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STAR TPC Luminosity Limitations

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STAR TPC Luminosity Limitations. Bar Harbor June 2002 Howard Wieman. Outline. Efficiency dependence on luminosity (hit density) Momentum dependence on luminosity (hit density) Space charge distortions Normal collisions (luminosity dependent) Beam gas showers (beam current dependent) - PowerPoint PPT Presentation
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STAR TPC Luminosity Limitations Bar Harbor June 2002 Howard Wieman
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Page 1: STAR TPC Luminosity Limitations

STAR TPC Luminosity Limitations

Bar Harbor

June 2002

Howard Wieman

Page 2: STAR TPC Luminosity Limitations

Outline

• Efficiency dependence on luminosity (hit density)

• Momentum dependence on luminosity (hit density)

• Space charge distortions– Normal collisions (luminosity dependent)– Beam gas showers (beam current dependent)

• Conclusions

Page 3: STAR TPC Luminosity Limitations

Method for efficiency estimate as a function of luminosity, i.e. pileup

0 200 400 6000

50

100

effi

cien

cy (

%)

dN

d

Use Bum Choi’s embedding analysis of efficiency for the high Pt paper.

This gives efficiency as a function of track multiplicity.

Estimate pileup track multiplicity as a function of luminosity.

Multiplicities are expressed as dN/d

Page 4: STAR TPC Luminosity Limitations

Tracking efficiency in central events as a function of luminosity

• Mean dN/ = 164 from high Pt paper

• Time for pileup: 2 x drift, 70 s

• Linear extrapolation0 5 1027 1 1028

0

50

100

effi

cien

cy (

%) 2 1026 80 1026

Luminosity 1

cm2

s

Result: 41% at upgrade luminosity

13% events have < 70 pileup tracks

Page 5: STAR TPC Luminosity Limitations

Method for Pt resolution estimate as a function of luminosity – effects do to pileup

Use Bum Choi’s embedding analysis of Pt resolution for the high Pt paper.

This gives Pt resolution as a function of track multiplicity.

Use track pile up multiplicity expected for different luminosities

Multiplicities are expressed as dN/d

0 200 400 6000

0.01

0.02

dN

d

Pt

Pt0.013 Pt b

b

Page 6: STAR TPC Luminosity Limitations

Pt resolution in central events as a function of luminosity

• Mean dN/ = 164 from high Pt paper

• Time for pileup: 2 x drift, 70 s

• Linear extrapolation

Result: Pt/Pt = 7.4% at upgrade luminosity, up from 6.1%

Pt/Pt at Pt = 3 GeV

0 2 1027 4 1027 6 1027 8 10270

10

20

Pt r

esol

utio

n (%

)

2 1026

Luminosity 1

cm2

s

Page 7: STAR TPC Luminosity Limitations

Space charge distortion – what to expect

VE

VEXB

VE

VEXB

+

DCA

B out ofplaner distortion from

radial E field component and EXB

Page 8: STAR TPC Luminosity Limitations

Space charge from normal collisions

Positive Ion Density

Q

r (cm) 50 200

z (cm)210

0

+ ion charge density

peak: 3000 +e/cm3

ionization density rate

50 100 150 200

ionization density rate as a function of r

r (cm)

5000 ions/cm3 s

HIJET

1/r2

•Design luminosity: 2 x 1026 1/cm2 s

•Mean dN/d = 400

•dN/d = constant gives uniform ionization in z

•dN/d = constant gives ionization 1/r2

•Ionization density for dN/d = 400 event at inner radius: ~ 4 ion-e pairs/cm3

Page 9: STAR TPC Luminosity Limitations

space charge error potential

Up

volt

Space charge error potential in the TPC gas volume

Central Membrane

z (cm)

r (c

m)

2 volts

Space charge from normal collisions at design luminosity

Solution for designated charge distribution in a conductive 0 volt box with the STAR field cage geometry

Page 10: STAR TPC Luminosity Limitations

Calculated distortion from normal collisions (beam axis view)

• Mean dN/d = 400• Design Luminosity –

2 x 1026 (1/cm2 s)• Full drift length• DCA = 700 m• Dunlop DCA = 3 mm

Calculated distortion at design L

0.1 0.05 0 0.050

50

100

150

200

0

Space charge distorted track

Undistorted track Pt =

Circle fit

r (cm)

x (cm)

Apparent DCA700 m

Page 11: STAR TPC Luminosity Limitations

Calculated distortion at 40 x design L

3 2 1 0 10

50

100

150

200

0

Calculated distortion from normal collisions (beam axis view)

• Average dN/d = 400• 40 x Design

Luminosity – 80 x 1026 (1/cm2 s)

• Full drift length• DCA = 2.7 cm

Space charge distorted track

Undistorted track

Circle fit

r (cm)

x (cm)

Apparent DCA

Page 12: STAR TPC Luminosity Limitations

r distortion as a function r and z

• 3 methods of calculation– 1/r2 charge distribution, no

end cap coax geometry

– HIJET r dependence, coax

– Full 2D solution

• Note z dependence shows advantage of TPC with shorter drift distance

50 100 150 200800

600

400

200

0

200

400

z (cm)

r-phi

dist

ortio

n (m

icro

ns)

r = 50, 60, 75, 100, 195 cm

r = 50 cm

r = 195 cm

210 z (cm) 0

Page 13: STAR TPC Luminosity Limitations

Space charge summary

L DCA measured (beam gas)

DCA expected (beam gas)

DCA calculated (normal collisions)

Year 1 ~0.5x1026 3 mm 0.2 mm

Design 2x1026 3 mm 0.7 mm

Upgrade 80x1026 3 mm 27 mm

Page 14: STAR TPC Luminosity Limitations

Conclusion

• Pt resolution loss is not significant• Tracking efficiency drop to 40% is a problem, but

this is a trade off with efficiency. Efficiency can be increased at the expense of Pt resolution

• Space charge distortion with a DCA = 2.7 cm is a real problem that requires a 100 to 1 correction to reach TPC design specification – but, not as much to be equal to what we have today

• Additional issues to be resolved: wire chamber aging


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