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. (ATLAS Collabo a ion), Measu emen o he je
adius and ans e se momen um dependence o inclusi e je
supp ession in lead-lead collisions a √sNN =2.76 TeV wi h
he ATLAS de ec o , Phys. Le . B 719,220 (2013).
[14] M. Aaboud e al. (ATLAS Collabo a ion), Measu emen o
he nuclea modi ica ion ac o o inclusi e je s in Pb+Pb
collisions a √sNN =5.02 TeV wi h he ATLAS de ec o , Phys.
Le . B 790,108 (2019).
[15] V. Khacha yan e al. (CMS Collabo a ion), Measu emen o in-
clusi e je c oss sec ions in pp and Pb-Pb collisions a √sNN =
2.76TeV, Phys. Re . C 96,015202 (2017).
[16] S. Acha ya e al. (ALICE Collabo a ion), Medium modi ica ion
o he shape o small- adius je s in cen al Pb-Pb collisions a
√sNN =2.76 TeV, J. High Ene gy Phys. 10 (2018)139.
[17] S. Cha chyan e al. (CMS Collabo a ion), Obse a ion and
s udies o je quenching in Pb-Pb collisions a √sNN =
2.76 TeV, Phys.Re .C84,024906 (2011).
[18] M. Aaboud e al. (ATLAS Collabo a ion), Measu emen o je
agmen a ion in Pb-Pb and pp collisions a √sNN =5.02 TeV
wi h he ATLAS de ec o , Phys.Re .C98,024908 (2018).
[19] K. M. Bu ke e al. (JET Collabo a ion), Ex ac ing he je
anspo coe icien om je quenching in high-ene gy hea y-
ion collisions, Phys. Re . C 90,014909 (2014).
[20] G.-Y. Qin and X.-N. Wang, Je quenching in high-ene gy hea y-
ion collisions, In . J. Mod. Phys. E 24,1530014 (2015).
[21] J.-P. Blaizo and Y. Meh a -Tani, Je s uc u e in hea y ion
collisions, In . J. Mod. Phys. E 24,1530012 (2015).
[22] A. Majumde and M. an Leeuwen, The heo y and phe-
nomenology o pe u ba i e QCD based je quenching, P og.
Pa . Nucl. Phys. 66,41 (2011).
[23] J.-W. Qiu, F. Ringe , N. Sa o, and P. Zu i a, Fac o iza ion o Je
C oss Sec ions in Hea y-Ion Collisions, Phys. Re . Le . 122,
252301 (2019).
[24] R. Elaya alli and K. Zapp, Medium esponse in JEWEL and i s
impac on je shape obse ables in hea y ion collisions, J. High
Ene gy Phys. 07 (2017)141.
[25] Y. He, S. Cao, W. Chen, T. Luo, L.-G. Pang, and X.-N. Wang,
In e playing mechanisms behind single inclusi e je supp es-
sion in hea y-ion collisions, Phys. Re . C 99,054911 (2019).
[26] M. Dasgup a, F. D eye , G. P. Salam, and G. Soyez, Small-
adius je s o all o de s in QCD, J. High Ene gy Phys. 04 (2015)
039.
[27] M. Dasgup a, F. A. D eye , G. P. Salam, and G. Soyez, Inclusi e
je spec um o small- adius je s, J. High Ene gy Phys. 06
(2016)057.
[28] Z.-B. Kang, F. Ringe , and I. Vi e , The semi-inclusi e je
unc ion in SCET and small adius esumma ion o inclusi e
je p oduc ion, J. High Ene gy Phys. 10 (2016)125.
[29] Z.-B. Kang, F. Ringe , and I. Vi e , Inclusi e p oduc ion o
small adius je s in hea y-ion collisions, Phys. Le . B 769,242
(2017).
[30] X. Liu, S.-O. Moch, and F. Ringe , Th eshold and Je Radius
Join Resumma ion o Single-Inclusi e Je P oduc ion, Phys.
Re . Le . 119,212001 (2017).
[31] X. Liu, S.-O. Moch, and F. Ringe , Phenomenology o single-
inclusi e je p oduc ion wi h je adius and h eshold esumma-
ion, Phys. Re . D 97,056026 (2018).
[32] J. Cu ie, E. W. N. Glo e , and J. Pi es, Nex - o-Nex - o Lead-
ing O de QCD P edic ions o Single Je Inclusi e P oduc ion
a he LHC, Phys. Re . Le . 118,072002 (2017).
[33] M. Czakon, A. an Hame en, A. Mi o , and R. Poncele , Single-
je inclusi e a es wi h exac colo a O(α4
s), J. High Ene gy
Phys. 10 (2019)262.
[34] G. A nison e al. (UA1 Collabo a ion), Measu emen o he
inclusi e je c oss sec ion a he CERN pp collide , Phys. Le .
B172,461 (1986).
[35] J. Appel e al. (UA2 Collabo a ion), Measu emen o he s
dependence o je p oduc ion a he CERN pp collide , Phys.
Le . B 160,349 (1985).
[36] T. Aal onen e al. (CDF Collabo a ion), Measu emen o he
inclusi e je c oss sec ion a he Fe milab Te a on ppcollide
using a cone-based je algo i hm, Phys. Re . D 78,052006
(2008).
[37] V. M. Abazo e al. (D0 Collabo a ion), Measu emen o he
Inclusi e Je C oss Sec ion in ppCollisions a √s=1.96 TeV,
Phys.Re .Le .101,062001 (2008).
[38] B. Abele e al. (STAR Collabo a ion), Longi udinal Double-
Spin Asymme y and C oss Sec ion o Inclusi e Je P oduc ion
in Pola ized P o on Collisions a √s=200 GeV, Phys. Re .
