Data based method for background subtraction: Z · 2006-04-20 · Jetset Herwig Pythia. Halina...

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni Nicoletti Higgs Meeting 18 April 2006,CERN. Data based method for background subtraction: Z →μ + μ - Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni Nicoletti Laboratori Nazionali di Frascati, Università di Roma La Sapienza, INFN

Transcript of Data based method for background subtraction: Z · 2006-04-20 · Jetset Herwig Pythia. Halina...

Page 1: Data based method for background subtraction: Z · 2006-04-20 · Jetset Herwig Pythia. Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni Nicoletti Higgs Meeting 18

Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Data based method for background subtraction:

Z →μ+μ-

Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni Nicoletti

Laboratori Nazionali di Frascati, Università di Roma La Sapienza, INFN

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

OutlineMotivation.Example of application: bb Z → µ+ µ-

Method proposedSoftware & Generators• Simulation, Reconstruction, Analysis.

Sample Conclusion and future development

Page 3: Data based method for background subtraction: Z · 2006-04-20 · Jetset Herwig Pythia. Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni Nicoletti Higgs Meeting 18

Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

MonteCarloIsajet Ariadne Sherpa

Les Houches Guidebook hep-ph/040345Cojest

JetsetPythiaHerwig

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Shower MonteCarlo

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Motivation

It is then extremely important to relyon alternative method to MonteCarlo, as much we

canWe propose a method based on a different

data sample of experimental dataOnly hypothesis: lepton universality.Example of application: bb Z → µ+ µ-

(most copious background of bb h0/A → µ+ µ- studies (14/12/2005) S.G. presentation, ATLAS-PHYS-2003-015, June 2003.)

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Signal & background

h0 bb→ µ− µ+bb

σ~ 0.2 - 0.01 pb(even lower)

σ ~ 22.8 pb

Zbb → µ-µ+ bb

(Pythia 6.226)AcerMC (v.2.3) interfacedwith Pythia 6.2 (hep/ph0405247).

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Background Subtraction Method

Experimental methodproposed based onZ→ µ+ µ− and Z→ e+ e-

Relying on experimental data

Br( h0→ e+ e-) neglegible

Different Inner Bremsstrahlung

Precise Knowledge of background is crucial

2

⎟⎟⎠

⎞⎜⎜⎝

⎛∝

emm µ

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Z production

bbbhbgg −+→→ µµ

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Software Release & SampleGeneration Athena 9.0.4 - Pythia (v.6.226) - Acer (v. 2.3)Simulation, Digitalization, Reconstruction Athena 10.0.1Analysis based on CBNT (root –ntuples).Final study in scenario

~ 600000 eventsIn this presentation Lint ~ 20 fb-1

~ 400000 events

∫ −= 130 fbLdt

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Study performedDifferent Inner Bremsstrahlung

Zbb → µ-µ+ bb (γ) Nγ ~ 0.086 Nev=464522Zbb → e-e+ bb (γ) Nγ ~ 0.157 Nev=442828Different Detector ResponseThe most significative variable of

bb h0/A → µ+ µ- analysis has be chosen Minv as test .NB. The combination of a same flavor lepton originating from b and one of Z are included inevitably in the plots

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Bremsstrahlung Photons

NγMC ~ 0.157Nγ

MC ~ 0.086

Zbb → µ−µ+ bb Zbb → e−e+ bb

e

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Bremsstrahlung PhotonsZbb → e−e+ bbZbb → µ−µ+ bb

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level: Zbb → µ-µ+ bbMinv(µ+µ-) Minv(µ+µ-)γ

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level: Zbb → µ-µ+ bbMinv(µ+µ-) Minv(µ+µ-)γ

Only events with a γ of Bremsstrahlung

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level: Zbb → µ-µ+ bb

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level: Zbb → e-e+ bbMinv(e+e-) Minv(e+e-)γ

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level: Zbb → e-e+ bbMinv(e+e-) Minv(e+e-)γ

Only events with a γ of Bremsstrahlung

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level: Zbb → e-e+ bb

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level

Bremsstrahlung events

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generator level

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Leptonsmuons electrons

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Photons: Zbb → µ-µ+ bbBremsstrahlung photonsAll photons

PT vs. Distance between γ and µ watch the different scale!Subsample(~25000 ev)

22 φηR ∆+∆=∆

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Photons: Zbb → µ-µ+ bb

Distance between γ and µ watch the different scale!

