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Hard QCD Results with Jets at the LHC SvenMenke1,aonbehalfoftheATLASandCMScollaborations Max-Planck-Institutfu¨rPhysik,Fo¨hringerRing6,80805Mu¨nchen,Germany √ Abstract. HardQCDresultsinproton-protoncollisionsat s=7TeVwithjetsfromdatarecordeduptothe endof2010bytheCMSandATLASexperimentsattheLHCarereported.Inclusivejetanddi-jetcrosssection measurementsaswellasobservablessensitivetomulti-jetactivityareshownandcomparedtosimulationsbased onleadinglogpartonshowersaswellasNLOQCDpredictions.Novelapproachestoidentifyhighlyboosted 2 1 massivefinalstatesbyexploitingthejetsubstructurearetestedonthedominantQCDbackground. 0 2 1 Introduction uncertainty are validated with in-situ methods using p n ⊥ a balanceindi-jetandγ-jeteventsandthemomentumpro- J TheATLAS[1]andCMS[2]experimentsbothhaverich jectionfractionmethodinγ-jetevents.TheMonnteCarlo 5 QCDprogramsinvolvinghigh p jetsaimingtoprobethe based correction factors are validated with single particle ⊥ 2 structure of the colliding protons, to measure the strong test-beamdataandE/pmeasurementsofisolatedhadrons coupling constant and to test the standard model (SM) at in collision data which are then extrapolated using frag- ] the shortest distance scales accessible today in the high- mentationpredictionstothejet-level.ThesystematicJES x e center-of-mass proton-proton collisions of the LHC. Fur- uncertaintyistypically3−6%forbothATLASandCMS - thermoredeviationsfromtheSMwouldindicatethepres- over a large range of pseudo-rapidities and p⊥, with the p enceofnewphysicsbeyondtheSM.Thedatasetsrecorded largervaluesatlarge|η|,verylowandveryhigh p⊥. e h uptotheendof2010andcorrespondingtointegratedlu- [ minositiesofL (cid:39) 35pb−1 perexperimenthavebeenused byATLASandCMStoupdatetheirmeasurementsofin- 3 Inclusive jet cross section 2 clusive jet and di-jet cross sections, as well as to mea- v measurements sure multi-jet and angular di-jet distributions. New meth- 8 ods based on the sub-structure of jets to detect heavily 7 9 boostedmassiveobjectsendingupinsinglejetsattheLHC TheinclusivejetcrosssectionismeasuredbyATLAS[10] 4 have also been tested on the dominant QCD background and CMS [11] as a function of transverse jet momentum . andcomparedtoexpectations. p⊥ andjetrapidityy.Thedataiscorrectedbin-by-binfor 1 migrationeffectsin p duetothesteeplyfallingspectrum 0 ⊥ in p and the finite p resolution. In CMS the corrected 2 ⊥ ⊥ 1 2 Jet reconstruction and calibration : v arXi Tgr0e.oh7creo.itnIihnnsmtpfrruua[tcr3ett]iodo-insthamuensdojeeddcteoablwllyginiotbehroaittrdhh-ismsaetafxaenprceeAern4impt-iav-ereknac⊥tmtsojeeritsntercststlheue0ms.t4iemnrc≤iinnluggRsiaev≤lie-- 2σ [pb/TeV]|yd|m/dd12max1111111000000011111220246801 ×NS yLNsOote npm QpaeCtriDct. uc(CnocrTre.ErtQa in6t.i6e)s 2100 .... 