Le . 97,252001 (2006).
[39] S. Acha ya e al. (ALICE Collabo a ion), Measu emen o
cha ged je c oss sec ion in pp collisions a √s=5.02 TeV,
Phys.Re .D100,092004 (2019).
[40] B. Abele e al. (ALICE Collabo a ion), Measu emen o he
inclusi e di e en ial je c oss sec ion in pp collisions a √s=
2.76 TeV, Phys. Le . B 722,262 (2013).
[41] V. Khacha yan e al. (CMS Collabo a ion), Measu emen o he
inclusi e je c oss sec ion in pp collisions a √sNN =2.76 TeV,
Eu . Phys. J. C 76,265 (2016).
[42] S. Cha chyan e al. (CMS Collabo a ion), Measu emen o he
a io o inclusi e je c oss sec ions using he an i-kTalgo i hm
wi h adius pa ame e s R=0.5 and 0.7 in ppcollisions a √s=
7TeV,Phys.Re .D90,072006 (2014).
[43] V. Khacha yan e al. (CMS Collabo a ion), Measu emen and
QCD analysis o double-di e en ial inclusi e je c oss sec ions
in pp collisions a √s=8 TeV and c oss sec ion a ios o 2.76
and 7 TeV, J. High Ene gy Phys. 03 (2017)156.
[44] V. Khacha yan e al. (CMS Collabo a ion), Measu emen o he
double-di e en ial inclusi e je c oss sec ion in p o on-p o on
collisions a √s=13 TeV, Eu .Phys.J.C76,451 (2016).
[45] G. Aad e al. (ATLAS Collabo a ion), Measu emen o he
inclusi e je c oss-sec ion in pp collisions a √sNN =2.76 TeV
and compa ison o he inclusi e je c oss-sec ion a √sNN =
7 TeV using he ATLAS de ec o , Eu . Phys. J. C 73,2509
(2013).
[46] G. Aad e al. (ATLAS Collabo a ion), Measu emen o inclusi e
je and dije p oduc ion in ppcollisions a √s=7 TeV using he
ATLAS de ec o , Phys. Re . D 86,014022 (2012).
[47] G. Aad e al. (ATLAS Collabo a ion), Measu emen o he
inclusi e je c oss-sec ion in p o on-p o on collisions a √s=
7TeVusing4.5 b−1o da a wi h he ATLAS de ec o , J. High
Ene gy Phys. 02 (2015)153.
[48] D. B i zge , K. Rabbe z, D. Sa oiu, G. Siebe , and M. Wobisch,
De e mina ion o he s ong coupling cons an using inclusi e
je c oss sec ion da a om mul iple expe imen s, Eu . Phys. J.
C79,68 (2019).
[49] R. D. Ball, S. Ca azza, L. D. Debbio, S. Fo e, Z. Kassabo ,
J. Rojo, E. Slade, and M. Ubiali, P ecision de e mina ion o
034911-15

S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020)
he s ong coupling cons an wi hin a global PDF analysis, Eu .
Phys. J. C 78,408 (2018).
[50] B. Malaescu and P. S a o oi o , E alua ion o he s ong cou-
pling cons an αSusing he ATLAS inclusi e je c oss-sec ion
da a, Eu .Phys.J.C72,2041 (2012).
[51] K. Aamod e al. (ALICE Collabo a ion), The ALICE expe i-
men a he CERN LHC, J. Ins um. 3,S08002 (2008).
[52] B. Abele e al. (ALICE Collabo a ion), Pe o mance o he
ALICE Expe imen a he CERN LHC, In . J. Mod. Phys. A
29,1430044 (2014).
[53] L. E ans and P. B yan , The CERN La ge Had on Collide :
Accele a o and expe imen s, J. Ins um. 3,S08001 (2008).
[54] P. Co ese e al. (ALICE Collabo a ion), ALICE elec o-
magne ic calo ime e echnical design epo , CERN-ALICE-
TDR-014, CERN-LHCC-2008-014, 2008 [h p://inspi ehep.
ne / eco d/794183].
[55] S. Acha ya e al. (ALICE Collabo a ion), ALICE 2017 lumi-
nosi y de e mina ion o pp collisions a √s=5 TeV, 2018
[h p://cds.ce n.ch/ eco d/2648933].
[56] B. Abele e al. (ALICE Collabo a ion), Cen ali y de e mi-
na ion o Pb-Pb collisions a √sNN =2.76 TeV wi h ALICE,
Phys.Re .C88,044909 (2013).
[57] ALICE Collabo a ion, Cen ali y de e mina ion in hea y ion
collisions [h p://cds.ce n.ch/ eco d/2636623].
[58] C. Loizides, J. Kamin, and D. d’En e ia, Imp o ed Mon e
Ca lo Glaube p edic ions a p esen and u u e nuclea collid-
e s, Phys.Re .C97,054910 (2018); E a um: Imp o ed Mon e
Ca lo Glaube p edic ions a p esen and u u e nuclea collide s
[Phys. Re . C 97, 054910 (2018)], 99,019901(E) (2019).
[59] T. Sjos and, S. Ask, J. R. Ch is iansen, R. Co ke, N. Desai, P.
Il en, S. M enna, S. P es el, C. O. Rasmussen, and P. Z. Skands,
An in oduc ion o PYTHIA 8.2, Compu . Phys. Commun. 191,
159 (2015).
[60] M. Gyulassy and X.-N. Wang, HIJING 1.0: A Mon e Ca lo
p og am o pa on and pa icle p oduc ion in high ene gy
had onic and nuclea collisions, Compu . Phys. Commun. 83,
307 (1994).
[61] S. Acha ya e al. (ALICE Collabo a ion), π0and ηmeson
p oduc ion in p o on-p o on collisions a √sNN =8TeV, Eu .
