glast (gamma-ray large area space telescope)

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Heavy ion irradiation on silicon strip sensors for GLAST & Radiation hardening of silicon strip sensors S.Yoshida, K.Yamanaka, T.Ohsugi, H.Masuda T.Mizuno, Y.Fukazawa (Hiroshima Univ.) Y.Iwata, T.Murakami (NIRS) H.Sadrozinski (SCIPP,UCSC) K.Yamamura, K.Yamamoto, K.Sato (HPK)

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Heavy ion irradiation on silicon strip sensors for GLAST & Radiation hardening of silicon strip sensors S.Yoshida , K.Yamanaka, T.Ohsugi, H.Masuda T.Mizuno, Y.Fukazawa (Hiroshima Univ.) Y.Iwata, T.Murakami (NIRS) H.Sadrozinski (SCIPP,UCSC) K.Yamamura, K.Yamamoto, K.Sato (HPK). - PowerPoint PPT Presentation

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Page 1: GLAST (Gamma-ray Large Area Space Telescope)

Heavy ion irradiation onsilicon strip sensors for GLAST

&Radiation hardening of silicon strip sensors

S.Yoshida, K.Yamanaka, T.Ohsugi, H.Masuda T.Mizuno, Y.Fukazawa (Hiroshima Univ.)

Y.Iwata, T.Murakami (NIRS)H.Sadrozinski (SCIPP,UCSC)

K.Yamamura, K.Yamamoto, K.Sato (HPK)

Page 2: GLAST (Gamma-ray Large Area Space Telescope)

GLAST (Gamma-ray Large Area Space Telescope)

e+e-

Array of Silicon Strip Sensor

Detect gamma-raythrough e+e- conversion

will be launched in 2006

Page 3: GLAST (Gamma-ray Large Area Space Telescope)

GLAST prototype sensorsingle-sided,n-bulk, p-stripAC coupling readout448 strips208 m strip pitch

9.5cm

9.5cm

↑quarter

Page 4: GLAST (Gamma-ray Large Area Space Telescope)

The aim of the heavy ion irradiation

(1) Investigate radiation damage due to high dE/dx particles. slowed-down Fe ions (8GeV/g/cm2 = 5000×MIP)

check items : full depletion voltage, leakage current,coupling capacitance, interstrip capacitance

(2)Investigate the differece between Crystal Orientations.<111> and <100>

Al

Al

p+strip

n+

SiO2

Si bulk

The difference comes from the nature of the SiO2/Si interface.

Si3N4

Page 5: GLAST (Gamma-ray Large Area Space Telescope)

Irradiation (HIMAC@NIRS, Japan)

Fe ion500MeV/n

Absorberto slow down

Fe ions

Sensor(in the box)

150V bias

dE/dx=8GeV/g/cm2

Page 6: GLAST (Gamma-ray Large Area Space Telescope)

<111>410m thick

<100>320m thick

Fe ion dose“8 krad” 111, 8 krad 100, 8 krad

Fe ion dose“22 krad” 111, 22krad 100, 22krad

Iradiated Sensors (4 sensors)

Expected dose for 5 years GLAST mission: 1 krad

Page 7: GLAST (Gamma-ray Large Area Space Telescope)

Full Depletion Voltage

111 (410m)

↑depletion voltage: 100 V

100 (320m)

↑depletion voltage: 80 V

Page 8: GLAST (Gamma-ray Large Area Space Telescope)

Leakage Current

111 (410m)

↑full depletion voltage

100 (320m)↑full depletionvoltage

Page 9: GLAST (Gamma-ray Large Area Space Telescope)

Leakage Current (strip)

leakage current is very uniform (before and after)no dead or noisy channel (before and after)

after irradiation

before irradiation

after irradiation

before irradiation

111(8krad) 100(8krad)

Page 10: GLAST (Gamma-ray Large Area Space Telescope)

Leakage Current vs Dose

11122krad

10022krad

1118krad

1008krad

leakage current : thickness×dose generated in bulkno difference between 111 and 10010nA/cm2/krad: typicallyexpected for ionizing damage

Page 11: GLAST (Gamma-ray Large Area Space Telescope)

Coupling Capacitance

111(10krad) 100(10krad)

None of the coupling capacitors were broken. No differences between grounded strips

and floating strips.

Readout strip:grounded

after irradiation

before irradiation

Readout strip:grounded after irradiation

before irradiation

Al stripSiO2

Si bulk

n+

Al

40M

p+ strip

+150 V

Si3N4

Page 12: GLAST (Gamma-ray Large Area Space Telescope)

Inter strip Capacitance

No differences between before and after the irradiation. No differences between grounded strips and floating strips.

