qcd meeting october 1, 2004

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QCD Meeting October 1, 2004 Is it due to the hard collision? Is it due to fragmentation ? Strong polarization seen in fixed-target experiments where jet NOT observed. Polarization Tom Devlin Rutgers/CDF _

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_.  Polarization Tom Devlin Rutgers/CDF. Strong polarization seen in fixed-target experiments where jet NOT observed. Is it due to the hard collision?. Is it due to fragmentation?. QCD Meeting October 1, 2004. Status and Plans. Three known contributions to dataset: - PowerPoint PPT Presentation

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Page 1: QCD Meeting October 1, 2004

QCD MeetingOctober 1, 2004

Is it due to the hard collision?

Is it due tofragmentation?

Strong polarization seenin fixed-target experimentswhere jet NOT observed.

PolarizationTom Devlin

Rutgers/CDF

_

Page 2: QCD Meeting October 1, 2004

Status and Plans

Three known contributions to dataset: -- Signal -- Ks Background -- Continuum 2-track background

MC code exists to generate first two.Coding in progress for the third.

Plan: Generate 20 MC of each type for each real event. Mix three MC samples, in appropriate proportions to produce 20 MC events for each real event. Adjust proportions of each and assumed polarization of MC ’s to fit data.

Page 3: QCD Meeting October 1, 2004

Old Distribution Shown Last TimeFit with no Mass Constraint: Assume Daughters are p

Subtract signal, Smooth Remainder (5-bins)

Page 4: QCD Meeting October 1, 2004

Fits Without and With Mass Constraints Shown Last Time

Two Major Improvements In This

Page 5: QCD Meeting October 1, 2004

Eliminate Decay Vertices Within 8 cm of Primary Interaction

Page 6: QCD Meeting October 1, 2004

Eliminate e+e- Cut Events with M2(ee)<0.01

Page 7: QCD Meeting October 1, 2004

Signal-Noise Improved By Large Factor

Page 8: QCD Meeting October 1, 2004

Huge Improvement in Signal/NoiseExtended Momentum Range

from 2-12 GeV/c to 2-20 GeV/cStudy , Ks, Background vs.

Momentum and Flight Distance Lxy

Page 9: QCD Meeting October 1, 2004

For one bin in p and Lxy: (loose-cut ) – (tight-cut ),(tight-cut Ks), plot both vs. M2(p)

Sum of two plots = Ks + backgroundSubtract from loose-cut Number of pure

Page 10: QCD Meeting October 1, 2004

Do this for all bins, and for Ks to get Relative Number of , Ks and Background

Page 11: QCD Meeting October 1, 2004

For Each Bin in Momentum and Lxy Evaluate Fractions of , Ks and

Page 12: QCD Meeting October 1, 2004

Restrictions on Angular Distribution

Page 13: QCD Meeting October 1, 2004

Work in Progress and Planned: Fall, 2004

11 Mass-constrained fits: 2-, 2-Ks, 1-ee.11 Sum of weights over solutions = 1.0 per event.11 Use 2 = 2(MassConstraint) - 2(NoMassConstraint)11 Determine relative proportions of , Ks and background5. Modify 2nd stage analysis code to mix MC samples from , Ks, in correct proportions. Possibly as fit parameters with constraints.6. See if a believable polarization analysis can be done in one of the three coordinate systems.7. If so, do polarization in the other two coordinate systems.