Phys. J. C 78,263 (2018).
[62] M. Caccia i, G. Salam, and G. Soyez, The an i-kTje clus e
algo i hm, J. High Ene gy Phys. 04 (2008)063.
[63] M. Caccia i, G. Salam, and G. Soyez, The ca chmen a ea o
je s, J. High Ene gy Phys. 04 (2008)005.
[64] B. Abele e al. (ALICE Collabo a ion), Measu emen o e en
backg ound luc ua ions o cha ged pa icle je econs uc ion
in Pb-Pb collisions a 2.76 TeV, J. High Ene gy Phys. 03 (2012)
053.
[65] S. Acha ya e al. (ALICE Collabo a ion), The ALICE de ini ion
o p ima y pa icles [h ps://cds.ce n.ch/ eco d/2270008/ iles/
cds.pd ].
[66] A. Hocke and V. Ka elish ili, SVD app oach o da a un old-
ing, Nucl. Ins um. Me hods A 372,469 (1996).
[67] RooUn old [h p://hepunx. l.ac.uk/∼adye/so wa e/un old/
RooUn old.h ml].
[68] G. D’Agos ini, A mul idimensional un olding me hod based on
Bayes’ heo em, Nucl. Ins um. Me hods A 362,487 (1995).
[69] S. Alioli, K. Hamil on, P. Nason, C. Olea i, and E. Re, Je pai
p oduc ion in POWHEG,J. High Ene gy Phys. 04 (2011)081.
[70] The POWHEG BOX use manual: Common ea u es
[h p:// h-www.i .uj.edu.pl/∼e ich e /POWHEG-BOX-
V2/Docs/manual-BOX.pd ].
[71] The POWHEG BOX V2 amewo k [h p:// h-www.i .uj.edu.pl/
∼e ich e /POWHEG-BOX-V2/Docs/V2-pape .pd ].
[72] ATLAS Collabo a ion, ATLAS Run 1 PYTHIA8 unes [h ps://
cds.ce n.ch/ eco d/1966419?ln=en].
[73] POWHEG me ging [h p://home. hep.lu.se/∼ o bjo n/
py hia82h ml/POWHEGMe ging.h ml].
[74] G. Soyez, A simple desc ip ion o je c oss-sec ion a ios, Phys.
Le . B 698,59 (2011).
[75] Y. He, T. Luo, X.-N. Wang, and Y. Zhu, Linea Bol zmann
anspo o je p opaga ion in he qua k-gluon plasma: Elas ic
p ocesses and medium ecoil, Phys. Re . C 91,054908 (2015).
[76] A. Idilbi and A. Majumde , Ex ending so collinea e ec i e
heo y o desc ibe ha d je s in dense QCD media, Phys.Re .D
80,054022 (2009).
[77] G. O anesyan and I. Vi e , An e ec i e heo y o je p opaga-
ion in dense QCD ma e : Je b oadening and medium-induced
b emss ahlung, J. High Ene gy Phys. 06 (2011)080.
[78] H. T. Li and I. Vi e , In e ing he mass hie a chy o je
quenching e ec s wi h p omp b-je subs uc u e, Phys. Le . B
793,259 (2019).
[79] J. Casalde ey-Solana, D. C. Gulhan, J. G. Milhano, D. Pablos,
and K. Rajagopal, A hyb id s ong/weak coupling app oach o
je quenching, J. High Ene gy Phys. 10 (2014)019.
[80] J. Casalde ey-Solana, D. C. Gulhan, J. G. Milhano, D. Pablos,
and K. Rajagopal, P edic ions o boson-je obse ables and
agmen a ion unc ion a ios om a hyb id s ong/weak cou-
pling model o je quenching, J. High Ene gy Phys. 03 (2016)
053.
[81] J. Casalde ey-Solana, D. C. Gulhan, J. G. Milhano, D. Pablos,
and K. Rajagopal, Angula s uc u e o je quenching wi hin a
hyb id s ong/weak coupling model, J. High Ene gy Phys. 03
(2017)135.
[82] Z. Hulche , D. Pablos, and K. Rajagopal, Resolu ion e ec s in
he hyb id s ong/weak coupling model, J. High Ene gy Phys.
03 (2018)010.
[83] K. Zapp, F. K auss, and U. Wiedemann, A pe u ba i e ame-
wo k o je quenching, J. High Ene gy Phys. 03 (2013)080.
[84] R. Elaya alli and K. Zapp, Simula ing V+je p ocesses in hea y
ion collisions wi h JEWEL,Eu .Phys.J.C76,695 (2016).
[85] J. Pu schke e al.,TheJETSCAPE amewo k, a Xi :1903.07706.
