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LPNHE Paris CNRS/IN2P3-Universités Paris 6&7

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Presentation on theme: "LPNHE Paris CNRS/IN2P3-Universités Paris 6&7"— Presentation transcript:

1 LPNHE Paris CNRS/IN2P3-Universités Paris 6&7
Hgg analysis at ATLAS M. Escalier, B. Laforge LPNHE Paris CNRS/IN2P3-Universités Paris 6&7 Status of TDR analysis Signal & background generation Kinematic variables Likelihood analysis Conclusion and outlooks Special thanks to Arthur for let me use his laptop for some update Thanks L. Fayard, G. Unal (discussion, feedback)

2 Status of TDR Leading Order: CTEQ 2L no K factor Pythia 5.700 ISR, FSR
Atlfast 2.0 from full reconstruction

3 Signal/B S/√B=6.5, signal & background computed at LO

4 Signal Hgg VBF direct production gg fusion associated production
WH,ZH,ttH

5 Signal pdf=CTEQ6L1 (comment of M. Spira) at Les Houches
Using correction of HDecay for decay Hgg

6 Background Irreductible background
NLO calculation using Diphox 1.2, pdf=CTEQ6M reductible background (LO Pythia), pdf=CTEQ6L1 g jet, 1 jet misidentified jet jet, 2 jets misidentified

7 Higgs mass resolution With Pythia/ATLFAST s=1.34 GeV
Next slides: use of s of full simu TDR for window 1.4 s Mgg (GeV)

8 Diphox definitions Thanks J. Ph. Guillet for help with Diphox

9 Analysis Requirements
CTEQ 6L1 pdf (LO fit), CTEQ 6M pdf for diphox (NLO) Pythia 6.210, Atlfast 2.53, Diphox 1.2 Cuts: photon candidates: pT1>40 GeV, pT2>25 GeV |h|<2.4 transition crack of |h|=1.45, Dh=0.15 considered Photon efficiency: 80% (Cf. M. Wielers) Jet rejection factor: 2900 (Cf. M. Wielers) photon Isolation cone R= ET<15 GeV In discussion (F. Derue: ) cf. Athens 4th Atlas Worshop

10 Branching ratio: depends on b mass and on QCD corrections
8.5% 56% Branching ratio: Pythia: running aQED for pythia (I mean by default) HDecay: QCD corrections more relevant No corrections aQED (better because real photons q2=0) gg fusion :compatible with papers R.Harlander and W.Kilgore   Phys Rev Lett 88,201801,2002 C.Anastasiou and K.Melnikov Nucl Phys B646,220,2002 K factor depending on higgs mass Ravindran, Smith, Van Neerven KNLO=1.76 VBF:compatible with talk of C. Oleari Total production cross-section What is the NLO Prediction ? HiGlu package (M. Spira et. al) gg fusion K=1.8 (using CTEQ6) VBF K=1.04 (using CTEQ6)

11 Ptgg>30 GeV likelihood analysis
Problem of resummation: C. Balazs has done resummation, use/compare his soft. later Ptgg contributions TDR analysis direct 16517 onef 8510 twof 883 gg background 29000 25910 g jet 5800 6737 jet jet 4600 5916 Higgs 1283 1097 S/√B 6.5 5.59 Ptgg<30 GeV Ptgg>30 GeV likelihood analysis

12 Ptgg distribution fsignal fbackground

13 Cos q* fsignal fbackground

14 Likelihood ratio R Search for optimal cut

15 Results 8.8 6 % 8.25

16 Conclusion Background: Irreductible background:
Use of NLO irreductible background Need resummation (but box is LO in Diphox) use Dixon calculations (L. Fayard, G. Unal) Does NNLO computation is possible ? reductible background: Know better the rejection factor (g jet) Then look for NLO computation of g jet, jet jet

17 Signal: gg fusion and VBF comp. at NLO (but K=f(Pt)need MC at NLO) gg fusion: Ravindran, Smith, Van Neerven KNLO is not smal (1.76), KNNLO=1.16 (use of KNNLO in the future) NNLO of VBF ? likelihood analysis:gain not so much important use neural network ? Understand background of gg jet jet with 2 tagged jets jet veto in central region


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