Klaus Rabbertz Hamburg, Germany, 03.12.2012 6. Terascale Workshop 2012 1 Klaus Rabbertz, KIT 6. Physics at the Terascale Workshop, Hamburg, 2012 Determination.

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Presentation transcript:

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Klaus Rabbertz, KIT 6. Physics at the Terascale Workshop, Hamburg, 2012 Determination of the strong Coupling from 3-Jet Rates at the Terascale Proton Structure (PDF) Proton Structure (PDF)

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Outline Motivation The Measurement Uncertainties Comparison to Theory Extraction of the strong Coupling α s Conclusions and Outlook CMS-PAS-QCD (2012). All results without explicit reference are taken from this CMS analysis! D0, PLB718 (2012) Tevatron limit published this year We'll start here...

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Jets at LHC Proton Structure (PDF) Proton Structure (PDF) Matrix Element Abundant production of jets → hadron colliders are “jet laboratories” Learn about hard QCD, the proton structure, non-perturbative effects... Hadrons

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Jets at LHC Proton Structure (PDF) Proton Structure (PDF) Matrix Element Abundant production of jets → hadron colliders are “jet laboratories” … and the strong coupling alpha_s ! Hadrons

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Jets and α s Avoids direct dependence on PDFs and the RGE of QCD Use cross-section ratios! → reduces other theor. and exp. uncertainties along the way → eliminates luminosity dependence (normalization) Choices of CMS: Ratio of inclusive 3-jet to 2-jet production Average dijet p T as scale Scalar p T sum (H T ) disfavoured Other 3-jet observables possible, see e.g. propositions by D0 M. Wobisch D0, PLB718 (2012) 56-63

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Analysis Setup CMS data of 2011 Anti-kT jet algorithm with R = 0.7 Compatible results with R = 0.5 as alternative Selection in rapidity y (1 bin): Ensure tracker coverage Two jets leading in p T must be selected Ensure hard dijet event Minimal transverse momentum p T : Alternative thresholds 50 and 100 GeV checked Alternative relative cut on hardness of 3 rd jet tested Minimal average 2-jet (27 bins): O(2000) 2-jet ev. incl. O(300) 3-jet events above 1 TeV

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Data Treatment Three single-jet triggers (highest p T threshold 370 GeV) Efficiency checked separately for incl. 2- and 3-jet events Particle-flow technique to reconstruct input objects to jet clustering Standard CMS event and jet selection criteria apply (η,p T )-dependent jet energy correction factors, typically: Correction of detector effects using Bayesian iterative unfolding (RooUnfold) Propagation of stat. uncertainties & correlations with MC toy method Cross-checked with SVD unfolding Comparison of directly unfolded ratio R 32 versus separate unfolding of inclusive 2- and 3-jet spectra

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Experimental Uncertainties Jet energy correction, known to %: Provided as 16 mutually uncorrelated sources; fully correlated within source; Gaussian behaviour assumed Dominated by absolute scale, followed by high pT extrapolation Unfolding uncertainty accounting for: Variation of jet p T spectral slopes following differences from Pythia6 Z2 (agrees with MadGraph) and Herwig Variation of jet energy resolution (JER) Addition of non-Gaussian tails to JER Luminosity (normalization) uncertainty cancels No assumptions on bin-to-bin correlations with respect to y necessary, only 1 bin considered Statistical uncertainties propagated via unfolding

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Theory Predictions Using NLOJet++ within fastNLO framework Fast recalculable NLO incl. 2- and 3-jet cross sections Same binning as the data Using global PDF sets at NNLO with fits for series of alpha_s values NNPDF21, MSTW2008, CT10 and ABM11 Difference between use of NLO vs. NNLO PDF found negligible for R 32 Scale uncertainties evaluated via 6-point scheme Max. deviations using scale factors (1/2,1/2), (1/2,1), (1,1/2), (1,2), (2,1), (2,1/2) for renormalization and factorization scales Non-perturbative corrections account for effects of multiple parton interactions and hadronization Correction below 2%, uncertainty negligible