S. Acha ya,141 D. Adamo á,93 A. Adle ,73 J. Adol sson,79 M. M. Agga wal,98 G. Aglie i Rinella,34 M. Agnello,31
N. Ag awal,10,53 Z. Ahammed,141 S. Ahmad,17 S. U. Ahn,75 A. Akindino ,90 M. Al-Tu any,105 S. N. Alam,141
D. S. D. Albuque que,122 D. Aleksand o ,86 B. Alessand o,58 H. M. Al anda,6R. Al a o Molina,71 B. Ali,17 Y. Ali,15
A. Alici,10,27,53 A. Alkin,2J. Alme,22 T. Al ,68 L. Al enkampe ,22 I. Al sybee ,112 M. N. Anaam,6C. And ei,47 D. And eou,34
H. A. And ews,109 A. And onic,144 M. Angele i,34 V. Anguelo ,102 C. Anson,16 T. An iˇ
ci´
c,106 F. An ino i,56 P. An onioli,53
R. Anwa ,125 N. Apadula,78 L. Aphece che,114 H. Appelshäuse ,68 S. A celli,27 R. A naldi,58 M. A a ia,78 I. C. A sene,21
034911-16
MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020)
M. A slandok,102 A. Augus inus,34 R. A e beck,105 S. Aziz,61 M. D. Azmi,17 A. Badalà,55 Y. W. Baek,40 S. Bagnasco,58
X. Bai,105 R. Bailhache,68 R. Bala,99 A. Baldisse i,137 M. Ball,42 S. Balouza,103 R. Ba be a,28 L. Ba ioglio,26
G. G. Ba na öldi,145 L. S. Ba nby,92 V. Ba e ,134 P. Ba alini,6K. Ba h,34 E. Ba sch,68 F. Ba u aldi,29 N. Bas id,134
S. Basu,143 G. Ba igne,114 B. Ba yunya,74 D. Bau i,48 J. L. Bazo Alba,110 I. G. Bea den,87 C. Bedda,63 N. K. Behe a,60
I. Beliko ,136 A. D. C. Bell Hecha a ia,144 F. Bellini,34 R. Bellwied,125 V. Belyae ,91 G. Bencedi,145 S. Beole,26 A. Be cuci,47
Y. Be dniko ,96 D. Be enyi,145 R. A. Be ens,130 D. Be zano,58 M. G. Besoiu,67 L. Be e ,34 A. Bhasin,99 I. R. Bha ,99
M. A. Bha ,3H. Bha ,48 B. Bha acha jee,41 A. Bianchi,26 L. Bianchi,26 N. Bianchi,51 J. Bielˇ
cík,37 J. Bielˇ
cíko á,93
A. Bilandzic,103,117 G. Bi o,145 R. Biswas,3S. Biswas,3J. T. Blai ,119 D. Blau,86 C. Blume,68 G. Boca,139 F. Bock,34,94
A. Bogdano ,91 L. Boldizsá ,145 A. Bolozdynya,91 M. Bomba a,38 G. Bonomi,140 H. Bo el,137 A. Bo isso ,91,144 H. Bossi,146
E. Bo a,26 L. B a ud,68 P. B aun-Munzinge ,105 M. B egan ,121 T. A. B oke ,68 M. B oz,37 E. J. B ucken,43 E. B una,58
G. E. B uno,104 M. D. Buckland,127 D. Budniko ,107 H. Buesching,68 S. Bu alino,31 O. Bugnon,114 P. Buhle ,113 P. Buncic,34
Z. Bu helezi,72,131 J. B. Bu ,15 J. T. Bux on,95 S. A. Bysiak,118 D. Ca a i,88 A. Cali a,105 E. Cal o Villa ,110 R. S. Camacho,44
P. Came ini,25 A. A. Capon,113 F. Ca nesecchi,10,27 R. Ca on,137 J. Cas illo Cas ellanos,137 A. J. Cas o,130 E. A. R. Casula,54
F. Ca alano,31 C. Ceballos Sanchez,52 P. Chak abo y,48 S. Chand a,141 W. Chang,6S. Chapeland,34 M. Cha ie ,127
S. Cha opadhyay,141 S. Cha opadhyay,108 A. Chau in,24 C. Cheshko ,135 B. Cheynis,135 V. Chiban e Ba oso,34
D. D. Chinella o,122 S. Cho,60 P. Chochula,34 T. Chowdhu y,134 P. Ch is akoglou,88 C. H. Ch is ensen,87 P. Ch is iansen,79
T. Chujo,133 C. Cicalo,54 L. Ci a elli,10,27 F. Cindolo,53 J. Cleymans,124 F. Colama ia,52 D. Colella,52 A. Collu,78 M. Colocci,27
M. Concas,58,aG. Conesa Balbas e,77 Z. Conesa del Valle,61 G. Con in,59,127 J. G. Con e as,37 T. M. Co mie ,94
Y. Co ales Mo ales,26,58 P. Co ese,32 M. R. Cosen ino,123 F. Cos a,34 S. Cos anza,139 P. C oche ,134 E. Cuau le,69 P. Cui,6
L. Cunquei o,94 D. Dab owski,142 T. Dahms,103,117 A. Dainese,56 F. P. A. Damas,114,137 M. C. Danisch,102 A. Danu,67
D. Das,108 I. Das,108 P. Das,84 P. Das,3S. Das,3A. Dash,84 S. Dash,48 A. Dashi,103 S. De,84 A. De Ca o,30 G. de Ca aldo,52
C. de Con i,121 J. de Cu eland,39 A. De Falco,24 D. De G u ola,10 N. De Ma co,58 S. De Pasquale,30 S. Deb,49 B. Debjani,3
H. F. Degenha d ,121 K. R. Deja,142 A. Delo ,83 S. Delsan o,26,131 D. De e ak,105 P. Dhankhe ,48 D. Di Ba i,33 A. Di Mau o,34
