Charged Hadrons IP resolution in -decays and reconstruction of CP- - - PowerPoint PPT Presentation

charged hadrons ip resolution in decays and
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Charged Hadrons IP resolution in -decays and reconstruction of CP- - - PowerPoint PPT Presentation

Charged Hadrons IP resolution in -decays and reconstruction of CP- mixing angle in H A. Raspereza, A. Tumasyan Outline PV resolution in ggF / VBF H processes Charged hadron IP resolution in + and


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Charged Hadrons IP resolution in τ-decays and reconstruction of CP-mixing angle in H→ττ

  • A. Raspereza, A. Tumasyan
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Outline

  • PV resolution in ggF / VBF H→ττ processes
  • Charged hadron IP resolution in τ ± → π± + ν

and τ ± → π± + π0 + ν

  • CP-mixing angle reconstruction in ggF/VBF

H→ττ

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General Information

Datasets

Fall17 MC /GluGluHToTauTau_M125_13TeV_powheg_pythia8/RunIIFall17MiniAOD- 94X_mc2017_realistic_v10-v1/MINIAODSIM /VBFHToTauTau_M125_13TeV_powheg_pythia8/RunIIFall17MiniAOD-94X_mc2017_realistic_v10- v1/MINIAODSIM Phase II MC samples with noPU: /GluGluHToTauTau_M125_14TeV_powheg_pythia8/PhaseIITDRFall17MiniAOD- noPU_93X_upgrade2023_realistic_v2-v1/MINIAODSIM /VBFHToTauTau_M125_14TeV_powheg_pythia8/PhaseIITDRFall17MiniAOD- noPU_93X_upgrade2023_realistic_v2-v1/MINIAODSIM Phase II MC samples PU=200 /GluGluHToTauTau_M125_14TeV_powheg_pythia8/PhaseIITDRFall17MiniAOD- PU200_93X_upgrade2023_realistic_v2-v2/MINIAODSIM /VBFHToTauTau_M125_14TeV_powheg_pythia8/PhaseIITDRFall17MiniAOD- PU200_93X_upgrade2023_realistic_v2-v2/MINIAODSIM

CMSSW_9_4_0_patch1 Selected events with Ptτ > 35, ητ < 2.3, and decay mode ≤ 1 Gen-Reco τ-matching with cone 0.3

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RECO PV vs GEN PV in ggF H→ττ

difference of charged hadron Vx, Vy, Vz Reco - Gen X Y Z

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RECO PV vs GEN PV in VBF H→ττ

difference of charged hadron Vx, Vy, Vz Reco - Gen

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Impact Parameter of charged hadron

PV Charged hadron Vertex Leading (in our case the only) charged hadron momentum Closest approach IP vector

Linear extrapolation was used for IP vector determination

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RECO IP vs GEN IP in ggF H→ττ

difference of charged hadron IPx, IPy, IPz Reco - Gen

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RECO IP vs GEN IP in VBF H→ττ

difference of charged hadron IPx, IPy, IPz Reco - Gen

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RECO IP vs GEN IP in ggF H→ττ wrt Gen-Vertex

difference of charged hadron IPx, IPy, IPz Reco – Gen wrt Gen PV

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CP-mixing angle reconstruction in H→ττ

  • Eur. Phys. J. C (2014) 74:3164

CP-mixing angle: φ*CP is

  • 1. prong 0

τ

+ → π + + ν

τ

  • → π
  • + ν

Angle between normalized IP*┴ of charged hadrons in π

+ π

  • - ZMF
  • 2. prong 1

τ

+ → ρ + + ν → π + + π 0 + ν

τ

  • → ρ
  • + ν → π
  • + π

0 + ν

Angle between transverse components of neutral hadrons (π

0) momentums in

π

+ π

  • - ZMF
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CP-mixing angle reconstruction in H→ττ

prong 0-0 τ

+ → π + + ν and τ

  • → π
  • + ν

Angle between normalized IP*┴ of charged hadrons in π

+ π

  • - ZMF

where arXiv:1510.03850v1

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CP-mixing angle reconstruction in H→ττ

prong 1-1 τ

+ → ρ + + ν → π + + π 0 + ν and τ

  • → ρ
  • + ν → π
  • + π

0 + ν

Angle between PT of neutral hadrons (π

0) in π + π

  • - ZMF

where arXiv:1510.03850v1

2 categories: yτ > 0 or yτ < 0

where

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CP-mixing angle reconstruction steps and combination

  • First we set 4-momentum of charged hadrons: q+ and q–
  • Reconstruction of charged hadron IP vector for 0-prong and

constructing (0, IP) 4-vector, or using 4-momentum vector of π

0 for

1-prong. Let’s denote these vectors p+ and p–

  • Boost to π

+ π

  • - ZMF and normalization: 𝑟

*± and 𝑞 *±

  • For 1-prong yτ sign needs to be determined (for 0-prong it always +)
  • If yτ < 0 then φ* = arcos (𝐪

*+

┴ · 𝐪

*–

┴) should be shifted by π to

combine with yτ > 0 category where φ* = arcos (𝐪 *+

┴ · 𝐪

*–

┴)

= 𝐫

*– · (𝐪 *+

┴ × 𝐪

*–

┴)

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CP-mixing angle in ggF H→ττ for various categories of yτ

yτ > 0 yτ < 0 yτ > 0 and shifted yτ < 0

Fall17 samples Generator Level

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CP-mixing angle with Fall17, Upgrade_noPU and Upgrade_200PU samples

Gen Reco Gen Reco

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CP-mixing angle: ggF vs VBF (Fall17)

ggF ggF VBF VBF

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What can be done to improve the results (separation power of φ*CP)

  • Propagation of charged hadron track to the point of closest

approach taking into account magnetic field (might be better IP resolution)

  • PV refitting excluding tracks from τ-decays

(might be better IP resolution)

Thank You