Measurements of inclusive jet spectra in pp and central Pb-Pb collisions at √sNN = 5.02 TeV

This is a sel -a chi ed e sion o an o iginal a icle. This e sion may di e om he o iginal in pagina ion and ypog aphic de ails. Au ho (s): Ti le: Yea : Ve sion: Copy igh : Righ s: Righ s u l: Please ci e he o iginal e sion: CC BY 4.0 h ps://c ea i ecommons.o g/licenses/by/4.0/ Measu emen s o inclusi e je spec a in pp and cen al Pb-Pb collisions a √sNN = 5.02 TeV ©2020 CERN, o he ALICE Collabo a ion Published e sion ALICE Collabo a ion ALICE Collabo a ion. (2020). Measu emen s o inclusi e je spec a in pp and cen al Pb-Pb collisions a √sNN = 5.02 TeV. Physical Re iew C, 101(3), A icle 034911. h ps://doi.o g/10.1103/PhysRe C.101.034911 2020 PHYSICAL REVIEW C 101, 034911 (2020) Measu emen s o inclusi e je spec a in pp and cen al Pb-Pb collisions a √sNN =5.02 TeV S. Acha ya e al.∗ (ALICE Collabo a ion) (Recei ed 4 Oc obe 2019; accep ed 12 Feb ua y 2020; published 16 Ma ch 2020) This a icle epo s measu emen s o he pT-di e en ial inclusi e je c oss sec ion in pp collisions a √s= 5.02 TeV and he pT-di e en ial inclusi e je yield in Pb-Pb 0–10% cen al collisions a √sNN =5.02 TeV. Je s we e econs uc ed a mid apidi y wi h he ALICE acking de ec o s and elec omagne ic calo ime e using he an i-kTalgo i hm. Fo pp collisions, we epo je c oss sec ions o je esolu ion pa ame e s R=0.1–0.6 o e he ange 20 <pT,je <140 GeV/c, as well as he je c oss-sec ion a ios o di e en Rand compa isons o wo nex - o-leading-o de (NLO)–based heo e ical p edic ions. Fo Pb-Pb collisions, we epo he R=0.2and R=0.4 je spec a o 40 <pT,je <140 GeV/cand 60 <pT,je <140 GeV/c, espec i ely. The scaled a io o je yields obse ed in Pb-Pb o pp collisions, RAA, is cons uc ed, and exhibi s s ong je quenching and a clea pTdependence o R=0.2. No signi ican Rdependence o he je RAA is obse ed wi hin he unce ain ies o he measu emen . These esul s a e compa ed o se e al heo e ical p edic ions. DOI: 10.1103/PhysRe C.101.034911 I. INTRODUCTION A decon ined s a e o s ongly in e ac ing ma e desc ibed by quan um ch omodynamics (QCD) is p oduced in ul a- ela i is ic hea y-ion collisions a he Rela i is ic Hea y Ion Collide (RHIC) and he La ge Had on Collide (LHC) [1–8]. Nume ous obse ables including high-pThad on supp ession, aniso opic low, and J/ψ supp ession and ecombina ion p o ide e idence ha he ho QCD s a e p oduced in hese collisions consis s o subnucleonic deg ees o eedom. One o he majo s a egies o in es iga e his ho QCD s a e is he s udy o je modi ica ion in hea y-ion collisions. Pa ons o en a e se a signi ican pa h leng h o he ho QCD medium, and he e ec ha he medium has on he esul ing je s can be deduced by compa ing je p ope ies in hea y-ion collisions o hose in pp collisions. Since he je p oduc ion c oss sec ion can be compu ed in pe u ba i e QCD, and since je s a e sensi i e o a wide ange o momen um exchanges wi h he medium, je physics is an appealing ool o in es iga e he medium a a wide ange o esolu ion scales. P e ious measu emen s demons a e supp ession o he je ans e se momen um (pT) spec um in hea y-ion collisions ela i e o pp collisions scaled by he numbe o incohe en bina y nucleon-nucleon collisions, indica ing ha je s ans e ene gy o he ho QCD medium [9–15]. Fu he mo e, je sub- s uc u e measu emen s indica e ha in hea y-ion collisions, he je co e is mo e collima ed and agmen s a e ha de [16], ∗Full au ho lis gi en a he end o he a icle. Published by he Ame ican Physical Socie y unde he e ms o he C ea i e Commons A ibu ion 4.0 In e na ional license. Fu he dis ibu ion o his wo k mus main ain a ibu ion o he au ho (s) and he published a icle’s i le, jou nal ci a ion, and DOI. while a wide angles om he je axis he e is an excess o so pa icles [17,18]. Je modi ica ion in hea y-ion collisions is desc ibed by se e al di e en heo e ical app oaches ypically based on ene gy loss ia medium-induced gluon adia ion and elas ic sca e ing [19–22, and e e ences he ein]; howe e , he e emains no clea consensus o he p ecise na u e o he in e ac ion o je s wi h he medium. New measu emen s o he absolu e le el o je supp ession and i s pTdependence will di ec ly es models and se e as a key cons ain o global analyses o high-pTobse ables. Addi ionally, he e olu ion o je supp ession wi h he je esolu ion pa ame e , R, can cons ain compe ing e ec s be ween he eco e y o ou -o - cone adia ion and he changing selec ion o he je popula ion (such as educ ion o he qua k/gluon ac ion) as Rinc eases [23–25]. The inclusi e je c oss sec ion in pp collisions con ains impo an QCD physics i sel . In ecen yea s, he inclusi e je c oss sec ion in pp collisions was compu ed a NLO wi h esumma ion o loga i hms o he je esolu ion pa am- e e [26–29] and h eshold loga i hms [30,31], and also o NNLO bo h wi h and wi hou he leading colo app oxima ion [32,33]. Measu emen s o he inclusi e pp je c oss sec ion ha e been made a he SPS [34,35], he Te a on [36,37], RHIC [38], and he LHC [39–47], and he la es compa isons o hese measu emen s wi h heo e ical p edic ions demon- s a e he impo ance o con ibu ions beyond NLO ixed- o de calcula ions, namely esumma ions o ma ched pa on showe s. Howe e , he p ecise con ibu ions o he pe u - ba i e aspec o he je , as well as he had oniza ion and unde lying e en (UE) e ec s, emain unde in es iga ion. Inclusi e je measu emen s a low-pTas a unc ion o R (including a ios o je c oss sec ions, which allow pa ial cancella ion o expe imen al and heo e ical unce ain ies) will help cla i y hese con ibu ions and p o ide es s o bo h he pe u ba i e and nonpe u ba i e con ibu ions o he 2469-9985/2020/101(3)/034911(21) 034911-1 ©2020 CERN, o he ALICE Collabo a ion S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020) inclusi e je c oss sec ion. Mo eo e , hese measu emen s can be used o cons ain pa on dis ibu ion unc ions (PDFs) and he s ong coupling cons an αs[43,45,48–50]. This a icle epo s measu emen s o inclusi e je pTspec- a in pp and cen al Pb-Pb collisions a √sNN =5.02 TeV wi h he ALICE de ec o . Je s we e econs uc ed in he pseu- do apidi y ange |ηje |<0.7−R o je esolu ion pa ame- e s R=0.1–0.6inpp collisions and R=0.2 and R=0.4 in Pb-Pb collisions. In Pb-Pb collisions, we equi ed je s o con ain a leas one cha ged ack wi h pT>5–7 GeV/c (depending on he je R) in o de o iden i y ha d je candida es (a ising om la ge momen um- ans e sca e ings) in he la ge backg ound om combina o ial je s. In pp collisions, we epo he c oss sec ion bo h wi h and wi hou his bias. The ela i e je yields obse ed in Pb-Pb and pp collisions a e epo ed using hei scaled a io, RAA, and compa ed o se e al heo e ical p edic ions. II. EXPERIMENTAL SETUP AND DATASETS The ALICE de ec o [51,52] is a dedica ed hea y-ion expe imen loca ed a he La ge Had on Collide [53]. The analysis elied on he cen al acking sys em and he elec o- magne ic calo ime e (EMCal), as well as de ec o s o e en igge ing and cen ali y de e mina ion. The acking sys em consis s o a six-laye silicon inne acking sys em (ITS) wi h adial dis ance 3.9–43 cm om he beamline, and a gas ime p ojec ion chambe (TPC) wi h adial dis ance 85–247 cm om he beamline. The combined acking sys em spans |η|< 0.9 and ull azimu h, and acks we e measu ed in he ange 150 MeV/c<pT, ack <100 GeV/c. The EMCal consis s o a Pb-scin illa o sampling calo ime e spanning |η|<0.7 and 1.4<ϕ<3.3 in azimu h, loca ed a adial dis ance 4.36 m om he beamline [54]. I con ains 12 288 cells o ganized in an app oxima ely p ojec i e geome y ela i e o he in e ac- ion poin . The Molie e adius o he EMCal is M=3.2cm, and i s cells ha e a ans e se size o app oxima ely 6.0× 6.0cm(η ×ϕ ≈0.014 ×0.014). Each cell has a dep h o 24.6 cm, co esponding o app oxima ely 20 elec omagne ic adia ion leng hs and one had onic in e ac ion leng h. The epo ed Pb-Pb (pp) da a we e eco ded in 2015 (2017) a √sNN =5.02 TeV. The e en s we e collec ed using a minimum bias (MB) igge equi ing a coincidence hi in bo h o he V0 scin illa o s, loca ed a 2.8<η<5.1(V0-A) and −3.7<η<−1.7(V0-C)[55]. An accep ed e en was equi ed o ha e a p ima y e ex success ully econs uc ed wi hin −10 cm <z<10 cm o he in e ac ion poin and o sa is y se e al e ex quali y c i e ia. In Pb-Pb collisions, he cen ali y was de e mined using he V0 mul iplici ies [56–58]. Addi ionally, ou -o -bunch pileup was ejec ed using iming cu s as well as co ela ing ack mul iplici ies be ween se e al subde ec o s. We u ilized a sample o app oxima ely 4.6M 0–10% mos cen al Pb-Pb accep ed e en s (6.0μb−1) and 760M pp accep ed e en s (15.7nb−1). Recons uc ed acks we e gene ally equi ed o include a leas one hi in he silicon pixel de ec o (SPD) comp ising he i s wo laye s o he ITS and o ha e a leas 70 TPC space poin s and a leas 80% o he geome ically indable space poin s in he TPC. T acks wi hou any hi s in he SPD, bu o he wise sa is ying he acking c i e ia, we e e i wi h a cons ain o he p ima y e ex o he e en . Including his second class o acks ensu ed app oxima ely uni o m accep- ance in ϕ, while p ese ing simila pT esolu ion o acks wi h SPD hi s. T acks wi h pT, ack >150 MeV/cwe e ac- cep ed o e −0.9<η<0.9,0<ϕ<2π. The pe o mance o he de ec o was es ima ed wi h a model o he ALICE de ec o and i s esponse o pa icles using GEANT3. The acking e iciency in pp collisions, as es ima ed by PYTHIA8 MONASH 2013 [59] and he ALICE GEANT3 de ec o simula- ion, is app oxima ely 67% a pT, ack =150 MeV/c, ises o app oxima ely 84% a pT, ack =1GeV/c, and emains abo e 75% a highe pT. S udies o he cen ali y dependence o he acking e iciency in a HIJING [60] simula ion demons a ed ha he acking e iciency is app oxima ely 2% lowe in 0–10% cen al Pb-Pb collisions compa ed o pp collisions, independen o pT, ack. The momen um esolu ion δpT/pT was es ima ed om he co a iance ma ix o he ack i [52] using PYTHIA8MONASH 2013, and was app oxima ely 1% a pT, ack =1GeV/cand 4% a pT, ack =50 GeV/c. Recons uc ed EMCal clus e s we e buil by clus e ing EMCal cells wi h Ecell >100 MeV a ound a seed cell wi h Eseed >300 MeV, using a clus e ing algo i hm ha allows each clus e o ha e only a single local maximum. The highes -ene gy cell in a clus e was equi ed o sa is y a iming cu . Clus e s wi h la ge appa en ene gy bu anomalously small numbe o con ibu ing cells we e emo ed om he analysis, since hey a e belie ed o be due o in e ac ions o slow neu ons o highly ionizing pa icles in he a alanche pho odiodes [9]. The linea i y o he ene gy esponse o he EMCal was de e mined om elec on es beam da a, and a co ec ion o abou 7% a Eclus e =0.5 GeV bu negligible abo e Eclus e =3 GeV was applied o he clus e ene gies. A s udy using he pho on con e sion me hod demons a ed ha wi h his nonlinea i y co ec ion, he π0mass in Mon e Ca lo (MC) simula ions ma ches ha in pp da a wi hin 1%. Fo pp collisions, an addi ional co ec ion ob ained om a pho on con e sion analysis was used o educe he small emaining o se o he ene gy scale in da a and MC simula ions [61]. The ene gy esolu ion ob ained om elec on es beam da a was abou 15% a Eclus e =0.5GeV and be e han 5% abo e Eclus e =3GeV. Since he je ene gy is econs uc ed by combining acks and clus e s, one needs o accoun o he ac ha cha ged pa icles deposi ene gy in bo h he acking sys em and he EMCal, as in Re . [40]. In pa icula , all accep ed acks we e p opaga ed o he a e age showe dep h o he EMCal, =440 cm, and allowed o ma ch geome ically o a mos one clus e ; clus e s we e allowed o ha e mul iple ma ching acks. I a ack was ma ched wi hin pT-dependen h esholds anging om (η, ϕ)≈(0.037,0.084) a pT=0.15 GeV/c o (η, ϕ)≈(0.010,0.015) a pT=100 GeV/c, hen a had onic co ec ion was applied o he clus e : Ehadco clus e =Enonlinco clus e −E, whe e Enonlinco clus e is he nonlinea i y co ec ed clus e ene gy, and E=cip ack i, whe e ispans all acks ma ched o he clus e , p ack iis he ack h ee-momen um, and cis he speed o ligh . A e he abo e cu s and co ec ions we e pe o med, clus e s wi h Ehadco clus e >300 MeV we e accep ed. 034911-2 MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020) TABLE I. App oxima e alues cha ac e izing he je econs uc ion pe o mance o R=0.2andR=0.4inpp