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M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meet ing, March 7, 2003 1 Blessing of Run II Diffractive Results Introduction Data Selection Plots for Blessing
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Page 1: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

1

Blessing of

Run II Diffractive Results

IntroductionData SelectionPlots for

Blessing

Page 2: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

2

Forward Physics

• Hard Single Diffraction• Double Pomeron Exchange• …

Page 3: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Diffractive Dijets

• Compare diffractive events to ND• Measure diffractive structure

function

from RSD/ND vs x bj

Measure pbar momentum loss fraction)from calorimeter information

Page 4: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

4

Momentum Loss Fraction

Diffractive events are boosted towards positive

small

Measure fractional momentum loss of anti-proton

MX 2

s

=yln (1/

e

s

Page 5: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Trigger

• RP is triggered on leading antiprotons• Use RP + jet triggers

require jets

Page 6: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Data Sample

• Use dedicated diffractive triggers

RP+J5 (diffractive sample)

J5 (control sample)

• Data sample ~9 pb-1

(PHYSICS_1_03_v1)

Page 7: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Event Selection

1. Triggered events 352,359

2. MET Significance<6 352,359

3. Two jets (ET>5, |<2.5) 175,292

4. RP coincidence 168,153

5. SD (0.02< <0.1) 15,209

6. All BSC East Gap 1,126

Page 8: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

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8

Question #4

Q : What is the ratio SD/ND for ET > 10 GeV

?

Page 9: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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DSF with Jet ET cut

ET* =

ET1 + ET

2

2

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Q2 Dependence

Page 11: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

11

Answer to Q#4

A : Slope and normalization change by ~ 1% .

Q : What is the ratio SD/ND for ET > 10 GeV

?

Page 12: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Plots For Blessing

Suggested modifications have been implemented

Page 13: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Distribution

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Rapidity

Run I PRL

Diffractive dijets are boosted away from the recoil antiproton

Page 15: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Mean Dijet ET

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jet1-jet2)

Diffractive dijets are more back to back

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M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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MP Multiplicity

Page 18: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Diffractive Structure Function

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Diffractive Structure Function (II)

Page 20: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

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East Multiplicity: BSC vs MP

Page 21: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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DPE Enhanced Sample

• Study a dedicated DPE trigger (RP+J5+GapE)

• ~300 k events

• ET(jet1,2)>5 GeV

• |(jet1,2(,3))|< 2.5

• (0,0) bin ~ 16,000 events (in Run I: 100 evts)

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jet1-jet2)

Page 23: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Dijet Mean Rapidity

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M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Jet Transverse Energy

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M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Conclusions

Relax, it is only physics.

Page 26: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Question # 1

Q : Is the BG peak at ~ 1 due to overlap events from multiple

interactions?

Page 27: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Distribution

Page 28: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Luminosity Dependence

Luminosity: 1.0 E31 1.5 E31 2.3 E31

Page 29: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Overlap Rate

ND (1 - e- n RP) + SD (1 - e- n )

SD e- n

R (ND/SD) =

J5 x RP overlap SD x MB overlap

nRP= ( 1 mb/50 mb) x n , n = 0.3 x L[1 x E31]

ND / SD ~ 600

R (ND/SD) = 12 n e n

SD surviving MB overlap

Page 30: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Multiple Interactions Shift ND Peak

R vs log (1 + n )

Page 31: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Run I vs Run II

Run I Run II

L um / bunch 0.16E30 / 6 20.0E30 / 36

ND / SD 300 (lower jet ET)

600 R (Run I/Run II ) = 1/60

R (Run II) = 10 R (Run I) =

0.15

Page 32: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

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Multiple Interactions

Page 33: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Answer to Q# 1

A : Yes.

1. Ratio is consistent with Run I numbers and Run II expectations.

2. Peak at ~ 1 shifts according to luminosity, as expected.

Q : Is the BG peak at ~ 1 due to overlap events from multiple

interactions?

Page 34: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

34

Question #2

Q : What is the effect of the MP energy scale calibration ?

Page 35: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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MP Calibration

• Use slope from ADC distribution

• Tower-to-tower relative calibration with data/MC

• Energy scale from MC

• MC/MBR

Pile-up at high luminosity

(Slope-Fit)/Fit ~7%for each ring

Time dependence (LED)

Page 36: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

36

MP Multiplicity

Page 37: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

37

MP Contribution to ND

Page 38: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

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Effect of MP Energy Scale

E = +/- 25%

log = +/- 0.1

Page 39: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

39

Answer to Q#2

A : An energy scale variation of +/- 25% yields

log = +/- 0.1.

1. log =0.1 is the bin width of our distribution .

2. Peak position in data is centered where expected, indicating the energy scale uncertainty is < 25% .

Q : What is the effect of the MP energy scale calibration ?

Page 40: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

40

Question #3

Q : What is the background in the RP inclusive rate ?

Page 41: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

41

RP Inclusive Data

Page 42: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

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Zero Crossings

Page 43: M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 20031 Blessing of Run II Diffractive Results Introduction Data Selection.

M. Gallinaro, `` RunII Diffractive Results: Blessing'' - QCD meeting, March 7, 2003

43

Answer to Q#3

Q : What is the background in the RP inclusive rate ?

A : It is 1-2% of all RP triggers, concentrated at log < - 3


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