1283 <<<< |||||yyyyy|||||mmmmmaaaaaxxxxx <<<<< 22100.....81283 (((((××××× 111110000086420))))) ther from stable particles in generator-level simulations, 108 106 partonsinNLOcalculations,topologicalcalorimeterclus- 104 ters [4,5] in ATLAS or particle flow (PF) objects [6,7] in 102 asn t=i k7t TjeetVs,, ∫ RL =d t0 =.4 37 pb 1 CMSinfullsimulationsanddata.Topologicalclusterscan 1 ATLASPreliminary 10 2 10 1 2×10 1 1 2 3 45 becalibratedpriortothejetmaking[5]inATLASorleft m12 [TeV] attheelectromagnetic(EM)scale.ThePFobjectsusein- Fig.1.InclusivejetcrosssectionfromCMS(left)forAnti-k jets formationfromallCMSsubsystemsandarecalibratedto ⊥ withR=0.5asfunctionof p for6rapidityintervalsscaledfor correspondtostableparticleslikeγ’s,leptons,chargedand ⊥ easierviewing.Thedatapoints(symbols)arecomparedtoNLO neutral hadrons. In all cases residual jet-level corrections predictions (solid lines) corrected for non-perturbative effects. areneededtoaccountforparticlelossesnotdetectableon Experimental uncertainties are indicated by the yellow bands; clusterorPFobjectlevel[8,9]withlargercorrections(up DoubledifferentialcrosssectionfromATLAS(right)forAnti-k ⊥ toafactorof2)forEM-scaleinputsandsmallcorrections di-jeteventswithR=0.4asfunctionofdi-jetmassm for5in- (onthelevelof5−10%)foralreadycalibratedinputs.The 12 tervalsofmaximumrapidity|y |withsystematicexperimental max jet-levelcalibrationsareMonteCarlo(MC)basedcorrec- uncertainties(greyband).NLOpredictionswithNPcorrections tion functions in |η| and p⊥. Jet energy scale (JES) and anduncertaintiesareshownaswell(yellowband). a e-mail:[email protected] EPJWebofConferences JJ σσ22/d|y|(CTEQ 6.6)/dp/d|y|/d/dpd0TT0001111.......468246821 AanTti kLtDCC AaTT jetE1at0SQs. 6R.P 6=0r.4e (l0i.m0<|iyn|<a0NNM.3NNrS)yPP T∆DDWPFFD2F 022(C0..018L((911000)00)) σσ22/d|y|(CTEQ 6.6)/dp/d|y|/d/dpd0TT0001111.......468246821 AanTti kLtDCH AaTE jetERatSQAs. P 6RD.P 6F=0 1r.4.e0 (l0i.m0<|iyn|<a0HG.3ErJ)RyR ∆ A2PPD0F0D(8CFL 19.05) ⊗Ratio to NLO (CT10) NP 1.125 CCMNHAMTNEBS1RPKST0WDA MD ⊗FP02a2 D90tN.a 0F1⊗P81 ⊗ , .N ⊗0∆ PN P⊗NPD PNFP CL68 ⊗Ratio to NLO (CT10) NP 1.125 CCMNHAMTNEBS1RPKTS0WDAM D⊗FP02a2 D90tN.a 0F1⊗P81 ⊗ , .N ⊗0∆ PN P⊗NPD PNFP CL68 102 103 pT[GeV] 102 103 pT[GeV] 0.5 0.5 σσ22/d|y|(CTEQ 6.6)/dp/d|y|/d/dpd0TT012...55521 AanTti kLCCtD ATTa jteE1at0SQs. 6R.P6 =0r.4e (l2i.m1<|iyn|<a2NNM.8NNrS)yPP T∆DDWPFFD2F 022(C0..018L((911000)00)) σσ22/d|y|(CTEQ 6.6)/dp/d|y|/d/dpd0TT012...55521 AanTti kLCHtD ATEa jteERatSQAs. P 6RD.P6 F=0 1r.4.e0 (l2i.m1<|iyn|<a2HG.8ErJ)RyR ∆ A2PPD0F0D(8CFL 19.05) CjFeiMtg.mS3a0.fsoRsrCD0a.Mi0(j0e tAS≤.tM2 iM| y oLa|nm s=jas jx3t o )<6 iA 0p-nf.b5tko-i1- k0t ⊥ Tv.√ h5Rse ==e0 j7r.7 eTdetVNso1uLwbOMliJetJh (pTderRVie3ff)dei=cretino0tni.a7s0lfadoC0D2si..Mi07jr-e S≤tj aM| y eLa||m ys=tas x3f 1 | <6 ucA 2pn.br5nt<-i1-o k c T√ sRst =s=i00 o7.7 Ts.ne5Ve2co(tlifeoMftnJthJ )(eTferaVo4d)nmid- 102 pT[GeV] 102 pT[GeV] 2.0<|y|<2.5(right).ThereferenceNLOpredictionusesCT10 whichiscomparedtotheratiosusingMSTW 2008,NNPDF 2.1, Fig.2.RatiooftheinclusivejetcrosssectionfromATLASfor HERAPDF 1.0andABKM09instead.Errorbarsindicatestatistical Anti-k jets with R = 0.4 as function of p over NLO predic- ⊥ ⊥ errors.Thegreybandshowstheexperimentalsystematicuncer- tionsfor|y| < 0.3(top)and2.1 < |y| < 2.8(bottom).Therefer- taintiesandtheyellowbandthetypicalPDFuncertainty(CT10). enceNLOpredictionisCTEQ 6.6whichiscomparedtothera- Non-perturbative uncertainties are dominant at low masses