R. A. Diaz,8T. Die el,124 P. Dillensege ,68 Y. Ding,6R. Di ià,34 Ø. Dju sland,22 U. Dmi ie a,62 A. Dob in,34,67 B. Dönigus,68
O. Do dic,21 A. K. Dubey,141 A. Dubla,105 S. Dudi,98 M. Dukhishyam,84 P. Dupieux,134 R. J. Ehle s,146 V. N. Eikeland,22
D. Elia,52 H. Engel,73 E. Epple,146 B. E azmus,114 F. E ha d ,97 A. E okhin,112 M. R. E sdal,22 B. Espagnon,61 G. Eulisse,34
D. E ans,109 S. E dokimo ,89 L. Fabbie i,103,117 M. Faggin,29 J. Fai e,77 F. Fan,6A. Fan oni,51 M. Fasel,94 P. Fecchio,31
A. Feliciello,58 G. Feo ilo ,112 A. Fe nández Téllez,44 A. Fe e o,137 A. Fe e i,26 A. Fes an i,34 V. J. G. Feuilla d,102
J. Figiel,118 S. Filchagin,107 D. Finogee ,62 F. M. Fionda,22 G. Fio enza,52 F. Flo ,125 S. Foe sch,72 P. Foka,105 S. Fokin,86
E. F agiacomo,59 U. F anken eld,105 U. Fuchs,34 C. Fu ge ,77 A. Fu s,62 M. Fusco Gi a d,30 J. J. Gaa dhøje,87 M. Gaglia di,26
A. M. Gago,110 A. Gal,136 C. D. Gal an,120 P. Gano i,82 C. Ga aba os,105 E. Ga cia-Solis,11 K. Ga g,28 C. Ga giulo,34
A. Ga ibli,85 K. Ga ne ,144 P. Gasik,103,117 E. F. Gauge ,119 M. B. Gay Duca i,70 M. Ge main,114 J. Ghosh,108 P. Ghosh,141
S. K. Ghosh,3P. Giano i,51 P. Giubellino,58,105 P. Giubila o,29 P. Glässel,102 D. M. Goméz Co al,71 A. Gomez Rami ez,73
V. Gonzalez,105 P. González-Zamo a,44 S. Go buno ,39 L. Gö lich,118 S. Go o ac,35 V. G abski,71 L. K. G aczykowski,142
K. L. G aham,109 L. G eine ,78 A. G elli,63 C. G igo as,34 V. G igo ie ,91 A. G igo yan,1S. G igo yan,74 O. S. G oe ik,22
F. G osa,31 J. F. G osse-Oe inghaus,34 R. G osso,105 R. Gue nane,77 M. Gui ie e,114 K. Gulb andsen,87 T. Gunji,132
A. Gup a,99 R. Gup a,99 I. B. Guzman,44 R. Haake,146 M. K. Habib,105 C. Hadjidakis,61 H. Hamagaki,80 G. Hama ,145
M. Hamid,6R. Hannigan,119 M. R. Haque,63,84 A. Ha lende o a,105 J. W. Ha is,146 A. Ha on,11 J. A. Hasenbichle ,34
D. Ha zi o iadou,10,53 P. Haue ,42 S. Hayashi,132 S. T. Heckel,68,103 E. Hellbä ,68 H. Hels up,36 A. He ghelegiu,47
E. G. He nandez,44 G. He e a Co al,9F. He mann,144 K. F. He land,36 T. E. Hilden,43 H. Hillemanns,34 C. Hills,127
B. Hippoly e,136 B. Hohlwege ,103 D. Ho ak,37 A. Ho nung,68 S. Ho nung,105 R. Hosokawa,16,133 P. H is o ,34 C. Huang,61
C. Hughes,130 P. Huhn,68 T. J. Humanic,95 H. Hushnud,108 L. A. Huso a,144 N. Hussain,41 S. A. Hussain,15 D. Hu e ,39
J. P. Iddon,34,127 R. Ilkae ,107 M. Inaba,133 G. M. Innocen i,34 M. Ippoli o ,86 A. Isako ,93 M. S. Islam,108 M. I ano ,105
V. I ano ,96 V. Izuchee ,89 B. Jacak,78 N. Jacazio,27,53 P. M. Jacobs,78 M. B. Jadha ,48 S. Jadlo ska,116 J. Jadlo sky,116
S. Jaelani,63 C. Jahnke,121 M. J. Jakubowska,142 M. A. Janik,142 M. Je cic,97 O. Je ons,109 M. Jin,125 F. Jonas,94,144
P. G. Jones,109 J. Jung,68 M. Jung,68 A. Jusko,109 P. Kalinak,64 A. Kalwei ,34 V. Kaplin,91 S. Ka ,6A. Ka asu Uysal,76
O. Ka a iche ,62 T. Ka a iche a,62 P. Ka czma czyk,34 E. Ka peche ,62 U. Kebschull,73 R. Keidel,46 M. Keil,34 B. Ke ze ,42
Z. Khabano a,88 A. M. Khan,6S. Khan,17 S. A. Khan,141 A. Khanzadee ,96 Y. Kha lo ,89 A. Kha un,17 A. Khun ia,118
B. Kileng,36 B. Kim,60 B. Kim,133 D. Kim,147 D. J. Kim,126 E. J. Kim,13 H. Kim,18,147 J. Kim,147 J. S. Kim,40 J. Kim,102
J. Kim,147 J. Kim,13 M. Kim,102 S. Kim,19 T. Kim,147 T. Kim,147 S. Ki sch,39,68 I. Kisel,39 S. Kisele ,90 A. Kisiel,142 J. L. Klay,5
C. Klein,68 J. Klein,58 S. Klein,78 C. Klein-Bösing,144 M. Kleine ,68 S. Klewin,102 A. Kluge,34 M. L. Knichel,34
A. G. Knospe,125 C. Kobdaj,115 M. K. Köhle ,102 T. Kollegge ,105 A. Kond a ye ,74 N. Kond a ye a,91 E. Kond a yuk,89
J. Konig,68 P. J. Konopka,34 L. Koska,116 O. Ko alenko,83 V. Ko alenko,112 M. Kowalski,118 I. K álik,64 A. K a ˇ