111(8krad) 100(8krad)

Readout strip:grounded

Readout strip:groundedafter irradiation

before irradiation

after irradiation

before irradiation

Page 13: GLAST (Gamma-ray Large Area Space Telescope)

Conclusion

Full Depletion Voltage:No significant differences between before and after the irradiation.Leakage Current:The increase after the irradiation is as expected from total dose. The strip current are very uniform before and after the irradiation. Coupling Capacitance:None of strip were broken.Inter Strip Capacitance:No significant difference between before and after the irradiation.

None of the strips has become insensitive.No significant differences between <111> and <100>.No differences between grounded strips and floating strips.

Page 14: GLAST (Gamma-ray Large Area Space Telescope)

Radiation hardening of silicon strip sensors(preliminary results)

We focused on surface radiation damage of silicon strip sensorsWe used leakage current as the probe for study

Microscopic reason of surface damage (increase of leakage current): the generation of radiation induced interface traps

Interface trap formation: Generated holes in SiO2 layer play a important role. Transport of holes to SiO2/Si interface initiate the formation.

To prevent trasport of holes to SiO2/Si interface, we tried two methods Method I : the leakage current after irradiation decreased by 26% Method II: the leakage current after irradiation decreased by 67%

Page 15: GLAST (Gamma-ray Large Area Space Telescope)

Method I To collect the holes generated in SiO2 layer,We applied negative voltage to the readout Al strips

during -ray (60Co) irradiation

+150 V

40Mbias resistor

0 ~ - 60 V

Page 16: GLAST (Gamma-ray Large Area Space Telescope)

0 0 0 0 0(V)

0 –2 0-1 -1(V)

0 –6 0-3 -3(V)

0 –20 0-10 -10

(V)

0 –60 0-30 -30

(V)Strip No.1 Strip No.384

The total of 25 readout Al strips were applied negative voltage. The rest of readout Al strips were floating

Page 17: GLAST (Gamma-ray Large Area Space Telescope)

6% down 25% down

26% down11% down

@150 Vbias voltage

Page 18: GLAST (Gamma-ray Large Area Space Telescope)

+150 V

40Mbias resistor

0 ~ - 60 V

strip leakage cyrrent : 0.1 nA (before irradiation)45nA (during -ray irradiation)

45nA×40M = 1.8 V

(+1.8 V)

Page 19: GLAST (Gamma-ray Large Area Space Telescope)

←23% lower ←57% lower

←65% lower ←20% higher

Page 20: GLAST (Gamma-ray Large Area Space Telescope)

+10 V (full depletion voltage is 60 V)

0 ~ - 60 V

depletionzone

Leakage current isgenerated at theinterface aroundp+ strip

Page 21: GLAST (Gamma-ray Large Area Space Telescope)

Method II The electric field in the SiO2 layer points toward the surfaceThe generated holes in SiO2 layer are transported to the surface.We put conducting sheet on the surface of sensor to collect holes

conducting sheetantistatic mat2 mm thinksurface resistivity (108)

+ 100 V

Page 22: GLAST (Gamma-ray Large Area Space Telescope)

Setup for the -ray irradiation (60Co)

conducting sheet

strip 9 - 219

Page 23: GLAST (Gamma-ray Large Area Space Telescope)

Strip leakage current before and after the irradiation

covered area:strip 9 - 219

8 nA

24 nA

Page 24: GLAST (Gamma-ray Large Area Space Telescope)

Summary

(1) The leakage current after -ray irradiation can be reduced 26 % (Method I) 67 % (Method II)

Method I(2) “-20 V” was the best among 5 trial bias voltage (0, -2, -6, -20, -60 V).(3) In the case of “-20V”, the leakage current at 10 V bias voltage was 65 %

lower than floating strips. interface traps were reduced mainly around the p+ stripfor the sensors having smaller strip pitch, Method I may work effectively.

(4) In the case of “-60V”, the leakage current at 10 V bias voltage was 20%higher than floating strips hole injection from Si bulk due to high electric field?

These results are consistent with the models that :The main reason of surface radiation damage is due to the holes generated in SiO2

and the subsequent transport of the holes to the SiO2/Si interface.

Method IIWe used the antistatic mat as the conducting sheet. (This is just first attempt)It should be thin coating on SiO2 layer. The material, thickness, resistivityis the future subject to study.