Kenneth Wraight Fully-leptonic ttbar + jets events at ATLAS • Introduction to top quarks at ATLAS • MC based di-leptonic cross-section measurement • Study of effect of jet algorithm choice • Study of effect of ISR model variation on simulated cross-section Thanks to Craig Buttar and Sarah Allwood-Spiers Part I Introduction to top quarks at ATLAS 2 The ubiquitous top quark • The strong force is measured in top pair production. • The weak force is measured in top decay and single top production. • Fundamental top parameters like mass, spin and charge still require precise measurement . • Tops decay before hadronisation, passing spin information to daughters. This provides unique environment for Beyond Standard Model searches. • Ultimate test of multi-scale QCD calculations used to predict top and new physics properties. 3 The top quark as background LHC will be the world’s first proper top quark factory: ~1 ttbar event per second for σ=833pb at L=1033cm-2s-1 Background to... associated Higgs production multi-jet SUSY decays new & exotic physics 4 Diameter = 25m, Length = 46m, Weight = 7000 tonnes LHC ATLAS (the detector) Muon detectors Calorimeters ATLAS Magnets Inner detector ATLAS is a general purpose detector designed to measure collision products in order to test the Higgs theory and look for signatures of ‘New Physics’. 5 Part II MC based di-leptonic cross-section measurement* *based on work done for Atlas Public Note: ATL-PHYS-PUB-2009-086 6 At 14 TeV total σ(LHC) = 125 ± 25 mb σ(ttbar) = 833 ± 12% pb try to extract ~1 signal event from 20 million total. Signal Vs. Background • Dileptonic (e/μ) events are only ~5% of the ttbar crosssection. BUT • Clean channel • Distinctive trigger • No need to reconstruct top mass Z+jets W+jets 7 Event Characteristics fully leptonic 2 opposite charge leptons (e/μ) 2 neutrinos large missing energy 2 b quarks + ISR/FSR 2 or more jets 8 Experimental Object Definitions (@ 10TeV) • Electrons: – – – – shower shape requirement isolation: etcone20 < 6 GeV pt > 20 GeV 0 < |η| < 1.37 or 1.52 < |η| < 2.47 • Muons: – – – – • Jets & MET: match inner det. & spectrometer isolation: etcone20 < 6 GeV pt > 20 GeV |η| < 2.5 – – – – Cone jets pt > 20 GeV |η| < 2.5 MET>20/35GeV • Overlap*: – select electrons – remove jets within ΔR < 0.2 of electron – remove muons within ΔR < 0.3 of jet *electrons & jets share same container 9 Samples & Event Selection (@ 10TeV) sample σ * k-factor ttbar (non hadronic) 202.86 * 1.07 Weν +jets 13253.84 * 1.22 Wμν +jets 13242.22 * 1.22 Wτν +jets 13237.72 * 1.22 Zee +jets 1183.66 * 1.22 Zμμ +jets 1182.41 * 1.22 Zττ +jets 1178.57 * 1.22 Wbb 14.64 * 1.22 WW 15.62 * 1.69 WZ 1.37 * 1.42 ZZ 4.87 * 1.81 single top (t-channel) 41.12 * 1.05 single top (W-channel) 14.41 * 0.99 • single flavor channel (ee, μμ): – trigger: 2 high-pt leptons (EF_e15_medium , EF_mu15, resp.) – two opposite charged leptons, pt > 20 GeV & |η|<2.5 – Etmiss > 35 GeV – ≥ 2 jets of pt > 20 GeV – Z-pole veto 86 < mll < 96 GeV • mixed flavor channel (eμ): – trigger: 2 high-pt leptons (EF e15 medium or EF mu15, resp.) – two opposite charged leptons, pt > 20 GeV & |η|<2.5 10 – Etmiss > 20 GeV *quoted errors are from sample statistics only cumulative*: exclusive*: di-electron channel selection cutflow (for L=200pb-1 @10TeV) ↑ATLAS work in Progress↓ 11 non-fully leptonic ttbar, Zee, Zμμ, Zττ, Weν, Wμν, Wτν, Wbb, WW, WZ, ZZ, t-chan, W-chan Ns=228 Nb=45 Results ATLAS work in progress • The selection procedure above results in the following S/√(S+B) ratios for 200pb-1: ee = 13.1, μμ = 16.3 and eμ = 24.5, cf. ee = 13.2, μμ = 16.4 and eμ = 24.6 from the Pub Note • with the following cross-sections: ee = 216.96 ± 23.9 pb, μμ = 217.03 ± 19.1 pb, eμ = 216.67 ± 13.4 pb σlep comb.