10 GeV2 (left) and 100 GeV2 (right)

Comparisons with inclusive jet production

In Fig. 15 predictions using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, and CUETHppS1 are compared to inclusive jet cross section at s=7TeV [51] in several rapidity ranges. Predictions using CUETP8M1 describe the data best, however, all the tunes overshoot the jet spectra at small pT. Predictions from the CUETHppS1 underestimate the high pT region at central rapidity (|y| < 2.0). In Fig. 16, the inclusive jet cross sections are compared to predictions from powheg interfaced to pythia8 using CUETP8S1-HERAPDF1.5LO and CUETP8M1. A very good description of the measurement is obtained.

Fig. 15.

Fig. 15

CMS data at s=7TeV [51] for the inclusive jet cross section as a function of pT in different rapidity ranges compared to predictions of pythia8 using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF, and CUETP8M1, and of herwig++ using CUETHppS1. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

Fig. 16.

Fig. 16

CMS data at s=7TeV [51] for the inclusive jet cross section as a function of pT in different rapidity ranges compared to predictions of powheg interfaced to pythia8 using CUETP8S1-HERAPDF1.5LO and CUETP8M1. The bottom panels of each plot show the ratios of these predictions to the data, and the green bands around unity represent the total experimental uncertainty

Comparisons with Z boson production

In Fig. 17 the pT and rapidity distributions of the Z boson in pp collisions at s=7TeV [52] are shown and compared to pythia8 using CUETP8M1, and to powheg interfaced to pythia8 using CUETP8S1-CTEQ6L1 and CUETP8M1. The prediction using pythia8 with CUETP8M1 (without powheg) agrees reasonably well with the distribution of the Z boson at small pT values. Also, when interfaced to powheg, which implements an inclusive Z boson NLO calculation, the agreement is good over the whole spectrum.

Fig. 17.

Fig. 17

Transverse momentum pT (left) and rapidity distributions (right) of Z boson production in pp collisions at s=7TeV [52]. The data are compared to pythia8 using CUETP8M1, and to powheg interfaced to pythia8 using CUETP8S1-CTEQ6L1 and CUETP8M1. The green bands in the ratios represent the total experimental uncertainty

In Fig. 18 the charged-particle and pTsum densities [26] in the toward, away, and transverse (TransAVE) regions as defined by the Z boson in proton–proton collisions at s=7TeV are compared to predictions of pythia8 using CUETP8M1. Also shown are MadGraph and powheg results interfaced to pythia8 using CUETP8S1-HERAPDF1.5LO and CUETP8M1. The MadGraph generator simulates Drell–Yan events with up to four partons, using the CTEQ6L1 PDF. The matching of ME partons and PS is performed at a scale of 20 GeV. The powheg events are obtained using NLO inclusive Drell–Yan production, including up to one additional parton. The powheg events are interfaced to pythia8 using CUETP8M1 and CUETP8S1-HERAPDF1.5LO. The predictions based on CUETP8M1 do not fit the Z boson data unless they are interfaced to a higher-order ME generator. In pythia8 only the Born term (qq¯Z), corrected for single-parton emission, is generated. This ME configuration agrees well with the observables in the away region in data, when the Z boson recoils against one or more jets. In the transverse and toward regions, larger discrepancies between data and pythia8 predictions appear at high pT, where the occurrence of multijet emission has a large impact. To describe Z boson production at s=7TeV in all regions, higher-order contributions (starting with Z+2-jets), as used in interfacing pythia to powheg or MadGraph, must be included.

Fig. 18.

Fig. 18

Charged-particle (left) and pTsum densities (right) in the toward (top), away (middle), and transverse (TransAVE) (bottom) regions, as defined by the Z-boson direction in Drell–Yan production at s=7TeV [26]. The data are compared to pythia8 using CUETP8M1, to MadGraph (MG) interfaced to pythia8 using CUETP8S1-CTEQ6L1 and CUETP8M1, and to powheg (PH) interfaced to pythia8 using CUETP8S1-HERAPDF1.5LO and CUETP8M1. The green bands in the ratios represent the total experimental uncertainty

Extrapolation to 13 TeV

In this section, predictions at s=13TeV, based on the new tunes, for observables sensitive to the UE are presented. Figure 19 shows the predictions at 13 TeV for the charged-particle and the pTsum densities in the TransMIN, TransMAX, and TransDIF regions, as defined by the leading charged particle as a function of pTmax based on the five new CMS UE tunes: CUETP6S1-CTEQ6L1, CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, CUETP8M1, and CUETHppS1. In Fig. 19 the ratio of the predictions using the four CMS tunes to the one using CUETP8M1 is shown. The predictions at 13TeV of all these tunes are remarkably similar. It does not seem to matter that the new CMS pythia8 UE tunes do not fit very well to the s=300GeV UE data. The new pythia8 tunes give results at 13TeV similar to the new CMS pythia6 tune and the new CMS herwig++ tune. The uncertainties on the predictions based on the eigentunes do not exceed 10 % relative to the central value.

