Data based method for background subtraction: Z → μ + μ -

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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

description

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. Outline. Motivation. Example of application: bb Z  m + m - - PowerPoint PPT Presentation

Transcript of Data based method for background subtraction: Z → μ + μ -

Page 1: Data based method for background subtraction: Z  → μ + μ -

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.

Outline

Motivation.Example of application: bb Z + -

Method proposedSoftware & Generators

• Simulation, Reconstruction, Analysis.

Sample Conclusion and future development

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

Les Houches Guidebook hep-ph/040345

MonteCarlo

CojestIsajet Ariadne

Herwig

Sherpa

PythiaJetset

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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 rely

on alternative method to MonteCarlo, as much we can

We propose a method based on a different

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

(most copious background of bb h0/A + - 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→ +bb

~ 0.2 - 0.01 pb (even lower)

~ 22.8 pb

Zbb → -+ bb

(Pythia 6.226)AcerMC (v.2.3) interfaced with 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 method

proposed based on

Z→ and Z→ e+ e-

Relying on experimental data

Br( h0→ e+ e-) neglegible

Different Inner Bremsstrahlung

Precise Knowledge of background is crucial

2

em

m

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

Z production

bbbhbgg

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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 events In 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 → -+ bb () N ~ 0.086 Nev=464522 Zbb → e-e+ bb () N ~ 0.157 Nev=442828Different Detector ResponseThe most significative variable of bb h0/A + - 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

N MC ~ 0.157N MC ~ 0.086

Zbb → + bb Zbb → ee+ bb

e

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

Bremsstrahlung PhotonsZbb → ee+ bbZbb → +

bb

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

Generator level: Zbb → -+ bb

MMinv(+-) Minv(+-)

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

Generator level: Zbb → -+ bb

Only events with a of Bremsstrahlung

Minv(+-) Minv(+-)

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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-)

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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-)

Only events with a 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

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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 → -+ bb

Bremsstrahlung photonsAll photons

PT vs. Distance between and 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 → -+ bb

Distance between and 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+ bb

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

22 φηR

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+ bb

Distance between and e

All photons Bremsstrahlung photons

watch the different

scale!

R ~ 0.25

22 φηR

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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 combined 4-momentum is measured. For the 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, and 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 ( 0.025, =0.05 ) and PT >5GeV, || >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 → -+ bbZbb → bb

PT > 5 GeV || >2.7 recontructed

Zbb → e-e+ bb

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

Reconstruction Muons: combined reconstruction (inner detector +

spectrometer), PT >10 GeV, || >2.5. Electrons: energy measured in calorimeter,() measured from

tracker, PT >10 GeV , || >2.5. Photons: e.m. cluster without track associated :

0.025, =0.05, PT > 5 GeV, || >2.5. Brem photons: >2 leptons reconstructed + reconstructed in a cone around lepton direction < R. Electrons sample only one cluster is reconstructed. Muon sample: track near photon cluster, misidentification. The number events reconstructed with brem identified is at

percent level.

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

Reconstruction: Zbb → -+ bb

Minv(+-)Minv(+-)

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

Reconstruction: Zbb → -+ bb

Minv(+-)Minv(+-)

Only events with a of Bremsstrahlung

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

Reconstruction: Zbb → e-e+ bb

Minv(e+e-)Minv(e+e-)

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

Reconstruction: Zbb → e-e+ bb

Minv(e+e-)Minv(e+e-)

Only events with a of Bremsstrahlung

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

Reconstruction

Only events with a of Bremsstrahlung

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

Reconstruction

The number bremsstrahlung reconstructed separatly in muons events is higher than electron events, where are mostly absorbed in the electron cluster

Page 34: Data based method for background subtraction: Z  → μ + μ -

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 + - 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 reasonably stable and the effect of Bremsstrahlung is negligible with respect to detector responseThe same method can be applied to H→ 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

0.025 =0.05Isolation broad 0.05 =0.10

R =0.07 size of cluster 5x 5 = 0.025 =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.