and Pb-Pb collisions. Fo cases wi h a leading ack equi emen , plead,ch T=5 GeV/cis used o R=0.2andplead,ch T=7 GeV/c o R=0.4. pp (plead,ch T>0 GeV/c)pp (plead,ch T>5/7 GeV/c)Pb-Pb(plead,ch T>5/7 GeV/c) pT,je 20 GeV/c100 GeV/c20 GeV/c100 GeV/c20 GeV/c100 GeV/c R=0.2 JES −29% −30% −18% −28% −23% −35% JER 27% 21% 19% 19% 35% 23% ε eco 98% 100% 86% 96% 86% 96% R=0.4 JES −30% −31% −14% −27% −6% −33% JER 23% 18% 15% 16% 77% 25% ε eco 99% 100% 82% 92% 82% 92% III. JET RECONSTRUCTION Je s we e econs uc ed wi h R=0.1–0.6inpp colli- sions and R=0.2,0.4 in Pb-Pb collisions using he an i-kT sequen ial ecombina ion algo i hm implemen ed in FAST- JET 3.2.1 [62,63] om he combina ion o cha ged pa i- cle acks and had onically co ec ed EMCal clus e s. We used he pT ecombina ion scheme, assuming EMCal clus- e s a e massless: p aw T,je =ipi T, ack +jpj T,clus e , whe e pT,clus e =Ehadco clus e /c. In Pb-Pb collisions, we sub ac ed he a e age combina- o ial backg ound ollowing he app oach in Re . [9]. The backg ound densi y ρwas de e mined in each e en and used o sub ac he a e age backg ound om each je in ha e en : p eco T,je =p aw T,je −ρA,whe e Ais he je a ea. The a - e age backg ound densi y in 0–10% cen al e en s is ypically ρ≈220–280 GeV/c, co esponding o ≈110–140 GeV/c o a R=0.4je .Inpp collisions, we did no sub ac he backg ound due o he unde lying e en , in o de o minimize he model dependence o he measu emen . Je s selec ed o he measu emen we e equi ed o sa is y se e al c i e ia in o de o be accep ed: (i) he cen e o he je mus be wi hin he iducial olume o he EMCal, i.e., a dis ance R≡(η)2+(ϕ)2 om any edge o he EMCal, (ii) he je mus no con ain any acks wi h pT, ack > 100 GeV/c, (iii) in Pb-Pb and applicable pp esul s, he je mus con ain a ack wi h pT, ack >5–7 GeV/c, depending on R, and (i ) in Pb-Pb collisions, he a ea o he je mus be A>0.6πR2.ThepT, ack <100 GeV/c equi emen emo ed only a small numbe o je s a la ge p eco T,je and has negligible bias o he p eco,max T,je selec ed in his analysis. The leading ack equi emen in oduces a small agmen a ion bias in he je sample, which may lead o a bias in he measu ed je supp ession. This e ec is discussed in Sec. VI and is es ima ed o ha e only a small e ec on he epo ed RAA.A la ge leading ack equi emen is needed o la ge Rsince he magni ude o backg ound luc ua ions inc eases wi h R. The a ea cu in Pb-Pb collisions was negligible excep a e y low p eco T,je , whe e i ejec s combina o ial je s. In Pb-Pb collisions, local luc ua ions in he backg ound smea he econs uc ed je momen um. To s udy je -by- je luc ua ions in he backg ound, we gene a ed a andom (η, ϕ) wi hin he iducial calo ime e accep ance in each e en and compa ed he sum o cons i uen s in a cone o adius R o he expec ed a e age backg ound in ha cone: δpT=cone (pT, ack +pT,clus e )−ρπR2. The wid h o he δpTdis ibu ion is a measu e o he size o he backg ound luc ua ions [64]. Fo R=0.2, he s anda d de ia ion o he δpTdis ibu ion is σδpT=6.5GeV/c, which g ows o σδpT= 16.1GeV/c o R=0.4. In he p esen analysis, he δpT dis ibu ions we e no explici ly used excep o de e mine he p eco T,je ange o u ilize in he analysis, which is discussed in Sec. IV. We e alua ed he pe o mance o ou je econs uc- ion s a egy by es ima ing he mean je ene gy scale shi , JES =(p eco T,je −p ue T,je )/p ue T,je , he je ene gy esolu- ion, JER =σ(p eco T,je )/p ue T,je , and he je econs uc ion e i- ciency, ε eco, omPYTHIA8MONASH 2013 and he ALICE de ec o simula ion. Table Ishows app oxima e alues o JES,JER,and ε eco o R=0.2 and R=0.4inpp and Pb-Pb collisions. The je ene gy scale shi is a long- ailed asymme ic dis ibu ion due o econs uc ion ine iciency (such as acking ine iciency) [10], and JES should be un- de s ood only as a ough cha ac e iza ion o his dis ibu ion. When a leading ack equi emen is imposed, he je econ- s uc ion e iciency and je ene gy scale shi a e p ima ily due o his equi emen in combina ion wi h he acking e iciency. No e ha he pp esponse app oxima ely, bu no exac ly, desc ibes he de ec o e ec s in je econs uc ion ele an o Pb-Pb collisions. In Pb-Pb collisions, he je e- cons uc ion pe o mance (including he e ec o backg ound luc ua ions) was de e mined by embedding pp MC e en s in o Pb-Pb da a, as desc ibed in de ail in Sec. IV.TheJER is app oxima ely cons an a ≈23% abo e p ue T,je =60 GeV/c o R=0.2, and de e io a es a lowe p ue T,je due o backg ound luc ua ions. As Rinc eases, he JER de e io a es due o he inc eased in luence o backg ound luc ua ions. IV. CORRECTIONS The econs uc ed p eco T,je spec um includes luc ua ions in he unde lying backg ound (in Pb-Pb collisions) and a a ie y o de ec o e ec s, including acking ine iciency, missing long-li ed neu al pa icles (n,K 0 L), and pa icle-ma e ial 034911-3 S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020) in e ac ions. We he e o e decon olu ed he econs uc ed je spec um wi h a esponse ma ix (RM) desc ibing he co e- la ion be ween p eco T,je and p ue T,je in o de o eco e he “ u h”- le el je spec um a he had on le el. In pp collisions, we gene a ed a RM using PYTHIA8 MONASH 2013 wi h he ull GEANT3 ALICE de ec o simu- la ion, based on he de ec o pe o mance in he ele an 2017 pp da a-collec ion pe iod. In Pb-Pb collisions, we gene a ed a RM by embedding PYTHIA e en s (wi h de ec o simula ion based on he de ec o pe o mance in he 2015 Pb-Pb da a- collec ion pe iod) in o Pb-Pb da a a e he de ec o -le el econs uc ion was un indi idually on bo h. The se o acks in he “hyb id” e en was aken as he sum o all acks in bo h e en s indi idually, while he se o EMCal clus e s we e eclus e ed om a combined pool o cells om bo h e en s. This embedding-based app oach, which uses eal backg ound, ensu es ha he de ec o esponse accu a ely e lec s he Pb-Pb esponse o he calo ime e , including pa icle o e laps in he calo ime e as well as he Pb-Pb pa icle composi ion, and ensu es he e ec o he had onic co ec ion is equi alen in da a and in he esponse. Mo eo e , i ensu es ha he co - ela ion be ween he local backg ound and he econs uc ed je due