Transcript
Page 1: Particle incident angle study with Mimosa 17

Particle incident angle study with Mimosa 17

C.Dritsa, J.Baudot

Outline• Motivation• Digitiser• Analysis• Summary

11th CBM collaboration meeting GSI Darmstadt

Page 2: Particle incident angle study with Mimosa 17

Motivation

Open charm feasibility studies are of major importance for CBMThe MVD is the key detector for open charm measurements.

Background & Signal Generation

Transport

(GEANT)

Simulate detector’s response

For MVD:gaussian smearing

The actual model using gaussian smearing is not adapted for studying event pile-up and delta electrons.

Can this model be improved ?

The implementation of a more realistic MAPS response ( digitisation model ) will allow us studying the impact of the above points especially on the open charm reconstruction. This work is under progress at IPHC, Strasbourg.

Geometry (thickness, stations’ position)

Page 3: Particle incident angle study with Mimosa 17

Simplistic illustration of the digitisation model

Digitisation model for non depleted detector (MAPS detector):

1. Particle trajectory divided in segments inside the sensitive volume.2. Energy deposited in each segment is translated into charge.3. Charge spread in the sensitive volume within a defined cone.

No Electric Field:

Electrons are diffusing sensitive volume

θ

Advantage of digitiser: possibility to study particles with inclined tracks.Need to adapt the model’s parameters in order to reproduce experimental data.

Page 4: Particle incident angle study with Mimosa 17

Beam Test

•Beam test performed in November 2007 at CERN with a 120 GeV pion beam.

•The chip under test was a MIMOSA 17 :30 μm pitch - 14μm epi

MIMOSA 17

MAPS response to tracks with large incident angle was not studied in detail yet.

Page 5: Particle incident angle study with Mimosa 17

• The two external planes (reference planes) are used for track reconstruction.• The middle plane is the Detector Under Test (DUT): the tracks extrapolated in the DUT are matched with the hit located closest to the reconstructed track position.• Measurements were taken for several angles:• θ: 0°, 15°, 30°, 45°, 60°, 75° and 80°

Analysis steps

Top view of the setup

Reference plane:MIMOSA 17

Reference plane:MIMOSA 17

DUT

θ: 080!

Page 6: Particle incident angle study with Mimosa 17

Charge collected

in each pixel

PitchSize

tN pix

tan

How is the cluster shape affected when track is inclined ?

L

,PitchSizeNU pix

Lt

L: length of the particle trajectory in the epitaxial layert: epitaxial layer thicknessθ: angle of incidence with respect to the vertical

cos

80 tQ tot

tantU

cos

tL ,)/(80 LmeQ tot

Page 7: Particle incident angle study with Mimosa 17

• 7x7 cluster

• Each square represents one pixel

•Color scale normalised

Average Cluster Shape

Q on seed (MPV, e-)

250

249

285

348

506

823

964

Angle (°)

0

15

30

45

60

75

80

0° 15° 30°

45° 60° 75°

80°

Differences in the average cluster shape are obvious for large angles (>60o)

Page 8: Particle incident angle study with Mimosa 17

0° 15° 30°

45° 60° 80°

Page 9: Particle incident angle study with Mimosa 17

Cha

rge

colle

cted

(el

ectr

ons)

Collected charge

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Signal to Noise Ratio on seed

• For small angles (<30o) the SNR is almost constant

• For bigger angles (>60o) the SNR varies significantly

Page 11: Particle incident angle study with Mimosa 17

Residuals

U

Vσ of the distribution of track-hit distance.

Page 12: Particle incident angle study with Mimosa 17

Can the inclination of the track be derived from cluster properties?

The number of significant pixels (above given threshold) is higher for 80° than for 0°.The aspect ratio is different.

Allow to identify and suppress hits from delta electrons?

U

V 0° 80°

Comparison of properties of average clusters for two angles:

Page 13: Particle incident angle study with Mimosa 17

....

...)3()2()1(

3,32,21,1

23,3

22,2

21,1

2

uvuvuv

uvuvuv

QQQ

vQvQvQ

Q

VQWidth defined by :

- 0°- 80°

V cluster width

U c

lust

er

wid

th

V cluster width

Can the inclination of the track be derived from cluster properties?