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Data comparison to NNPDF21 Agreement within uncertainties Scale uncertainty: PDF uncertainty: Fits only above 400 GeV to avoid threshold effects Similarly described by CT10 and even better by MSTW2008 Discrepancies observed with ABM11

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Data comparison to ABM11 Discrepancies with ABM11 especially below 600 GeV Fits of the strong coupling tend versus the upper edge of the available series in alpha_s No result from ABM11 to report Much smaller gluon down to 50% at high x at the same time as preference for smaller couplings Decorrelation of gluon and alpha_s via higher twist not present in other global PDFs ? Provide ABM11 PDFs with different settings for higher twist ? To be further discussed...

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Sensitivity to alpha_s Fits only above 400 GeV to avoid threshold effects Error bars show full uncertainty including the correlated systematic ones Compatible results from NNPDF21, CT10 and MSTW2008 with χ 2 fit using correlated experimental uncertainties: α s = 106 α s = 124 Not used NNPDF21: α s (M Z ) = ± CT10: α s (M Z ) = ± MSTW2008: α s (M Z ) = ±

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Determination of alpha_s Comparison to extractions from other hadron collider experiments Although only one point shown here extraction works equally well in e.g. four subranges newly covered range PDF uncertainty: Repeat fit for each replica → get estimators for μ and σ Scale uncertainty: Repeat fit for all six variations → get maximal deviation

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Conclusions & Outlook First determination of the strong coupling at the Terascale (TeV) Running of α s tested with mostly PDF independent ratio observable R 32 No deviation from expected running, i.e. almost flat at high p T, observed as could be expected from new coloured particles e.g. gluinos More data at high pT and test of other observables may still improve achievable statistical and experimental accuracy More precise theory (jets at NNLO …) desperately wanted! Thank you for your attention!

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Backup Slides

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Data comparison to MSTW2008 and CT10

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Sensitivity to alpha _s (other PDFs) MSTW2008 CT10 ABM11

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Gluon PDF at high x HEPDATA PDF Plotter x from 0.1 to 0.8; Q 2 = GeV 2 xg(x,Q2)Ratio to NNPDF21 ABM11 CT10 MSTW % line

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Strong Coupling α s NLO alpha_s in global PDFs: ABM11: (NNLO) CT10: GJR08: HERAPDF1.5: MSTW2008: NNPDF2.1: World Summary of alpha_s 2012, S. Bethke: PDG2012 But: Jet data from hadron colliders not included! Jets at NNLO urgently needed! Recent progress reported by Th. Gehrmann at

Klaus Rabbertz Hamburg, Germany, Terascale Workshop alpha_s from inclusive Jets CDF, PRL88, 2002 Using ATLAS data CDF: D0, PRD80, 2009Malaescu/Starovoitov, EPJC72, 2012 M/S: D0: Problem: Via the PDFs assumes the validity of the running of alpha_s according to the RGE D0 explicitly restricts phase space to where the RGE is already established.

Klaus Rabbertz Hamburg, Germany, Terascale Workshop Inclusive Jets

Klaus Rabbertz Hamburg, Germany, Terascale Workshop New jet angular correlation Observable from D0 D0, arXiv:

Klaus Rabbertz Hamburg, Germany, Terascale Workshop /2+: NLO Prediction & ΔPDF Cross section ratios: Outer/inner rapidity, 3+jets/2+jets, jet R=0.7/jet R=0.5,... new physics, ~ α s, QCD shower Largest systematic uncertainties cancel: Lumi (completely), JES, JER (partially) But also the α s sensitivity except for: CMS like selection (ATLAS not very different) LO > 1 ?! K factors ~ 0.67 PDF uncertainty reduced by a factor ~ 10 in ratio # NLO = 2x7 # NLO = 2x239