o local de ec o ine iciencies is accoun ed o . The u h-le el je was cons uc ed om he p ima y pa i- cles o he PYTHIA e en , de ined as all pa icles wi h a p ope decay leng h longe han 1 cm, excluding daugh e s o hese pa icles [65]. We co ec he je pT o include he “missing” long-li ed neu al pa icles. The de ec o -le el je in ppcollisions was cons uc ed om he PYTHIA acks and clus e s a de ec o le el. In Pb-Pb collisions, he de ec o -le el je was cons uc ed om he “hyb id” e en consis ing o bo h PYTHIA and Pb-Pb acks and clus e s a de ec o le el. To accoun o he dec eased acking e iciency in Pb-Pb collisions, we andomly ejec ed 2% o he PYTHIA acks in he Pb-Pb case, independen o pT. The a e age combina o ial backg ound was sub ac ed as in 0–10% cen al Pb-Pb da a: We compu ed he e en -by-e en ρcha ged using only Pb-Pb acks, and we applied he back- g ound scale ac o ob ained in Pb-Pb da a; we assume ha he combina o ial backg ound om he ppe en is negligible. In o de o ill he RM, we ma ched u h-le el je s o de ec o -le el je s by a geome ical ma ching p ocedu e. In ppcollisions, i an accep ed de ec o -le el je and an accep ed PYTHIA je we e wi hin R<0.6R, and hey we e bo h he closes je s o each o he , hen he je s we e ma ched, and hey con ibu e o he RM. In Pb-Pb collisions, i an accep ed hyb id je and an accep ed PYTHIA je we e wi hin R<1.5R, and hey we e bo h he closes je s o each o he , hen he je s we e ma ched, and hey con ibu e o he RM. The leading ack equi emen nulli ies he need in Pb-Pb collisions o u - he c i e ia such as a sha ed momen um ac ion equi emen in o de o gene a e accu a e ma ches. The RM was gene a ed wi h5GeV/cbin wid hs o p eco T,je and 10 GeV/cwid hs o p ue T,je and was no malized so as o p ese e he numbe o je s upon un olding. To pe o m he decon olu ion, we employed he SVD un olding algo i hm [66]using heROOUNFOLD package [67]. The egula iza ion pa ame e ksupp esses high- equency a ia ions in he un olded esul and was TABLE II. Minimum and maximum econs uc ed je pTused in he analysis as inpu o he decon olu ion p ocedu e. pp (GeV/c) Pb-Pb (GeV/c) p eco,min T,je p eco,max T,je p eco,min T,je p eco,max T,je R=0.2 7 130 20 120 R=0.4 10 130 35 120 selec ed by examining he so-called d- ec o dis ibu ion. S a is ical unce ain ies we e compu ed acco ding o MC pseudoexpe imen s wi hin ROOUNFOLD. The econs uc ed spec um was inpu o he un olding p ocedu e o e a ixed window o p eco T,je ∈[p eco,min T,je ,p eco,max T,je ], as illus a ed in Table II. In Pb-Pb collisions, each o hese p eco,min T,je co esponds o ≈2–3 ×σδpT, which, in combina ion wi h he leading cha ged had on equi emen , esul s in a sample la gely ee o combina o ial je s. A la ge alue o p eco,min T,je was used in Pb-Pb collisions in o de o minimize he impac o he combina o ial backg ound, which can des abilize he un olding p ocess. Any esidual combina o ial je s will s ill be un olded o low pTby he RM. Since unca ing he RM in p eco T,je loses he in o ma ion o he ac ion o u h-le el je s ha mig a e ou side o he measu ed de ec o -le el window, we co ec ed o his kinema ic e iciency. The un olded esul is hen epo ed in a ange o e which he inpu da a p o ides meaning ul cons ain s, ha is, a egion una ec ed by combina o ial je s and whe e he kinema ic e iciency is la ge han app oxima ely 80%. We co ec ed he un olded spec um o he ac ha he je inding p ocedu e ailed o econs uc a ce ain ac ion o je s. We compu ed he je econs uc ion e iciency as ε ecop ue T,je =Nma chedp ue T,je N u hp ue T,je , whe e Nma ched is he numbe o accep ed de ec o -le el je s ma ched o PYTHIA u h-le el je s ou o N u h accep ed u h- le el je s. In o de ha ε eco also includes he alse posi i e a e o accep ed de ec o -le el je s ha ha e no ma ching u h-le el je (which can occu i he u h-le el je was gene a ed sligh ly ou side o ou geome ical accep ance), he nume a o also con ains ma ches o u h-le el je s ou side o he EMCal iducial accep ance. No e ha ε eco does no explici ly include he bias o he leading cha ged had on e- qui emen , bu only he p obabili y o econs uc an accep ed je gi en a u h-le el je sa is ying he leading cha ged had on equi emen (when applicable). In o de o ε eco o be he je econs uc ion e iciency, he je ma ching e iciency mus be 100%. Howe e , in he Pb-Pb embedding en i onmen , his is di icul o achie e, since some c i e ia need o be imposed o supp ess combina o ial je s (in ou case, he leading ack equi emen ). The e o e, in he Pb-Pb case we used he je econs uc ion e iciency as de e mined om a pp simula ion alone (wi h 2% educed acking e iciency). The un olded solu ion was e i ied o be ma hema ically obus by pe o ming a e olding es and a “sel -closu e” es . The e olding es consis ed o gene a ing a RM ( om hal o he MC da a sample uns) and un olding he measu ed 034911-4 MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020) dis ibu ion, hen applying a RM ( om he o he hal o he MC da a sample) o he un olded esul , and compa ing he e olded solu ion o he measu ed dis ibu ion. The sel - closu e es consis ed o aking he ma ched de ec o -le el je spec um in he ull embedded sample and smea ing each da a poin wi h a Gaussian acco ding o he s a is ical unce ain ies o he measu ed da a. This spec um was hen un olded using he RM and compa ed he esul o he u h-le el PYTHIA je spec um. In bo h cases, consis ency was achie ed wi hin s a is ical unce ain ies. In Pb-Pb collisions, he un olded solu ion is e i ied o be physically co ec by a he mal model closu e es simila o ha in Re . [9]. The closu e es consis ed o pe o ming he en i e analysis on “hyb id” e en s con aining a PYTHIA e en and a he mal backg ound, in which “hyb id” je s we e clus e ed om he combina ion o PYTHIA de ec o -le el pa - icles and he mal backg ound pa icles. The backg ound was modeled by gene a ing Npa icles om a Gaussian, wi h pT aken om a dis ibu ion, (pT;β)∼pTe−pT/β , whe e he ee pa ame e s N,σ N,β we e ixed o oughly i he δpT dis ibu ion in 0–10% Pb-Pb da a. The es consis ed o con- s uc ing he hyb id de ec o -le el je spec um, building he