cigdem issever on the behalf of cdf collaboration

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22.05.2005 IOP 2005 Cigdem Issever, Universit y of Oxford 1 Measurement of the Forward-Backward Charge Asymmetry from W -> e Production in Collisions at = 1.96 TeV hep-ex/0501023 Cigdem Issever On the behalf of CDF Collaboration s pp more information: http://fcdfwww.fnal.gov/physics/ewk/2004/w_charge_asym/ w_charge_asymmetry.html CDF

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Measurement of the Forward-Backward Charge Asymmetry from W -> e n Production in Collisions at = 1.96 TeV hep-ex/0501023. Cigdem Issever On the behalf of CDF Collaboration. more information: http://fcdfwww.fnal.gov/physics/ewk/2004/w_charge_asym/w_charge_asymmetry.html. - PowerPoint PPT Presentation

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Page 1: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

1

Measurement of the Forward-Backward Charge Asymmetry from W -> e Production in Collisions at

= 1.96 TeV hep-ex/0501023

Cigdem IsseverOn the behalf of CDF Collaboration

s

pp

more information:http://fcdfwww.fnal.gov/physics/ewk/2004/w_charge_asym/

w_charge_asymmetry.html

CDF

Page 2: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

2

PDFs significant for many measurements at the Tevatron

How can we gain insights into parton momentum distribution functions (PDFs) of the proton at the Tevatron???

Measure W Charge Asymmetry

Ad(W ) /dyW d (W ) /dyWd(W ) /dyW d (W ) /dyW

PDFs not well known at high x (high )Don’t already know the answer, need to measure.Can improve many of our upcoming measurements.

Page 3: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

3

Reason for W Charge Asymmetry?

u quarks carry more momentum than d quarks

xf(

x,Q

2)

x

Q2 = 100 GeV2

MRST2004NLO

u

d

10-3 10-2 10-1

Page 4: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Reason for W Charge Asymmetry?

W+

dp

u

u

d

pu

u

e+

W- W+

protonantiproton

W+ and W- boosted in forward and backward direction; Information about u(x)/d(x) convoluted in W Asymmetry

Page 5: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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sensitive to PDF’s !

Measure Charge Asymmetry of Lepton Channel

Asymmetry in W production complicated by unknown pz

use lepton asymmetry:

which convolves W production with V-A decay.

uncertainty on PDF’s significant error in several measurements at CDF !

Page 6: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

6

CDF Run1 Result

Forward Tracking and Charge ID is the key!!

Measurement at large has high impact on PDF fits

Page 7: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Calorimeter Seeded OI Si-Tracking (PHX)

Forward Tracking outside COT

Seed tracksSi-track

Si-Hit

1) Reconstruction of Seed Track with

o Calorimeter cluster position

o Event vertex

o Calorimeter cluster ET

2) Reconstruction of Si-Tracks

o Using same algorithm as the COT OI Si-Tracking to attach Si hits.

vertex

Seed tracks

Page 8: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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W Event Selection• Baseline electron selection

• PHX track optimized for good charge identification:– #hits > 4

– 2 < 8

– 2 > 0.5

– Pull Ratio

• ET > 25 GeV

• Missing ET > 25 GeV

• 50 < MT < 100 GeV/c2

• No other EMO with ET>25 GeV to suppress QCD and DY

Page 9: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Needs to be corrected for

- background contributions and

- charge misidentification.

Raw, uncorrected Charge Asymmetry

Page 10: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Charge Identification

Incorrectly identified charge dilutes asymmetry.We can correct for it, if we know f=#wrong/total.

MC does not include residual misalignments. Must measure it in data as function of .

Measure f with Ze+e-.Use central (|| < 1.5) leg to tag charge of other leg.

Page 11: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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PHX Charge Misidentification Rate

Smaller than 6% in forward

Error calculated with Bayesian prescription

Page 12: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

12

Correction of Raw Asymmetry for Charge MisID

with f+ charge mis-id rate of positrons, f- charge mis-id rate of electrons

A charge dependence of charge id would directly bias measurement, hence: A = (Araw+ f+ - f-) / (1 - f+ - f-)

Page 13: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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We correct the asymmetry in each bin for backgrounds from

–W eAsymmetric, measured from MC, 4%

–Z e+ e-

Asymmetric, measured from MC, 1%

–QCDSymmetric, measured from data using

Isolation vs MEt.

Background Corrections

Page 14: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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QCD Background (BKG)

upper limit

We use (0.5 ± 0.25)*BKG. Becomes significant for >1.8

Page 15: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

15

Corrected Asymmetry with stat + total uncertainties

No evidence of CP asymmetry, level of agreement 2/dof=9.5/11.We are using method by R. Barlow, PHYSTAT2003, SLAC, Stanford, California, September 8-11, 2003, for incorporating the asymmetric uncertainties in the error propagation using likelihood distributions.

Page 16: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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For higher ET electrons, is closer to yW.

More information can be gained by

measuring A in bins of electron ET.

Current statistics allow use of two ET bins.

NEW : ET Dependence of Asymmetry

25 GeV < ET < 35 GeV

35 GeV < ET < 45 GeV

Page 17: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Results for 25 GeV < ET < 35 GeV

--- MRST02__ CTEQ6.1M

NLO RESBOS

Corrections for charge mis-id and backgrounds are measured and applied for each ET bin.

Page 18: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Results for 35 GeV < ET < 45 GeV

--- MRST02__ CTEQ6.1M

NLO RESBOS

2 probabilities are 11% for CTEQ and 0.6% for MRSTInclusion of our results will further constrain fits and improve predictions.

Page 19: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Outlook & Conclusion

• Results will be included into new PDF fits.

• CDF is beginning to explore a new method which fully reconstructs the W direction, see talk of Boyoung Han at APS 2005.

• CDF Run2 W Charge Asymmetry measurement provides new PDF constraints, particularly when separated by ET range.

• Measured Asymmetry for the first time in different ET bins.

Page 20: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Backup Slides

Page 21: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Systematic• Statistical uncertainty on charge mis-id rate dominates

• Uncertainty from QCD jet background is small and other backgrounds are negligible

• Using COT tracks, when available, results in no significant difference

• Checked that variation of detector alignments within their uncertainty has no significant effect on asymmetry

• No difference between asymmetry in the EAST and WEST

• Studied possible biases introduced by detector effects in the MC and found no significant effects.

Page 22: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Results: W Charge Asymmetry w. total error

Page 23: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Corrected W Charge Asymmetry Et>25 GeV

Page 24: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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CDF Run 2 Detector

Page 25: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Plug/PES Alignment Align PLUG calorimeter with COT tracks: allow offsets in x,y,z and a rotation in phi

global misalignments2<<8mrad;x,y ~3mm

internal misalignments~1mrad, r~1mm

PES Octant Boundary

Page 26: Cigdem Issever On the behalf of CDF Collaboration

22.05.2005IOP 2005

Cigdem Issever, University of Oxford

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Background Determination Method Is

ola

tion

MET [GeV]

0.

1

0.

4

0.

7

1.0

20 60 100 140

Signal Region