cáko á,38
L. K eis,105 M. K i da,64,109 F. K izek,93 K. K izko a Gajdoso a,37 M. K üge ,68 E. K yshen,96 M. K zewicki,39
A. M. Kube a,95 V. Ku ˇ
ce a,60 C. Kuhn,136 P. G. Kuije ,88 L. Kuma ,98 S. Kuma ,48 S. Kundu,84 P. Ku ash ili,83 A. Ku epin,62
A. B. Ku epin,62 A. Ku yakin,107 S. Kushpil,93 J. K apil,109 M. J. Kweon,60 J. Y. Kwon,60 Y. Kwon,147 S. L. La Poin e,39
P. La Rocca,28 Y. S. Lai,78 R. Langoy,129 K. Lapidus,34 A. La deux,21 P. La iono ,51 E. Laudi,34 R. La icka,37 T. Laza e a,112
R. Lea,25 L. Lea dini,102 J. Lee,133 S. Lee,147 F. Lehas,88 S. Lehne ,113 J. Leh bach,39 R. C. Lemmon,92 I. León Monzón,120
034911-17
S. ACHARYA e al. PHYSICAL REVIEW C 101, 034911 (2020)
E. D. Lesse ,20 M. Le ich,34 P. Lé ai,145 X. Li,12 X. L. Li,6J. Lien,129 R. Lie a a,109 B. Lim,18 V. Lindens u h,39
S. W. Lindsay,127 C. Lippmann,105 M. A. Lisa,95 V. Li iche skyi,43 A. Liu,78 S. Liu,95 W. J. Llope,143 I. M. Lo nes,22
V. Logino ,91 C. Loizides,94 P. Lonca ,35 X. Lopez,134 E. López To es,8J. R. Luhde ,144 M. Luna don,29 G. Lupa ello,59
Y. Ma,111 A. Mae skaya,62 M. Mage ,34 S. M. Mahmood,21 T. Mahmoud,42 A. Mai e,136 R. D. Majka,146 M. Malae ,96
Q. W. Malik,21 L. Malinina,74,bD. Mal’Ke ich,90 P. Malzache ,105 G. Mandaglio,55 V. Manko,86 F. Manso,134 V. Manza i,52
Y. Mao,6M. Ma chisone,135 J. Ma eš,66 G. V. Ma gaglio i,25 A. Ma go i,53 J. Ma gu i,63 A. Ma ín,105 C. Ma ke ,119
M. Ma qua d,68 N. A. Ma in,102 P. Ma inengo,34 J. L. Ma inez,125 M. I. Ma ínez,44 G. Ma ínez Ga cía,114
M. Ma inez Ped ei a,34 S. Masciocchi,105 M. Mase a,26 A. Masoni,54 L. Massac ie ,61 E. Masson,114 A. Mas ose io,52,138
A. M. Ma his,103,117 O. Ma onoha,79 P. F. T. Ma uoka,121 A. Ma yja,118 C. Maye ,118 M. Mazzilli,33 M. A. Mazzoni,57
A. F. Mechle ,68 F. Meddi,23 Y. Melikyan,62,91 A. Menchaca-Rocha,71 C. Mengke,6E. Meninno,30,113 M. Me es,14
S. Mhlanga,124 Y. Miake,133 L. Michele i,26 D. L. Mihaylo ,103 K. Mikhaylo ,74,90 A. Mischke,63,cA. N. Mish a,69
D. Mi´
skowiec,105 A. Modak,3N. Mohammadi,34 A. P. Mohan y,63 B. Mohan y,84 M. Mohisin Khan,17,dC. Mo dasini,103
D. A. Mo ei a De Godoy,144 L. A. P. Mo eno,44 I. Mo ozo ,62 A. Mo sch,34 T. M nja ac,34 V. Mucci o a,51 E. Mudnic,35
D. Mühlheim,144 S. Muhu i,141 J. D. Mulligan,78 M. G. Munhoz,121 K. Münning,42 R. H. Munze ,68 H. Mu akami,132
S. Mu ay,124 L. Musa,34 J. Musinsky,64 C. J. Mye s,125 J. W. My cha,142 B. Naik,48 R. Nai ,83 B. K. Nandi,48 R. Nania,10,53
E. Nappi,52 M. U. Na u,15 A. F. Nassi pou ,79 C. Na ass,130 R. Nayak,48 T. K. Nayak,84 S. Naza enko,107 A. Neagu,21
R. A. Neg ao De Oli ei a,68 L. Nellen,69 S. V. Nesbo,36 G. Nesko ic,39 D. Nes e o ,112 L. T. Neumann,142 B. S. Nielsen,87
S. Nikolae ,86 S. Nikulin,86 V. Nikulin,96 F. No e ini,10,53 P. Nomokono ,74 J. No man,77 N. No i zky,133 P. Nowakowski,142
A. Nyanin,86 J. Nys and,22 M. Ogino,80 A. Ohlson,79,102 J. Oleniacz,142 A. C. Oli ei a Da Sil a,121,130 M. H. Oli e ,146
C. Oppedisano,58 R. O a a,43 A. O iz Velasquez,69 A. Oska sson,79 J. O winowski,118 K. Oyama,80 Y. Pachmaye ,102
V. Pacik,87 D. Pagano,140 G. Pai´
c,69 J. Pan,143 A. K. Pandey,48 S. Panebianco,137 P. Pa eek,49,141 J. Pa k,60 J. E. Pa kkila,126
S. Pa ma ,98 S. P. Pa hak,125 R. N. Pa a,141 B. Paul,24,58 H. Pei,6T. Pei zmann,63 X. Peng,6L. G. Pe ei a,70 H. Pe ei a Da
Cos a,137 D. Pe esunko,86 G. M. Pe ez,8E. Pe ez Lezama,68 V. Pesko ,68 Y. Pes o ,4V. Pe áˇ
cek,37 M. Pe o ici,47
R. P. Pezzi,70 S. Piano,59 M. Pikna,14 P. Pillo ,114 L. O. D. L. Pimen el,87 O. Pinazza,34,53 L. Pinsky,125 C. Pin o,28