RM, un olding he hyb id je s—and compa ing he spec um o he u h-le el PYTHIA spec um. Since he backg ound does no ha e any je componen , his es is able o e i y whe he he analysis p ocedu e indeed eco e s he je spec um and is no con amina ed by combina o ial je s. These es s alida ed he analysis p ocedu e wi hin app oxima ely 5% o R=0.2 wi h plead,ch T=5GeV/cand R=0.4 wi h plead,ch T=7GeV/c. V. SYSTEMATIC UNCERTAINTIES Following Re . [9], we ca ego ized wo classes o sys em- a ic unce ain ies: co ela ed unce ain ies and shape unce - ain ies. Co ela ed unce ain ies encompass de ec o e ec s such as unce ain y on he acking e iciency and unce ain y on he EMCal esponse, which a e app oxima ely ully pos- i i ely co ela ed among all pT,je bins. Shape unce ain ies e e o sys ema ic un olding unce ain ies, which al e he shape o he inal pT,je spec um. The dominan sys ema ic unce ain ies in his analysis a e he unce ain y in he acking e iciency and he sys ema ic unce ain y in he un olding p ocedu e. No e ha in gene al he ollowing unce ain ies desc ibe unce ain ies on he je yield, no on he je pTscale. A. Co ela ed unce ain ies The dominan co ela ed unce ain y is he unce ain y on he modeling o he acking e iciency, since co ec ing o unmeasu ed acks has a majo e ec on he un olding p ocedu e. Fo he ack selec ion desc ibed in Sec. II, he unce ain y on he acking e iciency is app oxima ely 4%, as es ima ed om a ia ion in he ack selec ion pa ame e s and a ia ion in he ITS-TPC ma ching equi emen s. In o de o assign a sys ema ic unce ain y o he inal esul , we cons uc ed a RM using he same echniques as o he inal esul excep wi h an addi ional 4% o PYTHIA acks andomly ejec ed in je inding ( o Pb-Pb, his is in addi ion o he 2% ejec ion used o he main esul ). The je econs uc ion e iciency was also compu ed wi h his ex a 4% supp ession applied. This modi ied RM was hen used o un old he same measu ed spec um as used o he main esul . This a ied esul was co ec ed o he je econs uc ion e iciency and compa ed o he main esul , wi h he di e ences in each bin aken as he unce ain y. Addi ionally, he unce ain y due o he acking pT esolu ion was app oxima ely 1%. Sys ema ic unce ain ies due o he modeling o he EMCal esponse we e included in se e al ways. In o de o desc ibe he unce ain y in he MC desc ip ion o he EMCal had onic esponse, he sub ac ed ene gy in he had onic co ec ion was a ied om 100% o 70% o he ma ched ack mo- men um. Mo eo e , a sys ema ic unce ain y associa ed wi h he ack-ma ching c i e ia was included by changing he pT- dependen ack-ma ching c i e ia o pT-independen c i e ia η < 0.015,ϕ<0.03. These wo unce ain ies we e com- bined in quad a u e o o m he unce ain y on he EMCal had onic co ec ion p ocedu e. In o de o desc ibe he un- ce ain y in he MC desc ip ion o he EMCal elec omag- ne ic esponse, in he pp case he pho on con e sion based nonlinea i y co ec ion was swi ched o . These a ia ions we e indi idually pe o med bo h in he RM and he da a, and he sys ema ic unce ain y was e alua ed by compa ing he modi ied un olded esul o he main esul . In he Pb-Pb case, he e is an addi ional unce ain y due o he ac ha he MC does no exac ly desc ibe he clus e ene gy nonlinea i y. To accoun o his, di e en clus e nonlinea i y co ec ions a e ypically applied o da a and MC; howe e , in he Pb-Pb embedding p ocedu e, he clus e s a e mix u es o da a and MC cells. The main esul was compu ed by applying he da a nonlinea i y pa ame iza ion o he mixed da a and MC cells in he embedding p ocedu e. The e o e, we applied he MC nonlinea i y pa ame iza ion as a sys ema ic a ia ion. In Pb-Pb collisions o R=0.4, he unce ain ies on he EMCal nonlinea i y co ec ion and ack ma ching p ocedu e a e la ge, p ima ily due o un olding e ec s, which we do no decouple in he e alua ion o he co ela ed unce ain ies. We included also a sys ema ic unce ain y associa ed wi h he choice o je ma ching p ocedu e. Fo pp, he geome ical ma ching dis ance was a ied om 0.4R o 0.8R(excep o R=0.1 om0.2R o 0.9R), which esul ed in an unce ain y o less han 1% (1.5%). Fo Pb-Pb, we a ied om a pu e geome ical ma ching o an MC- ac ion based app oach, in which a sha ed momen um ac ion equi emen ensu es ha he ma ched je con ains mo e han 50% o he pTo he MC je . This ga e an unce ain y o 2–6%. We included also a sys ema ic unce ain y associa ed wi h he model-dependen eliance on PYTHIA o un old he spec a. In pp collisions, we eweigh ed he esponse ma ix acco d- ing o he je angula i y (g=ipT,i i/pT,je , whe e i= √η2+ϕ2is he dis ance o he i h cons i uen om he je axis) a u h le el. Speci ically, we e-weigh ed he esponse ma ix such ha he 50% la ges angula i y je s we e weigh ed an addi ional ±30% ela i e o he 50% lowes angula i y je s. This con ibu ed an unce ain y anging om ≈2% o 7% depending on he je R, and oughly independen o pT.The same unce ain ies we e aken o Pb-Pb collisions. Tables III and IV illus a e he con ibu ions o he a ious co ela ed unce ain ies o pp and Pb-Pb collisions. These 034911-5 S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020) TABLE III. Summa y o co ela ed sys ema ic unce ain ies on he pp je spec a wi hou a leading ack bias, o selec R. The columns pmin T,je and pmax T,je a e he unce ain ies a he minimum and maximum pT,je bin. Rela i e unce ain y (%) R=0.2R=0.6 pp pmin T,je pmax T,je A g. pmin T,je pmax T,je A g. T acking e iciency 5.9 9.1 7.7 9.4 8.9 9.0 T ack pT esolu ion 1.0 1.0 1.0 1.0 1.0 1.0 EMCal nonlinea i y 0.5 0.5 0.5 1.0 0.9 1.0 Had onic co ec ion 0.2 1.2 0.5 1.2 2.1 0.9 Je ma ching 0.1 0.0 0.0 0.2 0.2 0.2 PYTHIA agmen a ion 0.5 1.0 0.4 3.1 5.6 5.8 To al co . unce ain y 6.0 9.3 7.8 10.1 10.8 10.8 unce ain ies a e expec ed o be la gely independen , so we summed hei unce ain ies in quad a u e. B. Shape unce ain ies In o de o assign a shape unce ain y a ising om he un olding egula iza ion p ocedu e, we pe o med se e al sys- ema ic a ia ions: (1) Va ia ion o he un olding algo i hm: We un olded wi h a Bayes-inspi ed i e a i e un olding algo i hm [68]. (2) Va ia ion o he egula iza ion pa ame e : In