and tiosusingCT10,MSTW 2008,NNPDF 2.0andNNPDF 2.1(left); notshowninthefigures. HERAPDF 1.0,HERAPDF 1.5andGJR08(right).Error barsin- dicatestatisticalerrors.Thelightshadedbandshowstheexper- imentalsystematicuncertaintiesexcludingacommon3.4%un- certaintyfromtheluminositymeasurement.Theotherbandsin- dicatetherespectivetheoreticaluncertainties. R = 0.4. Similar results are obtained by CMS [14] for R = 0.7. Both ATLAS and CMS use full simulations to obtain the bin-by-bin migration corrections for the distri- butions. Dominant experimental systematic uncertainties stemfromtheJESuncertaintyandareintherangeof15− spectraareobtainedbyfittingamodifiedpower-lawfunc- 30%forATLASandaround15%atlowmassesand60% tion with Gaussian smearing in p to the observed spec- ⊥ at high masses for CMS. As is the case for the inclusive tra.InATLASthecorrectionfactorsareobtainedfromfull detectorsimulationsincludingdetectorinefficiencies.Typ- jet cross section measurement a comprehensive compar- ison to NLO pQCD predictions has been made by both icalcorrectionsareinthe10−15%rangebutcanextend ATLAS [10] and CMS [13]. Figure 3 shows the ratio of to30−50%attheedgesofthephasespace.TheNLOper- themeasureddoubledifferentialdi-jetcrosssectiontothat turbativeQCD(pQCD)predictionsonparton-levelonthe otherhandarecorrectedfornon-perturbative(NP)effects predicted in CT10-based MC simulation for two rapidity bins. The agreement with HERAPDF is best, but all tested due to hadronisation and the underlying event activities. PDFsetsagreewithinuncertainties. These corrections are obtained by comparing simulations with leading log generators (PYTHIA/HERWIG) which are runwithandwithouttheseeffectsenabled.Thecorrections dependstronglyonjetsize.ForR=0.5,0.6theunderlying 4 Angular and multi-jet variables eventeffectsdominateandcorrectionsarearound1.2−1.4 at small p⊥. For R = 0.4 hadronisation effects are domi- Duetotheirsensitivitytonewphysicsandtheirabilityto nant and corrections of about 0.8 are obtained at low p⊥. probe mass scales without explicitly relying on JES cal- Thecorrectionsapproachunityatlarger p⊥ forallusedR ibrations the angular distributions of multi-jet events are values. of particular interest. The azimuthal de-correlation ∆φ of Figure1(left)showstheinclusivejetcrosssectionmea- the two most energetic jets as measured by ATLAS [15] surement for jets with size R = 0.5 as a function of jet is shown in the left plot of figure 4. Values close to π are transversemomentummeasuredbyCMS.Theexperimen- expectedfordi-jeteventswhilesmallervaluesindicatethe tal uncertainties are in the range 10−20% and are dom- presenceofadditionaljets.NLOpQCDcalculationsusing inatedbytheuncertaintiesonJESandresolution.Similar NLOJet++andMSTW 2008agreewiththedatafor∆φ<π. distributionsforR = 0.4andR = 0.6areobtainedbyAT- Leadinglogsimulations(PYTHIA,HERWIG,SHERPAagree LAS,withuncertaintiesintherangeof10−30%.Different withthedataandgiveagooddescriptionoftheperturba- NLO predictions are tested [12,13] by comparing the ra- tively diverging point ∆φ = π. The right side plot of fig- tiosofdatatoNLOMCpredictionsforvariousPDFsets. ure4showsthedistributionofχ =exp|y −y |,theex- dijet 1 2 Figure 2 shows an example from ATLAS for the rapidity ponentialoftherapiditydifferencebetweenthetwolead- region|y|<0.3forR=0.4andR=0.6.CMSobtainssim- ing jets in p , as measured by CMS [16] for different di- ⊥ ilarcomparisonsforR = 0.5.TheNLOpredictionsarein jetmassintervals.Thedistributioninχ isexpectedtobe dijet general systematically above the data but still compatible almostflatforQCDwhilenewphysics(suchasquarkcom- with the measurement within the assigned uncertainties. positeness) would cause excess events at small χ . The dijet Thedeviationsbecomelargeratlarge|y|and p⊥. comparison to NLO pQCD calculations with NLOJet++ The double differential cross section in the maximum and the CTEQ 6.6 PDF-set shows good agreement with jet rapidity |y | and di-jet mass m for di-jet events as thedata,andalowerlimitonthecontactinteractionscale max 12 measuredbyATLAS[10]isshowninFigure1(right)for forleft-handedquarksofΛ+ =5.6TeV(Λ− =6.7TeV)for HadronColliderPhysicsSymposium2011 1] [radians/d d1/φ∆σσ111111100000003456789 aA1 1D654322 n16 000161aT t00 000000it a< L<<<<<<<k t∫ppp ppppppAjLemTmTmTmTmTmTmTmTmTtdaSaaaaaaaasxxxxxxxxxt ≤≤≤≤≤≤≤≤>=R 3128654328=66100001600 s000000000.p6 = bGGGGGGGGG 71 epeeeeeeeeVVVVVVVV VTT> (((((((((1e×××××××××0111111111V0000000000 017654328G)))))))))eV |y|<0.8 /d d1//d d1//d d1//d d1//d d1//d d1//d d1//d d1//d d1//d d1/χσσχσσχσσχσσχσσχσσχσσχσσχσσχσσdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijetdijet0000000000000000000000000000000000000000........................................4567456745674567456745674567456745674567 DΛΛQ+-aC t==Da 55 p TTreeedVVicti11Mo..n84jj <<> MM2.2jjjj T<< e21LV..s28 = C=TT 3ee M7VV6 S TpebV-(((1+++000...435))) Gap fraction345 2211197418520000000 ≤≤ ≤≤≤≤≤ pp pppppTT TTTTT<< <<<<<19 20222110 74185G 00000Ge GGGGGeVVeeeee VVVVV ( +( +0(((((0)+++++.322115).).))55)) LQAe0aT =d Li2n0gADHPP GOOaEpStTeJWWa Vd (HH2pij0eaEE1trGG t0so en++l e lPHecYvEtieoTRlnH)WIAIG RR32320000....686811 sC= M7 TSeV aLnintt=i-3K6T pRb=-10.5 102 1.1 < Mjj < 1.4 TeV (+0.25) 1110010 10 321 π/2 2π/3PNscDLaOFle &p u5Q nαπCcs ./Du6n cO.(α4s) π 000000000000000000000000000000..............................232323232323232323231111111111 00000.....58632 5555< <<<< M MMMMjj jjjjjjjj< <<<< 0 1000.6....18535 5 5 TTT TTeeeVeVeVVV((((++++0000....1210))55)) 21 0000....242400 00..55 11DPPPMAHSYYYLyaEAsPtTTTRDatGHHHeWGmIIIEAAARIGaN668At + i+Pcttt11+uuu HUP nnnt.. ueeeYn+55n cT ZD2PeeHC26r Y2tITaAT.3i6Hn tItyAun6e t uD22n6eT D6T 22..55 ∆φ [radians] 2222222222 4444444444 6666666666 8888888888 11111111110000000000 11111111112222222222 11111111114444444444χχχχχχχχχχ 11111111116666666666 00 1 2 3 4 5 ∆y6 HHTT ((TTeeVV)) ddddddddddiiiiiiiiiijjjjjjjjjjeeeeeeeeeetttttttttt Fig.4.Azimuthalde-correlation∆φofthetwomostenergeticjets Fig. 5. Gap-fraction (left) for the two leading jets in p as a ⊥ asmeasuredbyATLAS(left)forAnti-k⊥ jetswithR = 0.6for function of ∆y for various intervals of p¯⊥ as measured by AT- differentpmaxintervals(blackmarkers)comparedtoNLOpQCD LAS(markersandyellowerrorband)comparedtoHEJcalcula- ⊥ calculations(redlines)withassociatederrors(hatchpattern);The tions(blueband)andNLOsimulationswithPOWHEGinterfaced distributionofχ (blackpoints)fordifferentM rangesasmea- toPYTHIA(reddashes)andHERWIG(bluedot-dashes);Ratioof dijet jj suredbyCMS(right)forAnti-k⊥jetswithR=0.5comparedto inclusive3-jetoverthe2-jetcrosssectionsR32asfunctionofto- NLO pQCD calculations (shaded band) and predictions includ- taltransversemomentumH (right)asmeasuredbyCMS(black ⊥ ingcontactinteractions(coloredlines)forcompositenessscales dots and yellow uncertainty band) compared to various simu- ofΛ+/−=5TeV. lations using different PYTHIA tunes, MADGRAPH, ALPGEN and HERWIG++. destructive(constructive)interferencehasbeenobtainedat 5 Jet mass and sub-structure 95% CL. A complementary study of the rapidity gap be- tweenthetwojetswitheitherleading p orthelargestra- ⊥ In the high energy regime of LHC, heavy objects with piditygap∆yhasbeendonebyATLAS[17].Theso-called massesO(100GeV),canreceivelargeLorentzboostssuch gap-fractionisdefinedasthefractionofeventswithoutad- thattheirdecayproductsaremeasuredinasinglejet.Sev- ditionaljetactivityintherapidityintervalbetweenthetwo eralapproachesareconsideredtoexplorethesub-structure jets.Anyadditionaljetwithinthegaphastohaveatrans- of these jets with the aim to identify such heavy objects. verse momentum above a veto scale p > Q , with the ⊥ 0 default choice Q = 20GeV to stay far away from Λ . Amongthemare: 0 QCD The gap-fraction is shown in the left plot of figure 5 for C/Afiltering: Theclusteringoflarge(R(cid:39)1.2)Cambridge- the choice of leading jets in p⊥ as a function of ∆y for Aachen (C/A) [19] type jets is reversed until a large various intervals of the average transverse momentum of dropinjet-massisobserved.Theremainingconstituents the two leading jets p¯⊥. The comparison with HEJ calcu- arere-clusteredwithasmallerRparameter. lationsshowssomedeviationsinthelarge p¯⊥ regionsbut Jetpruning: C/Aork⊥[20,21]jet-clusteringisperformed theagreementimprovesasp¯⊥approachesQ0,whichisex- ontheconstituentsofalargejetandineachclustering pectedsinceHEJisdesignedtogiveagooddescriptionof step the softer of the two clusters being combined is QCDinthelimitwherealljetshavesimilar p⊥.Thebest discarded if it’s transverse momentum is below a cer- descriptionisachievedwithPOWHEGinterfacedtoPYTHIA tainfractionoftheoriginaljet p andtheangulardis- ⊥ although deviations are observed at large ∆y. POWHEG in- tancebetweenthetwoclustersislarge. terfaced to HERWIG tends to predict smaller gap fractions Forthejetsubstructurealgorithmstobeusefultheyhave over the full phase space and the deviations increase for larger∆yasforthePOWHEG+PYTHIAcase. to be tested on QCD jets as this will be the main back- ground.C/AFilteringisusefulforthedecaysofheavypar- The right hand plot in figure 5 shows the cross sec- ticles to two low mass objects and the QCD behavior has tion ratio of three-jet over two-jet events R as a func- tionofthetotaltransversemomentumsum H32 = (cid:80) p beenstudiedinATLASin[22].Themassdropm1/mjet of ⊥ jets ⊥ theleadingsubjetisrequiredtobesmallerthan0.67(light asmeasuredbyCMS[18].Manysystematicuncertainties (cid:16) (cid:17)2 suchasthoseduetotheJESandthejetselectionefficiency subjet)andthe p⊥asymmetry min(p1⊥,p2⊥)×∆R1,2/mjet largely cancel in this ratio, while the uncertainty due to largerthan0.09(fairlysymmetric).Onceareversedclus- the integrated luminosity vanishes entirely. Therefore R teringstepwiththesepropertiesisfoundthecurrentjetis 32 provides a stringent test of QCD predictions. Events with re-clusteredwithC/AandR=min(0.3,∆R /2)findingn 1,2 two or more Anti-k jets with R = 0.5 with |y| < 2.5 new subjets of which the leading min(3,n) are combined ⊥ and p > 50GeV and H > 0.2TeV are selected and togivethefinalC/Afilteredjet.Figure6showsthespec- ⊥ ⊥ compared to various PYTHIA6, PYTHIA8 and HERWIG++ trum of jet masses for C/A jets with R = 1.2 before and based tunes and to simulations using the multi-parton fi- afterthefilteringprocedureineventswithexactlyonepri- nalstategeneratorsMADPGRAPHandALPGENinterfacedto mary vertex (to remove pile-up) and at least one jet with PYTHIA6.Allpredictionsdescribetheobservedratiowell p > 300GeV and |y| < 2. The agreement with all three ⊥ in the region H > 0.5TeV but, with the exception of predictionsisgoodalthoughHERWIG++producesjetswith ⊥ MADPGRAPH,overshootbetween10−30%atlowerH . larger mass (before filtering) compared to data. Jet prun- ⊥ EPJWebofConferences σd 1 σdm [GeV]000...0000.00106821 ATLAS Preliminary CNPaVm =b r1id, gpAPHHeTTyeet Lrr h>wwAAiaii Sgga3J+ c20i+m0h01me 0Gyn D eaRVta=,, 1L| y.=2| 3 <j5ep 2tbs 1 σd 1 σdm [GeV]00..000.000681 ATLAS Preliminary CSNPpaVlmi t=/bF r1iildt,e gpAPHHreTTyeeet Lrr hd>wwAAia ii Sggwa3J+ c20ii+mt0h0h1me 0GRyn D qeaRqVt a=>,, 1L |0 y.=2.| 3 3 <j5ep 2tbs 1 AIo’fdcAlkiTkneLoAtowStlheaandndkgCtmhMeeSJnetftosPrerpfroorvmidainncgemanedwSiMth/QthCeDmgartoeuripasl 0.004 0.004 presented here. In particular I benefited greatly from dis- 0.002 0.002 cussionswithJ.Butterworth,M.Campanelli,A.Davison, MC / DataMC / Data0111101111..........8246882468011 50 100 150 200 250 300 MC / DataMC / Data0111101111..........8246882468011 50 100 150 200 250 300 A.DiCiaccio,K.Kousouris,andM.Voutilainen. 00..66 00..66 00..44 00..44 00..22 5500 110000 115500 220000 225500 330000 00..22 5500 110000 115500 220000 225500 330000 JJeett MMaassss [[GGeeVV]] JJeett MMaassss [[GGeeVV]] References Fig.6.JetmassesforC/AjetswithR=1.2before(left)andafter (right)thefilteringprocedure(seetext)asmeasuredbyATLAS. 1. G. Aad et al. (ATLAS Collaboration), JINST 3, Thedata(blackpointsandshadederrorband)isfullycorrected S08003(2008) fordetectoreffectsandcomparedtoPYTHIA,HERWIG/JIMMYand 2. R. Adolphi et al. (CMS Collaboration), JINST 3, HERWIG++. The lower portions of the plots show ratios of the S08004(2008) distributionsoverdata. 