= 217.41 ± 10.0 pb, cf. 217.06 pb* *MC@NLO sample cross-section*K-factor --from Pub. Note: ATL-PHYS-PUB-2009-086 12 Part III Study: systematic effect of jet algorithm choice 13 effect of jet algorithms • A few jet algorithms about these days... – – – – • • • • Atlas Cone (old favourite) – cone based, unsafe Kt – cluster based, IR&Collinear safe anti-Kt – cluster based, IR&Collinear safe SIS cone – cone based, IR&Collinear safe effects come from resolution & JES differences between algorithms observed distributions can change signal & background acceptances can change S/(S+B) & significance determine importance of acceptance changes • R= 0.4 for kt cut-off and SIS cone size. • Pseudo-event samples and selection same as in Top PubNote. • Main backgrounds (based on Pub Note selections) ... - ee : Zee + jets && Wenu + jets - mumu : Zmumu + jets - mix : Z tautau + jets 14 Signal & background... for L=200pb-1 @ 10TeV alg. cone Kt anti-Kt SIS cone chan. ee μμ eμ ee μμ eμ ee μμ eμ ee μμ eμ S 259 350 778 249 338 761 250 337 761 252 336 765 B 30.7 51.8 28.4 24.1 49.9 25.8 27.2 50.3 26.9 31.4 48.3 27.4 S/ 0.89 0.87 0.97 0.88 0.87 0.97 0.90 0.87 0.97 0.89 0.88 0.97 S+B S/ 15.2 17.5 27.4 14.8 17.2 27.1 15.0 17.1 27.1 15.0 17.1 27.2 √(S+B) ↑ATLAS work in Progress • Varying jet algorithm choice does not substantially effect signal or (main) background distributions. • Acceptance variance is within level of a few percent which is comparable with other systematics • Relative (i.e.S/(S+B)) selection is constant across algorithms. • S/√(S+B) varies slightly across algorithms. All compare well with Pub. Note: 15 ee: 14.2, μμ: 17.3, eμ: 26.2 Part IV Study: systematic effect of ISR model variation on simulated cross-section This research project has been supported by a Marie Curie Early Stage Research Training Studentship of the European Community’s Sixth Framework Programme under contract number (MRTN-CT-2006035606-MCnet) Special thanks to Peter Skands 16 320 = Perugia 0 Pythia tune: benchmark 321 = Perugia Pythia tune: larger ISR phase-space & harder hadron’n 322 = Perugia Pythia tune: smaller ISR phase-space & softer hadron’n ISR effects on ttbar pt spectra (hadron level) ATLAS work in progress ttbar system ATLAS work in progress tops ATLAS work in progress leptons ATLAS work in progress W bosons Initial differences in ttbar system washed-out by decay-chain 17 320 = Perugia 0 Pythia tune: benchmark 321 = Perugia Pythia tune: more pert. activity, less non-pert. particles 322 = Perugia Pythia tune: less pert. activity, more non-pert. particles ISR effects on ttbar hadrons & jets ATLAS work in progress ATLAS work in progress # cone jets hadron level FS hadrons atlfast # hadrons ATLAS work in progress hadron pt ATLAS work in progress selected Cone jets cone jet pt No. of jets determined by hadron pt not multiplicity 18 320 = Perugia 0 Pythia tune: benchmark 321 = Perugia Pythia tune: more pert. activity, less non-pert. particles 322 = Perugia Pythia tune: less pert. activity, more non-pert. particles ISR effects on sample selection • 100k events for each sample • used (close to) Pub. Note selection (see above) sample ee μμ eμ comb. ttbar 9390 +5.7% -3.5% 10975 +3.2% -4.2% 23631 +3.2% -2.7% 43996 +3.7% -3.2% W +jets 629 9.7% -25.6% -- 947 +3.5% -28.9% 1576 +6.0% -27.6% Z +jets 463 453 +10.6% -29.2% +6.4% -23.8% 3 919 +100% -33.3% +8.8% -26.6% WW +jets 323 451 +27.2% -17.0% +7.1% -22.8% 913 1687 +21.5% -15.3% +18.7% -17.6% Effects of ISR more important in background estimation 19 Summary • Completed a MC based cross-section measurement – including all relevant backgrounds (except QCD di-jets) – results in accordance with published results • Investigated the effects of jet algorithm choice – on ttbar signal and major channel backgrounds • Investigated the effects of ISR variations – on ttbar signal and selected background • Currently on MCnet studentship at CERN – working on min. bias & UE focussed analyses 20 Backup 21 non-fully leptonic ttbar, Zee, Zμμ, Zττ, Weν, Wμν, Wτν, Wbb, WW, WZ, ZZ, t-chan, W-chan Ns=228 Nb=45 selection stack plots (di-electron channel) – Jets & Etmiss ATLAS work in progress ATLAS work in progress ATLAS work in progress ATLAS work in progress 22 non-fully leptonic ttbar, Zee, Zμμ, Zττ, Weν, Wμν, Wτν, Wbb, WW, WZ, ZZ, t-chan, W-chan Ns=228 Nb=45 selection stack plots (di-electron channel) – Electrons ATLAS work in progress ATLAS work in progress ATLAS work in progress 23 Systematics (details) --from Pub. Note: ATL-PHYS-PUB-2009-086 24