he SVD un olding, we a ied he egula iza ion pa ame e k one uni abo e and below he nominal solu ion. (3) Va ia ion o he p io : The SVD algo i hm equi es a p io dis ibu ion as inpu , which o he main esul is he p ojec ion o he RM on o he u h axis (be o e no maliza ion). We a ied his inpu p io ei he by scaling he main p io by p±0.5 To eplacing i wi h a je c oss sec ion p oduced by POWHEG o he un olded main esul i sel . (4) Va ia ion o he inpu ange: Fo Pb-Pb (pp) collisions, we a ied he measu ed inpu ange ±5( +5 −3)GeV/c a ound he nominal alue o each R. The o al shape unce ain y is hen he s anda d de ia ion o he a ia ions, 3 i=1σ2 i/4, whe e σiis he sys ema ic due o a single a ia ion, since hey each comp ise independen mea- su emen s o he same unde lying sys ema ic unce ain y in he egula iza ion. Tables Vand VI illus a e he con ibu ions o he a ious shape unce ain ies o ppand Pb-Pb collisions. C. Unce ain ies on he je c oss-sec ion a io We compu ed he co ela ed sys ema ic unce ain ies on he pp je c oss-sec ion a io by making he same a ia ions as in Sec. VA on bo h spec a simul aneously and compa ed he a ied je c oss-sec ion a io o he main esul . This esul ed in signi ican cancella ion o he co ela ed unce ain ies be- ween he nume a o and denomina o , as can be seen in Sec. VI. We compu ed he shape sys ema ic unce ain ies by adding he single spec a shape unce ain ies in quad a u e. I is impo an o no e ha he s a is ical unce ain ies o he nume a o and denomina o a e pa ially co ela ed, due o e o p opaga ion h ough he un olding p ocedu e. We did no , howe e , ake his in o accoun . This may esul in a sligh ly conse a i e s a is ical unce ain y es ima ion, since he e may be signi ican cancella ion be ween he wo adii. Addi ionally, we did no use s a is ically independen samples o o m he a io, and so he nume a o and de- nomina o a e s a is ically co ela ed wi h each o he , which may lead o u he sligh o e es ima ion o he s a is ical unce ain ies. TABLE IV. Summa y o co ela ed sys ema ic unce ain ies on he Pb-Pb je spec a, o selec Rand plead,ch T h esholds. The columns pmin T,je and pmax T,je a e he unce ain ies a he minimum and maximum pT,je bin. Rela i e unce ain y (%) R=0.2,5 GeV/cR=0.4,7 GeV/c Pb-Pb pmin T,je pmax T,je A g. pmin T,je pmax T,je A g. T acking e iciency 5.8 8.9 8.0 9.9 9.8 9.8 T ack pT esolu ion 1.0 1.0 1.0 1.0 1.0 1.0 EMCal nonlinea i y 2.1 1.1 1.6 11.4 7.9 9.5 Had onic co ec ion 0.8 5.9 2.0 12.8 9.9 12.4 Je ma ching 2.0 2.0 2.0 6.0 2.0 2.8 PYTHIA agmen a ion 0.8 3.6 2.0 2.8 5.1 3.8 To al co . unce ain y 6.7 11.6 9.2 20.9 16.9 19.5 034911-6 MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020) TABLE V. Summa y o shape sys ema ic unce ain ies on he pp je spec a wi hou a leading ack bias, o selec R. The columns pmin T,je and pmax T,je a e he unce ain ies a he minimum and maximum pT,je bin. Rela i e unce ain y (%) R=0.2,0 GeV/cR=0.6,0 GeV/c pp pmin T,je pmax T,je A g. pmin T,je pmax T,je A g. Un olding me hod 0.0 16.0 3.4 2.6 16.0 4.5 Reg. pa ame e 0.7 2.4 1.3 1.0 3.5 2.1 P io 1.3 0.8 0.9 0.9 3.7 2.0 Inpu pT ange 0.8 3.3 1.3 0.4 3.2 1.4 To al shape unce ain y 0.8 8.3 2.2 1.5 8.5 3.0 VI. RESULTS A. Inclusi e je spec a 1. pp We epo he pp ull je c oss sec ion o R= 0.1,0.2,0.3,0.4,0.5,0.6inFig.1(le ). The c oss sec ions a e epo ed di e en ially in pT,je and ηje as d2σje dpT,je dηje = 1 L d2N dpT,je dηje ,whe e we expe imen ally measu ed he yield d2N dpT,je dηje and he in eg a ed luminosi y L[55]. The unce ain y on he luminosi y is 2.1%. The measu ed je c oss sec ions we e un olded o de ec o and backg ound e ec s and a e epo ed a he had on-le el. The c oss sec ions we e co ec ed o he kinema ic e iciency and je econs uc ion e iciency, as well as he pa ial azimu hal accep ance o he EMCal and he e ex e iciency. No e ha a leading ack equi emen was no imposed o he esul s in Fig. 1. We compa e he pp inclusi e je c oss sec ion o wo heo e ical calcula ions in Fig. 1( igh ). The p edic ions de- no ed NLO+NLL+NP a e analy ical p edic ions a NLO wi h esumma ion o je Rloga i hms and h eshold loga i hms o NLL accu acy, pe o med in a igo ous QCD ac o iza- ion scheme [28,30,31]. The e ec o unaccoun ed highe o de co ec ions was e alua ed by a ious scale a ia ions and is included as a sys ema ic unce ain y. A co ec ion o had oniza ion and mul ipa on in e ac ion (MPI) e ec s is applied o his p edic ion, based on PYTHIA8 une A14 and is shown in Fig. 2. These nonpe u ba i e (NP) e ec s become la ge o low pT,je a bo h small and la ge R, whe e sys ema ic unce ain ies in his co ec ion (beyond he scope o his a icle) a e likely c i ical. The p edic ions use PDF se CT14nlo. These p edic ions a e seen o be gene ally consis en wi h he da a, excep a low pTand small R. This ension may be due o he model-dependen NP co ec ion, which is la ge in his egion. The expe imen al da a p esen ed in Fig. 1, which co e a la ge ange o Rdown o low pTand he e o e span a wide ange o NP e ec s ( om had oniza ion domina ed a small R o MPI domina ed a la ge R, as seen in Fig. 2), can be used o u he cons ain NP e ec s in pp collisions. This is o ele ance bo h o pp QCD physics and o in e p e ing modi ica ions in hea y-ion collisions, which a e ypically s onges a low pT. The p edic ions deno ed POWHEG+PYTHIA8 consis o a MC pa on-showe -based model using NLO calcula ions om POWHEG [69] ma ched o a pa on showe and had oniza ion om PYTHIA8 une A14.1Two heo e ical unce ain ies we e compu ed o hese p edic ions, bo h in ega d o he POWHEG e en gene a ion: PDF unce ain y, compu ed as in Re . [73], and scale unce ain y, which was compu ed by a ying he 1The POWHEG e e ence was p oduced by POWHEG-BOX-V2a √s=5.02 TeV ia he je pai p oduc ion p ocess [69–71]. PDF se CT14nlo was used, along wi h he se ings bo nk min =1and bo nsupp ac =70. PYTHIA 8.2 une A14 NNPDF2.3LO was used o he pa on showe , which is uned wi h ATLAS pp collisions a √sNN =7 TeV using unde lying e en obse ables, je subs uc- u e obse ables, and se e al o he obse ables, no including he inclusi e je c oss sec ion [72]. Me ging wi