Fig. 19.

Fig. 19

Predictions at s=13TeV for the particle (left) and the pTsum densities (right) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (top), TransMAX (middle), and TransDIF (bottom) regions, as defined by the leading charged particle, as a function of the leading charged-particle pTmax for the five CMS UE tunes: pythia6 CUETP6S1-CTEQ6L1, and pythia8 CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, and herwig++ CUETHppS1. Also shown are the ratio of the tunes to predictions of CUETP8S1-CTEQ6L1. Predictions for CUETP8M1 are shown along with the envelope (green bands) of the corresponding eigentunes

In Figs. 20 and 21 the predictions at s=13TeV obtained using the new tunes from 7TeV are shown for the charged-particle and the pTsum densities in the TransMIN, TransMAX, and TransDIF regions, defined as a function of pTmax. Also shown is the ratio of 13TeV to 7TeV results for the five tunes. The TransMIN region increases much more rapidly with energy than the TransDIF region. For example, when using CUETP8M1, the charged-particle and the pTsum densities in the TransMIN region for 5.0<pTmax<6.0GeV is predicted to increase by 28 and 37%, respectively, while the TransDIF region is predicted to increase by a factor of two less, i.e. by 13 and 18% respectively.

Fig. 20.

Fig. 20

Charged-particle density at s=7TeV for particles with pT>0.5GeV and |η|<0.8 in the TransMIN (top), TransMAX (middle), and TransDIF (bottom) regions, as defined by the leading charged particle, as a function of the leading charged-particle pTmax. The data are compared to pythia6 using CUETP6S1-CTEQ6L1, to pythia8 using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, and to herwig++ using CUETHppS1. Also shown are the predictions (left) based on the CMS UE tunes at 13TeV (dashed lines), and the ratio of the 13TeV to 7TeV results for the five tunes (right)

Fig. 21.

Fig. 21

Charged pTsum density at s=7TeV for particles with pT>0.5GeV and |η|<0.8 in the TransMIN (top), TransMAX (middle), and TransDIF (bottom) regions, as defined by the leading charged particle, as a function of the leading charged-particle pTmax. The data are compared to pythia6 using CUETP6S1-CTEQ6L1, to pythia8 using CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, and to herwig++ using CUETHppS1. Also shown are the predictions (left) based on the CMS UE tunes at 13TeV (dashed lines), and the ratio of the 13TeV to 7TeV results for the five tunes (right)

In Fig. 22, predictions obtained with pythia8 using CUETP8S1-CTEQ6L1 and CUETP8M1, and Tune 4C are compared to the recent CMS data measured at s=13TeV [53] on charged-particle multiplicity as a function of pseudorapidity. Predictions from CUETP8S1-CTEQ6L1 and CUETP8M1 are shown with the error bands corresponding to the uncertainties obtained from the eigentunes. These two new CMS tunes, although obtained from fits to UE data at 7TeV, agree well with the MB measurements over the whole pseudorapidity range, while predictions from pythia8 Tune 4C overestimate the data by about 10 %. This confirms that the collision-energy dependence of the CMS UE tunes parameters can be trusted for predictions of MB observables.

Fig. 22.

Fig. 22

CMS data at s=13TeV [53] for the charged-particle pseudorapidity distribution, dNch/dη, in inelastic proton–proton collisions. The data are compared to predictions of pythia8 using CUETP8S1-CTEQ6L1, CUETP8M1, and Tune 4C. The predictions based on CUETP8S1-CTEQ6L1 and CUETP8M1 are shown with an error band corresponding to the total uncertainty obtained from the eigentunes. Also shown are the ratios of these predictions to the data. The green band represents the total experimental uncertainty on the data

Summary and conclusions

New tunes of the pythia event generator were constructed for different parton distribution functions using various sets of underlying-event (UE) data. By simultaneously fitting UE data at several center-of-mass energies, models for UE have been tested and their parameters constrained. The improvement in the description of UE data provided by the new CMS tunes at different collision energies gives confidence that they can provide reliable predictions at s=13TeV, where all the new UE tunes predict similar results for the UE observables.