80°v=

u

Page 14: Particle incident angle study with Mimosa 17

Beam test (pions, 120GeV) on inclined tracks up to 80° was performed.

For small angles (<30o) the SNR of the seed, the charge of the seed and the charge of the full cluster are constant.

For large angles (>60o) the SNR of the seed , the charge of the seed and the charge of the full cluster increase significantly.

The residuals along the V direction (along the rotation axis) remain constant but the residuals along the U direction increase (up to 4 times for 80 degrees, but algorithm not optimised)

It seems possible to identify hits created from tracks with large incident angle. Investigate possible applications of this identification.

Next steps:Implementation of the digitiserPerform simulation study to evaluate the fraction of particles with large incident angle.

Summary and results

MotivationImplement MAPS digitiser.Study MAPS response to inclined tracks.

Page 15: Particle incident angle study with Mimosa 17

1 1

1 1 1 1

1 1 1

Can the inclination of the track using information from the cluster be derived ?

Page 16: Particle incident angle study with Mimosa 17

Q(Vi,Ui) Q(1,1)

Q(0,0)

Q(-1,1)

....

...)1()1()0(

1,11,10,0

21,1

21,1

20,0

2

QQQ

QQQ

Q

VQ

U

V

Page 17: Particle incident angle study with Mimosa 17

1 Digital3 CoG 3x35 CoG 5x57 Eta 4var9 Eta 3x311 Eta 2x213 Eta 5x5

0 degrees 80 degrees

Residuals 7x7 cluster: Different methods

The residuals obtained from eta 3x3 are the best even for 80 degrees rotation

Res

idu

als

(μm

)

Page 18: Particle incident angle study with Mimosa 17

Charge on Seed

250 249 285348

506

823

964

0

200

400

600

800

1000

1200

0 10 20 30 40 50 60 70 80 90

rotation anlge (degrees)

elec

tro

ns

Charge on seedMIMOSA 17 ( 14microns epi )

Page 19: Particle incident angle study with Mimosa 17

Charge 49 pixelsMIMOSA 17 ( 14microns epi )

Charge on 49 pixels

886 895 10051258

1847

3755

5048

0

1000

2000

3000

4000

5000

6000

0 10 20 30 40 50 60 70 80 90

rotation angle

char

ge

on

49

pix

els

(e-)

Page 20: Particle incident angle study with Mimosa 17

Noise on seed

14,8 14,8

14,7

14,8

15

14,9

14,5

14,4

14,5

14,6

14,7

14,8

14,9

15

15,1

0 10 20 30 40 50 60 70 80 90

rotation angle (degrees)

elec

trons

Noise on seedMIMOSA 17 ( 14microns epi )

Page 21: Particle incident angle study with Mimosa 17

Charge on 49 pixels

886 895 10051258

1847

3755

5048

0

1000

2000

3000

4000

5000

6000

0 10 20 30 40 50 60 70 80 90

rotation angle

char

ge

on

49

pix

els

(e-)

cos

80 tQ tot

constQtot cos

if CCE is const and clustering is correct:

Qtot*cos(theta)

750

800

850

900

950

1000

-20 0 20 40 60 80 100

angle (degrees)

Q(4

9pix

els)

*co

s(th

eta)

~10%

Error bars correspond to 1o

error in defining the rotation

angle

With a 10% precision CCE can be approximated as constant wrt the particle incident angle

What about charge collection efficiency at large angles?

Charge on 49 pixels (Qtot)

Page 22: Particle incident angle study with Mimosa 17

0 degrees 80 degrees

Residuals 7x7 cluster

μm μm

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0 15 30

45 60 75

80

Page 24: Particle incident angle study with Mimosa 17

SNR on seed (MPV in e-)

250

249

285

348

506

823

964

Angle (degrees)

0

15

30

45

60

75

80

0 15 30

45 60 75

80

• 7x7 cluster

• Each square represents one pixel

•Color scale normalised

Mean Cluster Form (3D)


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