∆R ~ 0.15

All photons Bremsstrahlung photons

22 φηR ∆+∆=∆

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Photons: Zbb → e-e+ bb22 φηR ∆+∆=∆

PT vs. Distance between γ and e watch the different scale!Subsample(~25000 ev)

All photons Bremsstrahlung photons

5x5 cluster in ATLAS

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Photons: Zbb → e-e+ bbAll photons Bremsstrahlung photons

∆R ~ 0.25

22 φηR ∆+∆=∆

Distance between γ and e watch the different scale!

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

PhotonsIf the photon is emitted close to electron,

only one cluster is reconstructed and the combined4-momentum is measured. For the γ is effectively absorbed in the same cluster of the electron.

corresponds to a 5x5 cluster in ATLAS. The energy of electron is measured in e.m. calorimeter, θ and φ are measured in tracker.Photons, inside cone ∆R, are taken in account summing their 4-momentum to the 4-momentum of the nearest lepton. Photons reconstructed are e.m. clusters without track associated (∆η= 0.025,∆φ =0.05 ) and PT >5GeV, |η| >2.5.

Rφη ∆<∆+∆ 22

125.022 =∆+∆=∆ φηR

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

All Photons: Zbb → µ-µ+ bbZbb → µ−µ+ bb Zbb → e-e+ bb

PT γ> 5 GeV |η| >2.7 recontructed γ

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

ReconstructionMuons: combined reconstruction (inner detector + spectrometer), PT >10 GeV, |η| >2.5.Electrons: energy measured in calorimeter,(θ,φ) measured from tracker, PT >10 GeV , |η| >2.5.Photons: e.m. cluster without track associated :

∆η= 0.025, ∆φ =0.05, PT > 5 GeV, |η| >2.5.Brem photons: >2 leptons reconstructed +

γ reconstructed in a cone around lepton direction < ∆R. Electrons sample only one cluster is reconstructed. Muon sample: µ track near photon cluster, misidentification.

The number events reconstructed with γ brem identified is atpercent level.

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Reconstruction: Zbb → µ-µ+ bb

Minv(µ+µ-)γMinv(µ+µ-)

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Reconstruction: Zbb → µ-µ+ bb

Minv(µ+µ-)γMinv(µ+µ-)

Only events with a γ of Bremsstrahlung

Page 32: Data based method for background subtraction: Z · 2006-04-20 · Jetset Herwig Pythia. Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni Nicoletti Higgs Meeting 18

Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Reconstruction: Zbb → e-e+ bb

Minv(e+e-)γMinv(e+e-)

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Reconstruction: Zbb → e-e+ bbMinv(e+e-) Minv(e+e-)γ

Only events with a γ of Bremsstrahlung

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Reconstruction

Only events with a γ of Bremsstrahlung

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Reconstruction

The number γ bremsstrahlung reconstructed separatlyin muons events is higher than electron events, where are mostly absorbedin the electron cluster

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generation-reconstruction

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Generation-reconstruction

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

ConclusionsA study for an experimental method of background subtraction is developed based on fully simulated samples, Lint ~ 20 fb-1 of:

bb Z → µ+ µ- and bb Z → e+ e-

comparing:the Bremsstrahlung of the two samples.the ATLAS detector response.

The study is preliminary and needs careful tuning on data collected.∆R is an extremely important parameter, that should be carefully tuned.

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

ConclusionsIn the region Minv 98 -135 GeV the ratio is reasonablystable and the effect of Bremsstrahlung is negligible with respect to detector responseThe same method can be applied to H→ ττ and in general to all decays where the electron decay is negligible in the signal.The method relies on lepton universality and needs a good knowledge of detector response for different leptonsThe method doesn’t need an implementation on MC of higher order corrections

Acknowledgements: Borut Kersevan, Dirk Zerwas,Donatella Cavalli

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Riserve

Riserve

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

Matching track narrow∆η= 0.025 ∆φ =0.05

Isolation broad∆ η= 0.05 ∆φ =0.10

∆R =0.07 size of cluster 5x 5 ∆η= 0.025 ∆φ =0.05

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.

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Halina Bilokon, Vitaliano Chiarella, Simonetta Gentile, Giovanni NicolettiHiggs Meeting 18 April 2006,CERN.