The observables sensitive to double-parton scattering (DPS) were fitted directly by tuning the MPI parameters. Two W+dijet DPS tunes and two four-jet DPS tunes were constructed to study the dependence of the DPS-sensitive observables on the MPI parameters. The CMS UE tunes perform fairly well in the description of DPS observables, but they do not fit the DPS data as well as the DPS tunes do. On the other hand, the CMS DPS tunes do not fit the UE data as well as the UE tunes. At present, it is not possible to accurately describe both soft and hard MPI within the current pythia and herwig++ frameworks. Fitting DPS-sensitive observables has also provided the DPS effective cross section σeff associated to each model. This method can be applied to determine the σeff values associated with different MPI models implemented in the current MC event generators for the production of any final-state with two hard particles.

Predictions of pythia8 using the CMS UE tunes agree fairly well with the MB observables in the central region (|η|<2) and can be interfaced to higher-order and multileg matrix-element generators, such as powheg and MadGraph, while maintaining their good description of the UE. It is not necessary to produce separate tunes for these generators. In addition, we have verified that the measured particle pseudorapidity density at 13TeV is well reproduced by the new CMS UE Tunes. Furthermore, all of the new CMS tunes come with their eigentunes, which can be used to determine the uncertainties associated with the theoretical predictions. These new CMS tunes will play an important role in predicting and analyzing LHC data at 13 and 14TeV.

Acknowledgments

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 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 and the CMS detector provided by the following funding agencies: the Austrian Federal Ministry of Science, Research and Economy and the Austrian Science Fund; the Belgian Fonds de la Recherche Scientifique, and Fonds voor Wetenschappelijk Onderzoek; the Brazilian Funding Agencies (CNPq, CAPES, FAPERJ, and FAPESP); the Bulgarian Ministry of Education and Science; CERN; the Chinese Academy of Sciences, Ministry of Science and Technology, and National Natural Science Foundation of China; the Colombian Funding Agency (COLCIENCIAS); the Croatian Ministry of Science, Education and Sport, and the Croatian Science Foundation; the Research Promotion Foundation, Cyprus; the Ministry of Education and Research, Estonian Research Council via IUT23-4 and IUT23-6 and European Regional Development Fund, Estonia; the Academy of Finland, Finnish Ministry of Education and Culture, and Helsinki Institute of Physics; the Institut National de Physique Nucléaire et de Physique des Particules/CNRS, and Commissariat à l’Énergie Atomique et aux Énergies Alternatives/CEA, France; the Bundesministerium für Bildung und Forschung, Deutsche Forschungsgemeinschaft, and Helmholtz-Gemeinschaft Deutscher Forschungszentren, Germany; the General Secretariat for Research and Technology, Greece; the National Scientific Research Foundation, and National Innovation Office, Hungary; the Department of Atomic Energy and the Department of Science and Technology, India; the Institute for Studies in Theoretical Physics and Mathematics, Iran; the Science Foundation, Ireland; the Istituto Nazionale di Fisica Nucleare, Italy; the Ministry of Science, ICT and Future Planning, and National Research Foundation (NRF), Republic of Korea; the Lithuanian Academy of Sciences; the Ministry of Education, and University of Malaya (Malaysia); the Mexican Funding Agencies (CINVESTAV, CONACYT, SEP, and UASLP-FAI); the Ministry of Business, Innovation and Employment, New Zealand; the Pakistan Atomic Energy Commission; the Ministry of Science and Higher Education and the National Science Centre, Poland; the Fundação para a Ciência e a Tecnologia, Portugal; JINR, Dubna; the Ministry of Education and Science of the Russian Federation, the Federal Agency of Atomic Energy of the Russian Federation, Russian Academy of Sciences, and the Russian Foundation for Basic Research; the Ministry of Education, Science and Technological Development of Serbia; the Secretaría de Estado de Investigación, Desarrollo e Innovación and Programa Consolider-Ingenio 2010, Spain; the Swiss Funding Agencies (ETH Board, ETH Zurich, PSI, SNF, UniZH, Canton Zurich, and SER); the Ministry of Science and Technology, Taipei; the Thailand Center of Excellence in Physics, the Institute for the Promotion of Teaching Science and Technology of Thailand, Special Task Force for Activating Research and the National Science and Technology Development Agency of Thailand; the Scientific and Technical Research Council of Turkey, and Turkish Atomic Energy Authority; the National Academy of Sciences of Ukraine, and State Fund for Fundamental Researches, Ukraine; the Science and Technology Facilities Council, UK; the US Department of Energy, and the US National Science Foundation. Individuals have received support from the Marie-Curie programme and the European Research Council and EPLANET (European Union); the Leventis Foundation; the A. 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 Ministry of Education, Youth and Sports (MEYS) of the Czech Republic; the Council of Science and Industrial Research, India; the HOMING PLUS programme of the Foundation for Polish Science, cofinanced from European Union, Regional Development Fund; the OPUS programme of the National Science Center (Poland); the Compagnia di San Paolo (Torino); MIUR project 20108T4XTM (Italy); the Thalis and Aristeia programmes cofinanced by EU-ESF and the Greek NSRF; the National Priorities Research Program by Qatar National Research Fund; the Rachadapisek Sompot Fund for Postdoctoral Fellowship, Chulalongkorn University (Thailand); and the Welch Foundation, contract C-1845.

