+ All Categories
Home > Documents > Measurement of Luminosity at energy 2.23 GeV, 2.4 GeV, 2.8...

Measurement of Luminosity at energy 2.23 GeV, 2.4 GeV, 2.8...

Date post: 15-Oct-2018
Category:
Upload: nguyenlien
View: 219 times
Download: 0 times
Share this document with a friend
14
Measurement of Luminosity at energy 2.23 GeV, 2.4 GeV, 2.8 GeV and 3.4 GeV Geng Cong Center for Particle Physics and Technology University of Science and Technology of China September 3, 2012 Geng Cong (CPPT-USTC) Luminosity September 3, 2012 1 / 14
Transcript

Measurement of Luminosityat energy 2.23 GeV, 2.4 GeV, 2.8 GeV and 3.4 GeV

Geng Cong

Center for Particle Physics and TechnologyUniversity of Science and Technology of China

September 3, 2012

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 1 / 14

Outline

Introduction

Measurement with e+e− → e+e−

Measurement with e+e− → γγ

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 2 / 14

Introduction

Luminosity (integrated Luminosity, denoted as L ) is a keyparameter of high energy physics and an important input value ofmany analyses. Precise measurement of Luminosity is desired inany experiments.

In e+e− collider, the precise measurement is always achieved dueto the well-understood QED processes e+e− → (γ)e+e−,e+e− → (γ)γ+γ− and e+e− → (γ)µ+µ−.

For a special physical process, the corresponding events rate isN = L · σ(·ε), where the σ is cross section of the physical processand ε denotes the efficiency. So, conversely, using thewell-understood processes, the Luminosity is determined as:

L =N

σ · ε

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 3 / 14

Measurement with e+e− → e+e−: Event Selections

Tracks

Vr < 1.0cm, |Vz | < 10.0cm

N+ = N− = 1

180− arccos−→P+·−→P−

|P+||P−| < 50

Shower

| cos θ| < 0.8

Eshower > 1.3 GeV for 3.4 GeVEshower > 1.0 GeV for 2.8 GeVEshower > 0.8 GeV for 2.4 GeVEshower > 0.7 GeV for 2.23 GeV

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 4 / 14

Generators and Results

Two generators, Babayaga and Bhwide, are used to generate MC events ofe+e− → e+e−. The check by Bhwide is in progress.

2.23 GeV 2.4 GeV 2.8 GeV 3.4 GeVnumber of events 706237 785791 629424 193949

cross section (nb) 818.3 708.1 521.1 353.9Babayga efficiency (%) 32.8 32.5 32.2 31.7

Luminosity (pb−1) 2.631 3.415 3.751 1.729

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 5 / 14

Comparisons between data (Red) and MC (Black)

(eθcos

­0.8 ­0.6 ­0.4 ­0.2 0 0.2 0.4 0.6 0.80

2000

4000

6000

8000

10000

12000

14000

16000

)+

(eθcos

­0.8 ­0.6 ­0.4 ­0.2 0 0.2 0.4 0.6 0.80

2000

4000

6000

8000

10000

12000

14000

16000

Acollinearity

0 1 2 3 4 5 60

5000

10000

15000

20000

25000

30000

180− arccos−−→Pe+ ·−−→Pe−

|Pe+ ||Pe− |

φ∆

­50 ­40 ­30 ­20 ­10 0 10 20 30 40 50

1

10

210

310

410

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 6 / 14

Momentum and Energy: data (Red) and MC (Black)

) (GeV)­

momentum (e

1 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.80

5000

10000

15000

20000

25000

) (GeV)+

momentum (e

1 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.80

5000

10000

15000

20000

25000

30000

E

1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.90

2000

4000

6000

8000

10000

12000

14000

E

1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.90

2000

4000

6000

8000

10000

12000

14000

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 7 / 14

Check by Bhwide

(eθcos

­0.8 ­0.6 ­0.4 ­0.2 0 0.2 0.4 0.6 0.80

2000

4000

6000

8000

10000

12000

14000

16000

)+

(eθcos

­0.8 ­0.6 ­0.4 ­0.2 0 0.2 0.4 0.6 0.80

2000

4000

6000

8000

10000

12000

14000

16000

Acollinearity

0 1 2 3 4 5 60

5000

10000

15000

20000

25000

30000

φ∆

­50 ­40 ­30 ­20 ­10 0 10 20 30 40 50

1

10

210

310

410

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 8 / 14

Measurement with e+e− → γγ: Event Selections

Shower

| cos θ| < 0.8

Eshower > 1.3 GeV for 3.4 GeVEshower > 1.0 GeV for 2.8 GeVEshower > 0.8 GeV for 2.4 GeVEshower > 0.7 GeV for 2.23 GeV

Nshower = 2

180− arccos−→P1·−→P2

|P1||P2| < 50

−20 < 180− |φ1 − φ2| < 40

Tracks

Vr < 1.0cm, |Vz | < 10.0cm

Ntrack = 0

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 9 / 14

e+e− → e+e− and e+e− → γγ

Without taking into account the number of tracks in MDC.

φ∆

­50 ­40 ­30 ­20 ­10 0 10 20 30 40 500

2000

4000

6000

8000

10000

12000

14000

16000

18000

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 10 / 14

Results

Babayaga is used to generate MC events of e+e− → γγ.

2.23 GeV 2.4 GeV 2.8 GeV 3.4 GeVnumber of events 81222 91036 73041 22694

cross section (nb) 56.07 48.52 35.69 24.24Babayga efficiency (%) 55.0 54.9 54.5 53.8

Luminosity (pb−1) 2.634 3.418 3.755 1.740

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 11 / 14

Comparisons between data (Red) and MC (Black)

θcos

­0.8 ­0.6 ­0.4 ­0.2 0 0.2 0.4 0.6 0.80

200

400

600

800

1000

Acollinearity

0 1 2 3 4 5 60

200

400

600

800

1000

1200

1400

1600

1800

φ∆

­10 ­8 ­6 ­4 ­2 0 2 4 6 8 10

10

210

310

E

1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.90

500

1000

1500

2000

2500

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 12 / 14

Another generator: Radgg

Radgg generate MC events with full geometric coverage. Efficiency is 6.7% andcross section is 210 nb. The calculated luminosity is 1.613 pb−1.

φ∆

­10 ­8 ­6 ­4 ­2 0 2 4 6 8 10

10

210

310

Acollinearity

0 1 2 3 4 5 60

200

400

600

800

1000

1200

1400

1600

1800

θcos

­0.8 ­0.6 ­0.4 ­0.2 0 0.2 0.4 0.6 0.80

200

400

600

800

1000

1200

1400

1600

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 13 / 14

Summary

2.23 GeV 2.4 GeV 2.8 GeV 3.4 GeVLuminosity(e+e− → e+e−) (pb−1) 2.631 3.415 3.751 1.729Luminosity(e+e− → γγ) (pb−1) 2.634 3.418 3.755 1.740difference 0.1% 0.1% 0.1% 0.6%Radgg (pb−1) 2.464 3.202 3.517 1.613online (pb−1) 1.466 2.341 3.099 1.658

Geng Cong (CPPT-USTC) Luminosity September 3, 2012 14 / 14


Recommended