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W/Z Plan For Winter Conferences

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W/Z Plan. For Winter Conferences. Tom Diehl. FNAL _at_ Saclay 12/2001. W/Z Group's Charge. Goals for spring conferences: Z- mm (ee) Mass & Cross Sections ... – PowerPoint PPT presentation

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Title: W/Z Plan For Winter Conferences


1
W/Z Plan For Winter Conferences
  • Tom Diehl
  • FNAL
  • _at_ Saclay 12/2001

2
W/Z Groups Charge
  • Goals for spring conferences
  • Z-gt mm (ee) Mass Cross Sections
  • W-gt mn (en) Transverse Mass and Cross Sections
  • W-gt mg (eg) Event Displays
  • My take on these goals Selected because
    they demonstrate that the upgraded detector is
    shaping up
  • Show that the new muon detectors and trigger will
    do their jobs
  • Its Most important that we demonstrate the
    capabilities of the new central tracker.

3
W/Z Groups Charge
  • Ambitious
  • We will achieve the results in the electron
    channels with O(100s) of events.
  • Muons are more challenging because weve been
    limited by the trigger bandwidth and because the
    CFT trigger is late.
  • Z-gtmm definitely, maybe W-gtmn
  • Use the Tracker! Why?
  • Zs and Ws are cleaner.
  • pT resolution is much better than the rest of the
    muon detector
  • We will be using it in the long run We should
    learn to use it now.

4
WZ Groups Plan
  • Data Collection
  • WZ_Reco (see Georgs talk)
  • La Macchina (Selecting from Reco_S events)
  • Efficiency Calculation
  • The plan - what we are doing
  • I wrote down some equations - shows my bias for
    using the tracker in the selection
  • Background Estimate
  • Examples

5
Efficiency Calculation
  • Partly from Monte Carlo.
  • Monte Carlo calculates acceptance kinematic
    selection
  • Monte Carlo doesnt model the detector
    performance
  • Partly from Data
  • Use Data whenever possible
  • See above in reverse for Data

6
Efficiency Calculation
  • Loose is fraction of signal which passes the
    Loose selection criteria in MC.
  • Tight is efficiency of Tight cuts w.r.t.
    Loose cuts.
  • 5 components
  • Take care that all of Loose is in the
    denominator
  • Take care there are several ways for one muon
    to be reconstructed as two or more
  • The multiple NSEG thing
  • Multi-region muons

7
Efficiency Calculation
  • For Ws, Trigger is efficiency of L1 for a
    single Tight muon
  • For instance, compare the number of events with a
    reconstructed Tight muon that pass the MU-EM
    trigger with the number of those that pass the
    1-EM trigger
  • With any kind of luck there will be a L3
    component to this with an efficiency close to 1.0
  • For Zs, Trigger is a little more complicated
    because it involves Tight and Loose muons
  • Loose allowed us to miss an A or BC
    scintillator hit
  • so its not quite Trigger2

8
Efficiency Calculation
  • Track is probability to reconstruct and match
    the gtrk
  • Has anybody tried this?
  • Isolation is the probability for a muon from W
    or Z to be isolated.
  • Monte Carlo doesnt yet model delta-phi very well
    so we have to get this from the data.
  • For instance, select events with two isolated
    high pT central tracks, two tight muons, and at
    least one isolated one isolated muon. Look at
    other muon.
  • Definition of Isolation

9
W/Z Group MC Requests
  • Muon-Relevant Samples
  • 50,000 W-gt mn
  • 20,000 Z/g-gt mm
  • 10,000 W-gt tn (all channels)
  • 10,000 Z/g-gt tt (all channels)
  • Characteristics
  • Pythia Generated
  • Geant Version
  • Plate-Level Simulation
  • Most Recent D0Gstar Geometry (including CF Bottom
    B-layer PDT rotation fix)
  • Zero extra interactions
  • Recod with p10.13 or later

10
W Backgrounds
  • Combinatoric Cosmic
  • Small if CFT is used? Prove it. Hint Use
    Cosmic Ray Runs.
  • W-gttnX-gtmnnnX
  • Get this from the MC with a similar calculation
    used to measure the efficiency.
  • Muons from heavy quark decay
  • Determine this from the data.

The background Jets are away or too low ET
11
W-gtmn Bkgd. Setup
12
W-gtmn Backgrounds
  • With events that pass same trigger, muon ID
    criteria, etc
  • 3 Samples (Using 1/2 detector as Tagged-Side)

Keeping track of sides, you can get 2X more stats
than this.
13
Z Backgrounds
  • Combinatoric Cosmic
  • Small if CFT is used? Prove it. Hint Use
    Cosmic Ray Runs.
  • Z-gtttX-gtmmnnnnX
  • Get this from the MC with a similar calculation
    used to measure the efficiency.
  • Muons from heavy quark decay
  • Determine this from the data as with the Ws.

14
Summary
  • Goals for spring conferences
  • Z-gt mm (ee) Mass Cross Sections
  • W-gt mn (en) Transverse Mass and Cross Sections
  • W-gt mg (eg) Event Displays
  • My take on these goals
  • Show that the new muon detectors and trigger will
    do their jobs
  • Its Most important that we demonstrate the
    capabilities of the new central tracker.
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