S. Pisano,10,51 D. Pis one,55 M. Płosko´
n,78 M. Planinic,97 F. Plique ,68 J. Plu a,142 S. Pochybo a,145,cM. G. Poghosyan,94
B. Polich chouk,89 N. Poljak,97 A. Pop,47 H. Poppenbo g,144 S. Po eboeu -Houssais,134 V. Pozdniako ,74 S. K. P asad,3
R. P eghenella,53 F. P ino,58 C. A. P uneau,143 I. Pshenichno ,62 M. Puccio,26,34 V. Punin,107 J. Pu schke,143 R. E. Quishpe,125
S. Ragoni,109 S. Raha,3S. Rajpu ,99 J. Rak,126 A. Rako oza ind abe,137 L. Ramello,32 F. Rami,136 R. Raniwala,100
S. Raniwala,100 S. S. Räsänen,43 R. Ra h,49 V. Ra za,42 I. Ra asenga,31 K. F. Read,94,130 K. Redlich,83,eA. Rehman,22
P. Reichel ,68 F. Reid ,34 X. Ren,6R. Ren o d ,68 Z. Rescako a,38 J.-P. Re ol,10 K. Reyge s,102 V. Riabo ,96 T. Riche ,79,87
M. Rich e ,21 P. Riedle ,34 W. Riegle ,34 F. Riggi,28 C. Ris ea,67 S. P. Rode,49 M. Rod íguez Cahuan zi,44 K. Røed,21
R. Rogale ,89 E. Rogochaya,74 D. Roh ,34 D. Röh ich,22 P. S. Roki a,142 F. Ronche i,51 E. D. Rosas,69 K. Roslon,142
A. Rossi,29,56 A. Ro ondi,139 F. Roukou akis,82 A. Roy,49 P. Roy,108 O. V. Rueda,79 R. Rui,25 B. Rumyan se ,74 A. Rus amo ,85
E. Ryabinkin,86 Y. Ryabo ,96 A. Rybicki,118 H. Ry konen,126 S. Sadhu,141 S. Sado sky,89 K. Ša aˇ
ík,34,37 S. K. Saha,141
B. Sahoo,48 P. Sahoo,48,49 R. Sahoo,49 S. Sahoo,65 P. K. Sahu,65 J. Saini,141 S. Sakai,133 S. Sambyal,99 V. Samsono ,91,96
D. Sa ka ,143 N. Sa ka ,141 P. Sa ma,41 V. M. Sa i,103 M. H. P. Sas,63 E. Scappa one,53 B. Schae e ,94 J. Schambach,119
H. S. Scheid,68 C. Schiaua,47 R. Schicke ,102 A. Schmah,102 C. Schmid ,105 H. R. Schmid ,101 M. O. Schmid ,102
M. Schmid ,101 N. V. Schmid ,68,94 A. R. Schmie ,130 J. Schuk a ,87 Y. Schu z,34,136 K. Schwa z,105 K. Schweda,105 G. Scioli,27
E. Scompa in,58 M. Še ˇ
cík,38 J. E. Sege ,16 Y. Sekiguchi,132 D. Sekiha a,45,132 I. Selyuzhenko ,91,105 S. Senyuko ,136
D. Se eb yako ,62 E. Se adilla,71 A. Se cenco,67 A. Shabano ,62 A. Shabe ai,114 R. Shahoyan,34 W. Shaikh,108
A. Shanga ae ,89 A. Sha ma,98 A. Sha ma,99 H. Sha ma,118 M. Sha ma,99 N. Sha ma,98 A. I. Sheikh,141 K. Shigaki,45
M. Shimomu a,81 S. Shi inkin,90 Q. Shou,111 Y. Sibi iak,86 S. Siddhan a,54 T. Siemia czuk,83 D. Sil e my ,79 G. Sima o ic,88
G. Simone i,34,103 R. Singh,84 R. Singh,99 R. Singh,49 V. K. Singh,141 V. Singhal,141 T. Sinha,108 B. Si a ,14 M. Si a,32
T. B. Skaali,21 M. Slupecki,126 N. Smi no ,146 R. J. M. Snellings,63 T. W. Snellman,43,126 C. Soncco,110 J. Song,60,125
A. Songmoolnak,115 F. So amel,29 S. So ensen,130 I. Spu owska,118 J. S achel,102 I. S an,67 P. S ankus,94 P. J. S e anic,130
E. S enlund,79 D. S occo,114 M. M. S o e ed ,36 L. D. S i o,30 A. A. P. Suaide,121 T. Sugi a e,45 C. Sui e,61 M. Suleymano ,15
M. Suljic,34 R. Sul ano ,90 M. Šumbe a,93 S. Sumowidagdo,50 S. Swain,65 A. Szabo,14 I. Sza ka,14 U. Tabassam,15
G. Taillepied,134 J. Takahashi,122 G. J. Tamba e,22 S. Tang,6,134 M. Ta hini,114 M. G. Ta zila,47 A. Tau o,34 G. Tejeda Muñoz,44
A. Telesca,34 C. Te e oli,125 D. Thaku ,49 S. Thaku ,141 D. Thomas,119 F. Tho esen,87 R. Tieulen ,135 A. Tikhono ,62
A. R. Timmins,125 A. Toia,68 N. Topilskaya,62 M. Toppi,51 F. To ales-Acos a,20 S. R. To es,9,120 A. T i i o,55 S. T ipa hy,49
T. T ipa hy,48 S. T ogolo,29 G. T ombe a,33 L. T opp,38 V. T ubniko ,2W. H. T zaska,126 T. P. T zcinski,142 B. A. T zeciak,63
T. Tsuji,132 A. Tumkin,107 R. Tu isi,56 T. S. T e e ,21 K. Ullaland,22 E. N. Umaka,125 A. U as,135 G. L. Usai,24 A. U obicic,97
M. Vala,38 N. Valle,139 S. Valle o,58 N. an de Kolk,63 L. V. R. an Do emalen,63 M. an Leeuwen,63 P. Vande Vy e,34
D. Va ga,145 Z. Va ga,145 M. Va ga-Ko a ago,145 A. Va gas,44 M. Va gyas,126 M. Vasileiou,82 A. Vasilie ,86