Appendix A: Tables of tune uncertainties

This section provides the values of the parameters corresponding to the eigentunes of the new CMS pythia8 and the herwig++ tunes. A change in the χ2 of the fit that equals the absolute χ2 value obtained in the tune defines the eigentunes listed in Tables 9, 10, 11 and 12 for the new pythia8 and the new herwig++ tunes. The different parameter values indicated refer to the deviation tunes along each of the maximally independent directions in the parameter space, obtained by using the covariance matrix in the region of the best tune. The number of directions defined in the parameter space equals the number of free parameters n used in the fit and results into 2n parameter variations, i.e. eigentunes. These variations represent a good set of systematic errors on the given tune.

Table 9.

Eigentunes sets for CUETP8S1-CTEQ6L1

pythia8 parameter 1- 1+ 2- 2+ 3- 3+ 4- 4+
MultipartonInteractions:pT0Ref [GeV] 2.101 2.101 2.068 2.135 2.100 2.102 2.079 2.123
MultipartonInteractions:ecmPow 0.191 0.231 0.210 0.211 0.231 0.191 0.191 0.231
MultipartonInteractions:expPow 1.609 1.609 1.602 1.616 1.613 1.605 1.714 1.503
ColourReconnection:range 3.030 3.609 3.313 3.313 3.311 3.314 3.314 3.311

Table 10.

Eigentunes sets for CUETP8S1-HERAPDF

pythia8 parameter 1- 1+ 2- 2+ 3- 3+ 4- 4+
MultipartonInteractions:pT0Ref [GeV] 2.000 2.000 1.960 2.043 1.999 2.001 1.968 2.030
MultipartonInteractions:ecmPow 0.275 0.226 0.250 0.250 0.226 0.275 0.274 0.227
MultipartonInteractions:expPow 1.691 1.690 1.681 1.700 1.695 1.686 1.831 1.559
ColourReconnection:range 6.224 5.972 6.096 6.096 6.101 6.091 6.091 6.101

Table 11.

Eigentunes sets for CUETP8M1

pythia8 parameter 1- 1+ 2- 2+
MultipartonInteractions:pT0Ref [GeV] 2.403 2.402 2.400 2.405
MultipartonInteractions:ecmPow 0.253 0.251 0.253 0.252

Table 12.

Eigentunes sets for CUETHppS1

herwig++ parameter 1- 1+ 2- 2+ 3- 3+ 4- 4+
MPIHandler:InvRadius 2.290 2.227 2.318 2.196 2.272 2.237 2.254 2.256
RemnantDecayer:colourDisrupt 0.396 0.811 0.634 0.623 0.632 0.625 0.596 0.666
MPIHandler:Power 0.396 0.351 0.331 0.408 0.399 0.342 0.361 0.381
ColourReconnector:ReconnectionProbability 0.615 0.460 0.529 0.527 0.523 0.533 0.444 0.626

Appendix B: Comparisons of PYTHIA6 UE tunes to data

Figures 23, 24, 25 and 26 show the CDF data at s=0.3, 0.9, and 1.96TeV, and the CMS data at s=7TeV on charged-particle and pTsum densities in the TransMIN and TransMAX regions, as a function of the transverse momentum of the leading charged-particle pTmax. The distributions are compared to predictions obtained with pythia6 Tune Z2lep and the two new CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO. The new CMS pythia6 tunes are able to describe the measurements better than Tune Z2lep, in both the rising and the plateau regions of the spectra.

Fig. 23.

Fig. 23

CDF data at s=300GeV [11] on the particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the pythia6 Tune Z2lep, CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO. The green bands in the ratios represent the total experimental uncertainties

Fig. 24.