h PYTHIA was done as in Re . [73]. The same se o p ima y pa icles was used as desc ibed ea lie [65]. TABLE VI. Summa y o shape sys ema ic unce ain ies on he Pb-Pb je spec a, o selec Rand plead,ch T h esholds. The columns pmin T,je and pmax T,je a e he unce ain ies a he minimum and maximum pT,je bin. Rela i e unce ain y (%) R=0.2,5 GeV/cR=0.4,7 GeV/c Pb-Pb pmin T,je pmax T,je A g. pmin T,je pmax T,je A g. Un olding me hod 7.7 10.0 5.4 30.3 2.5 18.2 Reg. pa ame e 4.2 8.7 4.4 24.9 20.6 23.1 P io 1.5 6.7 2.4 2.3 8.3 4.2 Inpu pT ange 0.4 0.9 0.6 1.5 1.7 1.4 To al shape unce ain y 4.4 7.4 3.8 19.6 11.2 15.5 034911-7 S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020) FIG. 1. Le : Un olded pp ull je c oss sec ion a √s=5.02 TeV o R=0.1–0.6. No leading ack equi emen is imposed. Righ : Ra io o NLO+NLL+NP and POWHEG+PYTHIA8 une A14 p edic ions o he measu ed da a. The sys ema ic unce ain ies in he a io a e deno ed by boxes and a e he quad a ic sum o he sys ema ic unce ain ies in da a and he p edic ions. No e ha no sys ema ic unce ain ies o he nonpe u ba i e co ec ion in he NLO+NLL+NP p edic ion we e included. eno maliza ion and ac o iza ion scales. The o al heo e ical unce ain y on he c oss sec ion was ob ained by adding hese wo con ibu ions in quad a u e. No e ha la ge nonpe u ba- i e e ec s, simila o Fig. 2, a e implici ly p esen in his FIG. 2. Nonpe u ba i e co ec ion ac o applied o pa on-le el NLO+NLL p edic ions, ob ained om PYTHIA8 une A14 as he a io o he inclusi e je spec um a had on-le el wi h MPI compa ed o pa on-le el wi hou MPI. p edic ion as well. The POWHEG+PYTHIA8 p edic ions a e consis en wi h he measu ed da a o all Rand pT,je . Figu e 1 does no include p edic ions by PYTHIA alone, since i is well es ablished ha NLO con ibu ions a e necessa y o ob ain he pp inclusi e je c oss sec ion [32,39]. Figu e 3shows he pp je c oss sec ion a io o a ious R, buil om he spec a in Fig. 1. The op wo panels show he a ios o R=0.2 o o he adii, and he bo om wo panels show he a ios o R=0.1 o o he adii. The le panels also include compa isons o POWHEG+PYTHIA8, and he igh panels include compa isons o NLO+NLL+NP. Co ela ed unce ain ies la gely cancel [40,74], which allows his obse able o elucida e highe p ecision e ec s com- pa ed o he inclusi e je c oss sec ion. The sys ema ic un- ce ain ies on he POWHEG+PYTHIA8 p edic ion la gely can- cel as well, and he esul ing high-p ecision compa isons show ha he c oss-sec ion a ios a e gene ally well-desc ibed by POWHEG+PYTHIA8. The sys ema ic unce ain ies in he NLO+NLL+NP p edic ion, howe e , do no subs an ially cancel, because he scale a ia ions include a ia ion o so e scales which a e sensi i e o nonpe u ba i e e ec s; he NLO+NLL+NP p edic ions a e consis en wi h he measu ed da a wi hin he size o hese la ge heo e ical unce ain ies. 2. Pb-Pb We epo he 0–10% cen al Pb-Pb je spec a o R=0.2 and R=0.4inFig.4. The spec a a e epo ed di e en ially in pT,je and ηje as 1 TAA 1 Ne en d2NAA je dpT,je dηje ,whe e TAA≡Ncoll σNN inel is he a io o he numbe o bina y nucleon-nucleon collisions o he inelas ic nucleon-nucleon c oss sec ion, compu ed in a Glaube model o be TAA=23.07 ±0.44 (sys) mb−1 o 034911-8 MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020) [12] L. Adamczyk e al. (STAR Collabo a ion), Measu emen s o je quenching wi h semi-inclusi e had on+je dis ibu ions in Au +Au collisions a √sNN =200 GeV, Phys. Re . C 96, 024905 (2017). [13] G. Aad e al. 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R. Caianiello” dell’Uni e si à and G uppo Collega o INFN, Sale no, I aly 31Dipa imen o DISAT del Poli ecnico and Sezione INFN, Tu in, I aly 32Dipa imen o di Scienze e Inno azione Tecnologica dell’Uni e si à del Piemon e O ien ale and INFN Sezione di To ino, Alessand ia, I aly 33Dipa imen o In e a eneo di Fisica “M. Me lin” and Sezione INFN, Ba i, I aly 34Eu opean O ganiza ion o Nuclea Resea ch (CERN), Gene a, Swi ze land 35Facul y o Elec ical Enginee ing, Mechanical Enginee ing and Na al A chi ec u e, Uni e si y o Spli , Spli , C oa ia 36Facul y o Enginee ing and Science, Wes e n No way Uni e si y o Applied Sciences, Be gen, No way 37Facul y o Nuclea Sciences and Physical Enginee ing, Czech Technical Uni e si y in P ague, P ague, Czech Republic 38Facul y o Science, P. J. Ša á ik Uni e si y, Košice, Slo akia 39F ank u Ins i u e o Ad anced S udies, Johann Wol gang Goe he-Uni e si ä F ank u , F ank u , Ge many 40Gangneung-Wonju Na ional Uni e si y, Gangneung, Republic o Ko ea 41Gauha i Uni e si y, Depa men o Physics, Guwaha i, India 42Helmhol z-Ins i u ü S ahlen- und Ke nphysik, Rheinische F ied ich-Wilhelms-Uni e si ä Bonn, Bonn, Ge many 43Helsinki Ins i u e o Physics (HIP), Helsinki, Finland 44High Ene gy Physics G oup, Uni e sidad Au ónoma de Puebla, Puebla, Mexico 45Hi oshima Uni e si y, Hi oshima, Japan 46Hochschule Wo ms, Zen um ü Technologie ans e und Telekommunika ion (ZTT), Wo ms, Ge many 47Ho ia Hulubei Na ional Ins i u e o Physics and Nuclea Enginee ing, Bucha es , Romania 48Indian Ins i u e o Technology Bombay (IIT), Mumbai, India 49Indian Ins i u e o Technology Indo e, Indo e, India 034911-19 S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020) 50Indonesian Ins i u e o Sciences, Jaka a, Indonesia 51INFN, Labo a o i Nazionali di F asca i, F asca i, I aly 52INFN, Sezione di Ba i, Ba i, I aly 53INFN, Sezione di Bologna, Bologna, I aly 54INFN, Sezione di Caglia i, Caglia i, I aly 55INFN, Sezione di Ca ania, Ca ania, I aly 56INFN, Sezione di Pado a, Pado a, I aly 57INFN, Sezione di Roma, Rome, I aly 58INFN, Sezione di To ino, Tu in, I aly 59INFN, Sezione di T ies e, T ies e, I aly 60Inha Uni e si y, Incheon, Republic o Ko ea 61Ins i u de Physique Nucléai e d’O say (IPNO), Ins i u Na ional de Physique Nucléai e e de Physique des Pa icules (IN2P3/CNRS), Uni e si é de Pa is-Sud, Uni e si é Pa is-Saclay, O say, F ance 62Ins i u e o Nuclea Resea ch, Academy o Sciences, Moscow, Russia 63Ins i u e o Suba omic Physics, U ech Uni e si y/Nikhe , U ech , Ne he lands 64Ins i u e o Expe imen al Physics, Slo