O. Vázquez Doce,103,117 V. Veche nin,112 A. M. Veen,63 E. Ve cellin,26 S. Ve ga a Limón,44 L. Ve mun ,63 R. Ve ne ,7
R. Vé esi,145 L. Vicko ic,35 J. Viinikainen,126 Z. Vilakazi,131 O. Villalobos Baillie,109 A. Villa o o Tello,44 G. Vino,52
A. Vinog ado ,86 T. Vi gili,30 V. Visla icius,87 A. Vodopyano ,74 B. Volkel,34 M. A. Völkl,101 K. Voloshin,90 S. A. Voloshin,143
G. Volpe,33 B. on Halle ,34 I. Vo obye ,103 D. Voscek,116 J. V láko á,38 B. Wagne ,22 M. Webe ,113 S. G. Webe ,105,144
034911-18
MEASUREMENTS OF INCLUSIVE JET SPECTRA IN pp … PHYSICAL REVIEW C 101, 034911 (2020)
A. Weg zynek,34 D. F. Weise ,102 S. C. Wenzel,34 J. P. Wessels,144 J. Wiechula,68 J. Wikne,21 G. Wilk,83 J. Wilkinson,10,53
G. A. Willems,34 E. Willshe ,109 B. Windelband,102 W. E. Wi ,130 Y. Wu,128 R. Xu,6S. Yalcin,76 K. Yamakawa,45 S. Yang,22
S. Yano,137 Z. Yin,6H. Yokoyama,63 I.-K. Yoo,18 J. H. Yoon,60 S. Yuan,22 A. Yuncu,102 V. Yu chenko,2V. Zaccolo,25
A. Zaman,15 C. Zampolli,34 H. J. C. Zanoli,63,121 N. Za dosh i,34 A. Za ochen se ,112 P. Zá ada,66 N. Za iyalo ,107
H. Zb oszczyk,142 M. Zhalo ,96 S. Zhang,111 X. Zhang,6Z. Zhang,6V. Zhe ebche skii,112 N. Zhiga e a,90 D. Zhou,6Y. Zhou,87
Z. Zhou,22 J. Zhu,6,105 Y. Zhu,6A. Zichichi,10,27 M. B. Zimme mann,34 G. Zino je ,2and N. Zu lo140
(ALICE Collabo a ion)
1A. I. Alikhanyan Na ional Science Labo a o y (Ye e an Physics Ins i u e) Founda ion, Ye e an, A menia
2Bogolyubo Ins i u e o Theo e ical Physics, Na ional Academy o Sciences o Uk aine, Kie , Uk aine
3Bose Ins i u e, Depa men o Physics and Cen e o As opa icle Physics and Space Science (CAPSS), Kolka a, India
4Budke Ins i u e o Nuclea Physics, No osibi sk, Russia
5Cali o nia Poly echnic S a e Uni e si y, San Luis Obispo, Cali o nia, USA
6Cen al China No mal Uni e si y, Wuhan, China
7Cen e de Calcul de l’IN2P3, Villeu banne, Lyon, F ance
8Cen o de Aplicaciones Tecnológicas y Desa ollo Nuclea (CEADEN), Ha ana, Cuba
9Cen o de In es igación y de Es udios A anzados (CINVESTAV), Mexico Ci y and Mé ida, Mexico
10Cen o Fe mi, Museo S o ico della Fisica e Cen o S udi e Rice che “En ico Fe mi,” Rome, I aly
11Chicago S a e Uni e si y, Chicago, Illinois, USA
12China Ins i u e o A omic Ene gy, Beijing, China
13Chonbuk Na ional Uni e si y, Jeonju, Republic o Ko ea
14Comenius Uni e si y B a isla a, Facul y o Ma hema ics, Physics and In o ma ics, B a isla a, Slo akia
15COMSATS Uni e si y Islamabad, Islamabad, Pakis an
16C eigh on Uni e si y, Omaha, Neb aska, USA
17Depa men o Physics, Aliga h Muslim Uni e si y, Aliga h, India
18Depa men o Physics, Pusan Na ional Uni e si y, Pusan, Republic o Ko ea
19Depa men o Physics, Sejong Uni e si y, Seoul, Republic o Ko ea
20Depa men o Physics, Uni e si y o Cali o nia, Be keley, Cali o nia, USA
21Depa men o Physics, Uni e si y o Oslo, Oslo, No way
22Depa men o Physics and Technology, Uni e si y o Be gen, Be gen, No way
23Dipa imen o di Fisica dell’Uni e si à ’La Sapienza’ and Sezione INFN, Rome, I aly
24Dipa imen o di Fisica dell’Uni e si à and Sezione INFN, Caglia i, I aly
25Dipa imen o di Fisica dell’Uni e si à and Sezione INFN, T ies e, I aly
26Dipa imen o di Fisica dell’Uni e si à and Sezione INFN, Tu in, I aly
27Dipa imen o di Fisica e As onomia dell’Uni e si à and Sezione INFN, Bologna, I aly
28Dipa imen o di Fisica e As onomia dell’Uni e si à and Sezione INFN, Ca ania, I aly
29Dipa imen o di Fisica e As onomia dell’Uni e si à and Sezione INFN, Pado a, I aly
30Dipa imen o di Fisica “E. 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