3. M. Cacciari, G.P. Salam, G. Soyez, JHEP 04, 063 (2008),arXiv:0802.1189 4. W. Lampl, S. Laplace, D. Lelas, P. Loch, H. Ma, S. Menke, S. Rajagopalan, D. Rousseau, S. Snyder, Probability000..0.112.6822 3CJ4eM.t7 SP DPPH prPyyaeubtttrrhhna-we1ii iaailagni mTTt+g uu+ inn AsTneeu alZD=ng2r6 eoyT72rT3iethVm Probability0000..00..00343455 3CJ4eM.t7 SP DPPH prPyyaeubtttrrhhna-we1ii iaailagni mTTt+g uu+ inn AsTneeu alZD=ng2r6 eoyT72rT3iethVm 5. GGG..enUeAnvaaadl(2(A0e0Tt8L)Aa,lAS.TLC(-AoLTllAaLRbAGoS-raPtUiCoBno-)l2,la0Tb0eo8cr-ha.0ti0ore2np)., C(2E0R09N),, 0.14 arXiv:0901.0512 0.12 0.025 0.1 0.02 6. CMS Collaboartion, Tech. rep., CERN, Geneva 00..0068 0.015 (2009),CMS-PAS-PFT-09-001 0.01 0.04 7. CMS Collaboration, Tech. rep., CERN, Geneva 0.02 0.005 00 20 40 60 80 100 m1j2e0t (G1e4V0/c2) 00 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 mmje1t1 8. S(2.0C10h)a,trCcMhSy-aPnAeSt-aPlF.T(C-1M0S-0C0o1llaboration), JINST 6, Fig.7.Leadingjetpruningquantitiesineventswithatleast2hard P11002(2011),arXiv:1107.4277 jetsasmeasuredbyCMS(datapoints).Shownarethemassofthe 9. ATLAS Collaboration, Tech. rep., CERN, Geneva pruned jet (left) and the mass dropof the leading subjet (right) (2011),ATLAS-CONF-2011-032 The data is normalized to unity and compared to two PYTHIA 10. ATLAS Collaboration, Tech. rep., CERN, Geneva tunes(redandblue)andHERWIG++(green). (2011),ATLAS-CONF-2011-047 11. S.Chatrchyanetal.(CMSCollaboration),Phys.Rev. Lett.107,132001(2011) 12. ATLAS Collaboration, Tech. rep., CERN, Geneva (2011),ATLAS-PHYS-PUB-2011-005 ing is useful for W tagging and the QCD behavior has 13. CMS Collaboartion, Tech. rep., CERN, Geneva beentestedbyCMSin[23].ForboostedWsdecayinginto (2011),CMS-NOTE-2011-004 twoquarkswithsimilarenergyandmasstwolightsubjets 14. S. Chatrchyan et al. (CMS), Phys. Lett. B700, 187 are expected in the pruning algorithm with the pruned jet (2011),arXiv:1104.1693 mass close to m . The mass drop m /m of the leading W 1 jet 15. G. Aad et al. (ATLAS Collaboration), Phys.Rev.Lett. subjetshouldbesmallerthan0.4consistentwithtwolight 106,172002(2011),arXiv:1102.2696 subjets.Figure7showsthepruningpropertiesofthelead- 16. V. Khachatryan et al. (CMS Collabora- ingjetineventswithatleasttwohigh p > 200GeVjets ⊥ tion), Phys.Rev.Lett. 106, 201804 (2011), with ∆φ > 2.1 and |η| < 2.5 in comparison to two differ- arXiv:1102.2020 ent PYTHIA tunes and HERWIG++. The overall agreement 17. G.Aadetal.(ATLASCollaboration),JHEP1109,053 of the data with simulation is good – especially with the (2011),arXiv:1107.1641 HERWIG++tune. 18. S. Chatrchyan et al. (CMS Collaboration), Phys.Lett. B702,336(2011),arXiv:1106.0647 19. Y.L. Dokshitzer, G. Leder, S. Moretti, B. Webber, JHEP9708,001(1997),hep-ph/9707323 6 Conclusions 20. S. Catani, Y.L. Dokshitzer, M. Seymour, B. Webber, Nucl.Phys.B406,187(1993) 21. S.D. Ellis, D.E. Soper, Phys.Rev. D48, 3160 (1993), Both ATLAS and CMS have made comprehensive stud- hep-ph/9305266 iesofhardQCDinvolvingjets.Excellentagreementwith 22. ATLAS Collaboration, Tech. rep., CERN, Geneva NLO pQCD calculations has been found and constraints (2011),ATLAS-CONF-2011-073 onnewphysicsweresetbytheobservedagreement.Novel 23. CMS Collaboartion, Tech. rep., CERN, Geneva techniques to identify massive boosted objects were suc- (2011),CMS-PAS-JME-10-013 cessfully tested on the large QCD background expected. The challenge will be to continue the studies presented hereundertheincreasedpile-upconditionsinthedatataken beyond2010.

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