ak Academy o Sciences, Košice, Slo akia 65Ins i u e o Physics, Homi Bhabha Na ional Ins i u e, Bhubaneswa , India 66Ins i u e o Physics o he Czech Academy o Sciences, P ague, Czech Republic 67Ins i u e o Space Science (ISS), Bucha es , Romania 68Ins i u ü Ke nphysik, Johann Wol gang Goe he-Uni e si ä F ank u , F ank u , Ge many 69Ins i u o de Ciencias Nuclea es, Uni e sidad Nacional Au ónoma de México, Mexico Ci y, Mexico 70Ins i u o de Física, Uni e sidade Fede al do Rio G ande do Sul (UFRGS), Po o Aleg e, B azil 71Ins i u o de Física, Uni e sidad Nacional Au ónoma de México, Mexico Ci y, Mexico 72iThemba LABS, Na ional Resea ch Founda ion, Some se Wes , Sou h A ica 73Johann-Wol gang-Goe he Uni e si ä F ank u Ins i u ü In o ma ik, Fachbe eich In o ma ik und Ma hema ik, F ank u , Ge many 74Join Ins i u e o Nuclea Resea ch (JINR), Dubna, Russia 75Ko ea Ins i u e o Science and Technology In o ma ion, Daejeon, Republic o Ko ea 76KTO Ka a ay Uni e si y, Konya, Tu key 77Labo a oi e de Physique Suba omique e de Cosmologie, Uni e si é G enoble-Alpes, CNRS-IN2P3, G enoble, F ance 78Law ence Be keley Na ional Labo a o y, Be keley, Cali o nia, USA 79Lund Uni e si y Depa men o Physics, Di ision o Pa icle Physics, Lund, Sweden 80Nagasaki Ins i u e o Applied Science, Nagasaki, Japan 81Na a Women’s Uni e si y (NWU), Na a, Japan 82Na ional and Kapodis ian Uni e si y o A hens, School o Science, Depa men o Physics, A hens, G eece 83Na ional Cen e o Nuclea Resea ch, Wa saw, Poland 84Na ional Ins i u e o Science Educa ion and Resea ch, Homi Bhabha Na ional Ins i u e, Ja ni, India 85Na ional Nuclea Resea ch Cen e , Baku, Aze baijan 86Na ional Resea ch Cen e Ku cha o Ins i u e, Moscow, Russia 87Niels Boh Ins i u e, Uni e si y o Copenhagen, Copenhagen, Denma k 88Nikhe , Na ional Ins i u e o Suba omic Physics, Ams e dam, Ne he lands 89NRC Ku cha o Ins i u e IHEP, P o ino, Russia 90NRC Ku cha o Ins i u e ITEP, Moscow, Russia 91NRNU Moscow Enginee ing Physics Ins i u e, Moscow, Russia 92Nuclea Physics G oup, STFC Da esbu y Labo a o y, Da esbu y, Uni ed Kingdom 93Nuclea Physics Ins i u e o he Czech Academy o Sciences, ˇ Rež u P ahy, Czech Republic 94Oak Ridge Na ional Labo a o y, Oak Ridge, Tennessee, USA 95Ohio S a e Uni e si y, Columbus, Ohio, USA 96Pe e sbu g Nuclea Physics Ins i u e, Ga china, Russia 97Physics Depa men , Facul y o Science, Uni e si y o Zag eb, Zag eb, C oa ia 98Physics Depa men , Panjab Uni e si y, Chandiga h, India 99Physics Depa men , Uni e si y o Jammu, Jammu, India 100Physics Depa men , Uni e si y o Rajas han, Jaipu , India 101Physikalisches Ins i u , Ebe ha d-Ka ls-Uni e si ä Tübingen, Tübingen, Ge many 102Physikalisches Ins i u , Rup ech -Ka ls-Uni e si ä Heidelbe g, Heidelbe g, Ge many 103Physik Depa men , Technische Uni e si ä München, Munich, Ge many 104Poli ecnico di Ba i, Ba i, I aly 105Resea ch Di ision and Ex eMe Ma e Ins i u e EMMI, GSI Helmhol zzen um ü Schwe ionen o schung GmbH, Da ms ad , Ge many 106Rudje Boško i´c Ins i u e, Zag eb, C oa ia 107Russian Fede al Nuclea Cen e (VNIIEF), Sa o , Russia 034911-20 MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020) 108Saha Ins i u e o Nuclea Physics, Homi Bhabha Na ional Ins i u e, Kolka a, India 109School o Physics and As onomy, Uni e si y o Bi mingham, Bi mingham, Uni ed Kingdom 110Sección Física, Depa amen o de Ciencias, Pon i icia Uni e sidad Ca ólica del Pe ú, Lima, Pe u 111Shanghai Ins i u e o Applied Physics, Shanghai, China 112S . Pe e sbu g S a e Uni e si y, S . Pe e sbu g, Russia 113S e an Meye Ins i u ü Suba oma e Physik (SMI), Vienna, Aus ia 114SUBATECH, IMT A lan ique, Uni e si é de Nan es, CNRS-IN2P3, Nan es, F ance 115Su ana ee Uni e si y o Technology, Nakhon Ra chasima, Thailand 116Technical Uni e si y o Košice, Košice, Slo akia 117Technische Uni e si ä München, Excellence Clus e “Uni e se,” Munich, Ge many 118The Hen yk Niewodniczanski Ins i u e o Nuclea Physics, Polish Academy o Sciences, C acow, Poland 119The Uni e si y o Texas a Aus in, Aus in, Texas, USA 120Uni e sidad Au ónoma de Sinaloa, Culiacán, Mexico 121Uni e sidade de São Paulo (USP), São Paulo, B azil 122Uni e sidade Es adual de Campinas (UNICAMP), Campinas, B azil 123Uni e sidade Fede al do ABC, San o And e, B azil 124Uni e si y o Cape Town, Cape Town, Sou h A ica 125Uni e si y o Hous on, Hous on, Texas, USA 126Uni e si y o Jy äskylä, Jy äskylä, Finland 127Uni e si y o Li e pool, Li e pool, Uni ed Kingdom 128Uni e si y o Science and Techonology o China, He ei, China 129Uni e si y o Sou h-Eas e n No way, Tonsbe g, No way 130Uni e si y o Tennessee, Knox ille, Tennessee, USA 131Uni e si y o he Wi wa e s and, Johannesbu g, Sou h A ica 132Uni e si y o Tokyo, Tokyo, Japan 133Uni e si y o Tsukuba, Tsukuba, Japan 134Uni e si é Cle mon Au e gne, CNRS/IN2P3, LPC, Cle mon -Fe and, F ance 135Uni e si é de Lyon, Uni e si é Lyon 1, CNRS/IN2P3, IPN-Lyon, Villeu banne, Lyon, F ance 136Uni e si é de S asbou g, CNRS, IPHC UMR 7178, F-67000 S asbou g, F ance, S asbou g, F ance 137Uni e si é Pa is-Saclay Cen e d’E udes de Saclay (CEA), IRFU, Dépa men de Physique Nucléai e (DPhN), Saclay, F ance 138Uni e si à degli S udi di Foggia, Foggia, I aly 139Uni e si à degli S udi di Pa ia, Pa ia, I aly 140Uni e si à di B escia, B escia, I aly 141Va iable Ene gy Cyclo on Cen e, Homi Bhabha Na ional Ins i u e, Kolka a, India 142Wa saw Uni e si y o Technology, Wa saw, Poland 143Wayne S a e Uni e si y, De oi , Michigan, USA 144Wes älische Wilhelms-Uni e si ä Müns e , Ins i u ü Ke nphysik, Müns e , Ge many 145Wigne Resea ch Cen e o Physics, Budapes , Hunga y 146Yale Uni e si y, New Ha en, Connec icu , USA 147Yonsei Uni e si y, Seoul, Republic o Ko ea aP esen add ess: Dipa imen o DET del Poli ecnico di To ino, Tu in, I aly. bP esen add ess: M. V. Lomonoso Moscow S a e Uni e si y, D. V. Skobel syn Ins i u e o Nuclea , Physics, Moscow, Russia. cDeceased. dP esen add ess: Depa men o Applied Physics, Aliga h Muslim Uni e si y, Aliga h, India. eP esen add ess: Ins i u e o Theo e ical Physics, Uni e si y o W oclaw, Poland. 034911-21