Fig. 24

CDF data at s=900GeV [11] on the particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading-charged particle pTmax. The data are compared to the pythia6 Tune Z2lep, CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO. The green bands in the ratios represent the total experimental uncertainties

Fig. 25.

Fig. 25

CDF data at s=1.96TeV [11] on the particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the pythia6 Tune Z2lep, CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO. The green bands in the ratios represent the total experimental uncertainties

Fig. 26.

Fig. 26

CMS data at s=7TeV [17] on the particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the pythia6 Tune Z2lep, CUETP6S1-CTEQ6L1 and CUETP6S1-HERAPDF1.5LO. The green bands in the ratios represent the total experimental uncertainties

Appendix C: Comparisons to HERWIG++ UE tunes to data

Figures 27, 28, 29 and 30 show the CDF data at s=0.3, 0.9, and 1.96TeV, and the CMS data at s=7TeV on the charged-particle and pTsum densities in the TransMIN and TransMAX regions as a function of pTmax, and compared with predictions obtained with the herwig++ Tune UE-EE-5C and the new CUETHppS1. These two herwig++ tunes are very similar and adequately describe the UE data at all four energies.

Fig. 27.

Fig. 27

CDF data at s=300GeV [11] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the herwig++ Tune UE-EE-5C and CUETHppS1. The green bands in the ratios represent the total experimental uncertainties

Fig. 28.

Fig. 28

CDF data at s=900GeV [11] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the herwig++ Tune UE-EE-5C and CUETHppS1. The green bands in the ratios represent the total experimental uncertainties

Fig. 29.

Fig. 29

CDF data at s=1.96TeV [11] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the herwig++ Tune UE-EE-5C and CUETHppS1. The green bands in the ratios represent the total experimental uncertainties

Fig. 30.

Fig. 30

CMS data at s=7TeV [17] on particle (top) and pTsum densities (bottom) for charged particles with pT>0.5GeV and |η|<0.8 in the TransMIN (left) and TransMAX (right) regions as defined by the leading charged particle, as a function of the transverse momentum of the leading charged-particle pTmax. The data are compared to the herwig++ Tune UE-EE-5C and CUETHppS1. The green bands in the ratios represent the total experimental uncertainties

Appendix D: Additional comparisons at 13 TeV

In this section, a supplementary collection of comparisons among predictions of the new tunes are shown for DPS and MB observables at 13TeV.

D.1 DPS predictions at 13 TeV

In Fig. 31, the predictions for the DPS-sensitive observables at 13TeV are shown for the three CMS pythia8 UE tunes: CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, for CUETHppS1, and for the two CMS pythia8 DPS tunes CDPSTP8S1-4j and CDPSTP8S2-4j. In herwig++, σeff is independent of the center-of-mass energy, while pythia8 gives a σeff that increases with energy. The pythia8 UE tunes predict that σeff will increase by about 7% between 7 and 13TeV, while the CDPSTP8S2-4j predicts an increase of about 20%. This results in slightly different predictions for the DPS-sensitive observables at 13TeV for the CMS UE tunes and the CMS DPS tunes.

Fig. 31.

Fig. 31

Predictions at s=13TeV for the normalized distributions of the correlation observables ΔS (left), and ΔrelpT (right) for four-jet production in pp collisions for the three CMS pythia8 UE tunes CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1, for CUETHppS1, and for CDPSTP8S1-4j and CDPSTP8S2-4j. Also shown are the ratios of the tunes to predictions of CUETP8S1-CTEQ6L1

D.2 MB predictions at 13 TeV

Predictions of the CMS UE tunes at s=13TeV are shown in Fig. 32 for the charged-particle pseudorapidity distribution, dNch/dη, for inelastic, non single-diffraction-enhanced, and single-diffraction-enhanced proton–proton collisions. In Fig. 32, the ratio of 13 to 8TeV results is shown for each of the tunes. The densities in the forward region are predicted to increase more rapidly than the central region between 8 and 13TeV. However, the UE observables in Figs. 20 and 21 increase much faster with center-of-mass energy than do these MB observables.

Fig. 32.

Fig. 32

Predictions at s=13TeV for the charged-particle pseudorapidity distribution dNch/dη, for (top) inelastic, (middle) NSD-enhanced, and (bottom) SD-enhanced pp collisions from CUETP6S1-CTEQ6L1, CUETP8S1-CTEQ6L1, CUETP8S1-HERAPDF1.5LO, and CUETP8M1. Also shown are the ratios of the tunes to predictions of CUETP8M1, and the ratio of 13 to 8TeV results for each of the tunes (right)

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