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Herwig++ News Herwig++ Keith Hamilton Universit degli Studi di Milano-Bicocca Monday, 6 September 2010 Bhr Gieseke Gigg Herwig++ Grellscheid Latunde-Dada Pltzer Richardson Seymour Tully Webber Monday, 6 September 2010 Main


  1. Herwig++ News Herwig++ Keith Hamilton Università degli Studi di Milano-Bicocca Monday, 6 September 2010

  2. Bähr Gieseke Gigg Herwig++ Grellscheid Latunde-Dada Plätzer Richardson Seymour Tully Webber Monday, 6 September 2010

  3. Main News: NLO POWHEG simulations A method for including NLO corrections in a parton shower simulation [Nason - 2004, Frixione, Nason, Oleari - 2007]. A POWHEG code just outputs weight +1 events, according to NLO+[N]LL resummed distributions, as Les Houches event files. Hadronize non-radiative events and shower radiative events using any shower MC. Monday, 6 September 2010

  4. POWHEG Hardest emission: Always generated according to the NLO real ME [in A.O. shower ≠ 1st radiation hardest] Shower independent: Easy to make [we did it!] Easier for attempting complex NLO processes Insensitive to shower problems / development / fixes [kinematics reconstruction of HW++ has changed 3 times] Opens the door for the NLO community Only weight +1 events: Conventional statistical analysis Easier to attack complex analysis [NN’s, DA’s, ...] Monday, 6 September 2010

  5. Angular ordering QCD coherence can be implemented, approximately, in shower MC’s by ordering emissions by their angle. For an A.O. shower the first emission isn’t a priori the hardest: H Monday, 6 September 2010

  6. Angular ordering QCD coherence can be implemented, approximately, in shower MC’s by ordering emissions by their angle. For an A.O. shower the first emission isn’t a priori the hardest: H Monday, 6 September 2010

  7. Angular ordering When POWHEG gives a real emission according to the NLO calculation it’s supposed to be the hardest. So in general you just veto emissions from the shower with p T > p T,POWHEG H POWHEG real emission [Nason 2004, Implementation KH, Richardson, Tully 2008] Monday, 6 September 2010

  8. Angular ordering When POWHEG gives a real emission according to the NLO calculation it’s supposed to be the hardest. So in general you just veto emissions from the shower with p T > p T,POWHEG H POWHEG real p T vetoed shower emission [Nason 2004, Implementation KH, Richardson, Tully 2008] Monday, 6 September 2010

  9. Angular ordering When POWHEG gives a real emission according to the NLO calculation it’s supposed to be the hardest. So in general you just veto emissions from the shower with p T > p T,POWHEG H POWHEG real p T vetoed shower emission But if the shower is A.O. then the shower should also try to include ‘earlier’ soft wide angle emissions [Nason 2004, Implementation KH, Richardson, Tully 2008] Monday, 6 September 2010

  10. Angular ordering When POWHEG gives a real emission according to the NLO calculation it’s supposed to be the hardest. So in general you just veto emissions from the shower with p T > p T,POWHEG H POWHEG real p T vetoed shower emission soft truncated shower But if the shower is A.O. then the shower should also try to include ‘earlier’ soft wide angle emissions [Nason 2004, Implementation KH, Richardson, Tully 2008] Monday, 6 September 2010

  11. Herwig++ in-house POWHEGs Shipping with the current release: hh ➞ γ / Z / W / H / ZH / WH [KH, Richardson, Tully] Spin correlations in decays [also for real emissions] Truncated showers Also available in Contrib: POWHEG top and Higgs decays [Latunde-Dada] Monday, 6 September 2010

  12. Herwig++ in-house POWHEGs Shipping in a few months: VBF [Under validation - D’Errico, Richardson] hh ➞ WZ / ZZ / WW [Validated - KH] Longer term: Enhance compatibility with POWHEG-BOX [see Re’s talk] Colour coherent CKKW [JHEP 0911:038,2009] Monday, 6 September 2010

  13. ☞ Herwig++ POWHEG validation 1. MCFM: Total cross sections agree at O(0.1%) O(20) IR safe distributions checked; ‘Born variables’ are scrutinized and show excellent agreement. 2. MC@NLO + 3. Matrix Element Corrections: Shift focus to resummation & radiation generation i.e. here we wanted to check the shapes normalized to 1. Good agreement in all 3 approaches. POWHEG & ME Corr tend to have harder spectrum [and we understand why]. 4. Data: For e+e- and DY we compared to the data. Monday, 6 September 2010

  14. Results Drell-Yan vector boson production _ l h A q _ W, Z / γ q h B l [KH, Richardson, Tully] Monday, 6 September 2010

  15. Results: Drell-Yan vector boson production W boson p T spectrum compared to D0 run I data Solid line: NLO Herwig++ POWHEG Blue dashes: MC@NLO Red dashes: Herwig++ with ME corrections Monday, 6 September 2010

  16. Results: Drell-Yan vector boson production Z boson p T spectrum compared to D0 run II data Solid line: NLO Herwig++ POWHEG Blue dashes: MC@NLO Red dashes: Herwig++ with ME corrections Monday, 6 September 2010

  17. Results Higgs production via gluon fusion g t H t t g [KH, Richardson, Tully] Monday, 6 September 2010

  18. Results: Higgs production via gluon fusion Higgs boson rapidities compared to fixed order NLO calculations gg → H → τ + τ - Red: NLO Herwig++ POWHEG Black: NLO MCFM fixed order Magenta: LO Herwig++ POWHEG Dashes: LO MCFM fixed order Monday, 6 September 2010

  19. Results: Higgs production via gluon fusion _ x 1/s 1 max 1 [ LHC m H =115 GeV ] shower a y dead zone shower b - 1 Monday, 6 September 2010

  20. Results Higgs-strahlung _ W, Z q W * , Z * q H [KH, Richardson, Tully] Monday, 6 September 2010

  21. _ - - Results: Higgs-strahlung (qq ➞ HZ/W ) Polar angle of electron vs fixed order NLO calculations: Tevatron Red: NLO Herwig++ POWHEG Black: NLO MCFM fixed order Magenta: LO Herwig++ POWHEG Dashes: LO MCFM fixed order Monday, 6 September 2010

  22. _ Results: Higgs-strahlung (qq ➞ HZ) Monday, 6 September 2010

  23. _ Results: Higgs-strahlung (qq ➞ HW) j q q h h HW Monday, 6 September 2010

  24. _ Results: Higgs-strahlung (qq ➞ HW) j q q h h HW Monday, 6 September 2010

  25. Results: Diboson production h A W, Z q _ q W, Z h B h A W, Z q W, Z, γ _ q W, Z h B [KH] Monday, 6 September 2010

  26. Results: Diboson production at LHC [KH, in preparation] LO total inclusive cross section PS has half as many 80 GeV jet events [LL approx] Direction of hard jets not like the NLO real correction Monday, 6 September 2010

  27. Results: Diboson production at LHC Monday, 6 September 2010

  28. Results: Diboson production at LHC Factor of 3 enhancement in LO distribution! Really “soft” W emission from hard quark qg ➞ qZ ➞ qWZ Also big enhancement due to incident gluon flux [Nason et al] Monday, 6 September 2010

  29. Results VBF q W, Z H W, Z q , [D’Errico, Richardson] Monday, 6 September 2010

  30. Results: VBF Rapidity of Higgs at NLO Herwig++ VBFNLO LHC 14 TeV [D’Errico, Richardson] Monday, 6 September 2010

  31. Results: VBF p T of Higgs at NLO Herwig++ VBFNLO LHC 14 TeV [D’Errico, Richardson] Monday, 6 September 2010

  32. Other news Multiple Interactions Colour Coherent Formulation of CKKW Monday, 6 September 2010

  33. Multiple Parton Interations ‣ Original Herwig: UA1 model of the soft UE but option to link to JIMMY model of MPIs ‣ Herwig++:built in MPI model building on JIMMY technology. Herwig++ CDF [Bahr, Butterworth, Gieseke, Seymour] Monday, 6 September 2010

  34. Colour Coherent CKKW: LEP jet rates ME Corrs JHEP CKKW 0911:038,2009 merging scale variation [& jet Eur.Phys.J.C measure] 17:19-51, 2000 [KH, Richardson, Tully] Monday, 6 September 2010

  35. Colour Coherent CKKW: fit to LEP data CKKW tune at y merge = 10 -2 gives much better fit to LEP data than standard tune [HW++ with ME corrections]: Hw+ME χ 2 / d . o . f CKKW χ 2 / d . o . f Observable Thrust 23.48 10.62 Sphericity 5.638 0.580 Oblateness 2.450 0.339 Planarity 1.249 1.211 y 23 2.400 0.867 y 34 1.887 1.026 y 45 4.571 2.018 cos α 34 0.569 3.301 cos χ BZ 1.002 0.775 cos Φ KSW 1.469 1.337 cos θ NR 4.509 0.702 [KH, Richardson, Tully] Monday, 6 September 2010

  36. Colour Coherent CKKW: CDF jet E T spectra W+jets: E T of 2nd Jet W+jets: E T of 3rd Jet CDF 2008 PRD77:011108 [Richardson, Tully] Monday, 6 September 2010

  37. Main news summary Herwig++ ships with the following in-house POWHEG codes: hh ➞ γ / Z / W / H / ZH / WH All processes underwent lengthy validations via comparison with MCFM, MC@NLO, ME Corrections and real data. The only sizeable discrepancies found were in p T spectra and rapidity correlations w.r.t. MC@NLO for gg ➞ H. Our studies conclude that these discrepancies stem from the dependency of MC@NLO on the underlying shower MC, in particular its phase space partitioning [should not occur in MC@NLO+PYTHIA]. VBF is being validated and WW/ZZ/WZ production is validated: HW++ will ship with these in the coming months. Monday, 6 September 2010

  38. Bonus material Monday, 6 September 2010

  39. Results: Drell-Yan vector boson production Z boson rapidity compared to D0 run II data Solid line: NLO Herwig++ POWHEG Red dashes: MC@NLO Blue dashes: Herwig++ Monday, 6 September 2010

  40. Radiative phase space variables: x & y NLO real emission correction: g+g → H+g g 1-x g g θ h A h B H Monday, 6 September 2010

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