Charge Drift in partially-depleted epitaxial GaAs detectors

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Paul Sellin, Radiation Imaging Group Charge Drift in partially-depleted epitaxial GaAs detectors P.J. Sellin, H. El-Abbassi, S. Rath Department of Physics University of Surrey, Guildford, UK J.C. Bourgoin LMDH, Université Pierre et Marie Curie, Paris, France

description

Charge Drift in partially-depleted epitaxial GaAs detectors. P.J. Sellin, H. El-Abbassi, S. Rath Department of Physics University of Surrey, Guildford, UK J.C. Bourgoin LMDH, Université Pierre et Marie Curie, Paris, France. Overview. Chemical reaction growth of thick epitaxial GaAs layers - PowerPoint PPT Presentation

Transcript of Charge Drift in partially-depleted epitaxial GaAs detectors

Page 1: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Charge Drift in partially-depleted epitaxial GaAs detectors

P.J. Sellin, H. El-Abbassi, S. RathDepartment of Physics

University of Surrey, Guildford, UK

J.C. BourgoinLMDH, Université Pierre et Marie Curie, Paris, France

Page 2: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Overview

Chemical reaction growth of thick epitaxial GaAs layers

Depletion thickness and residual impurity concentration

Performance of partially depleted detectors

C-V measurements of impurity concentration at low temperature

Optical probing of charge transport using a focussed laser

Page 3: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Potential challenges for epitaxial GaAs

Strengths of epitaxial GaAs: intermediate photon detection efficiency between Si and

CZT/CdTe metal-semiconductor contacts and device physics are well

understood epitaxial GaAs has low concentrations of native EL2 defect source of highly uniform whole wafer material, compatible with

flip-chip bonding and monolithic electronics

Existing problems: even high purity epitaxial is compensated due to residual

impurities- does not exhibit intrinsic carrier concentrations depletion thickness is severely limited charge carrier lifetimes are reduced

Page 4: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Chemical Reaction growth of thick epitaxial GaAs

Epitaxial GaAs material studied in this work was grown by a Chemical Reaction Method by Jacques Bourgoin (Paris).

• An undoped GaAs wafer is used as the material source, which is decomposed in the presence of high temperature high pressure water vapour to produce volatile species.

•Typically, growth rates of <10 m/hr are used to achieve EL2 concentrations of ~1013 cm-3

L. El Mir, et al, “Compound semiconductor growth by chemical reaction”, Current Topics in Crystal Growth Research 5 (1999) 131-139.

Page 5: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Whole wafer photoluminescence mapping

GaAs material uniformity is characterised using room temperature photo-luminescence mapping - a contact-less, whole wafer technique:

A 25 mW 633 nm HeNe laser is focussed to ~50 m on the wafer

the wafer is mounted on an XY stage, and scanned

PL intensity maps at peak the band edge emission wavelength (870 nm) are acquired

Page 6: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

PL maps of GaAs

Photoluminescence mapping clearly shows the uniformity of epitaxial GaAs compared to semi-insulating VGF material:

H. Samic et al., NIM A 487 (2002) 107-112.

Epitaxial GaAs Bulk GaAs

Page 7: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Calculated depletion thickness

This material is nominally 1-5 x 1014 cm-3- corresponds to a 10-20 m depletion thickness @ 30V, and 15-30 m @ 80V

Width of GaAs Space Charge Region vs Reverse Bias Voltage

Reverse bias voltage (V)

0 50 100 150 200

SC

R w

idth

( m

)

0

50

100

150

200

250

0

50

100

150

200

250

N = 5x1012 cm-3

N = 1x1013 cm-3

N = 5x1013 cm-3

N = 1x1014 cm-3

N = 5x1014 cm-3

Page 8: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

-particle spectra taken with an applied bias of 30V

Channel no.

0 500 1000 1500 2000 2500

Cou

nts

1

10

100

1000

220C-540CV = 30VV = 80V

Alpha particle spectra

5.48 MeV alpha particles are irradiated through the Schottky (cathode) contact - range in GaAs ~20m.

A peltier cooler controlled the device temperature in the range +25°C to -55°C. Shaping time = 0.5 s.

Page 9: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Alpha particle pulse shapes

Alpha particle pulses at room temperature:

preamplifier

shaping amplifier

time base = 1s per division

slow component

fast component

Page 10: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Alpha particle tracks

An un-collimated alpha particle source produces a characteristic ‘double peak’ pulse height spectrum if the depletion thickness is shallower than the particle

range:

Page 11: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

59.5 keV gamma spectra

Depth-dependent CCE produces poorly resolved gamma spectra:

Channel no.

200 400 600 800 1000

log

co

unts

1

10

100

1000

Energy (keV)

0 10 20 30 40 50 60

-15V-30V -50V-70V -90V

T = -50°C

Page 12: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Temperature dependent CV analysis

Allows the doping density ND to be extracted from the gradient of 1/C2 vs V :

dVCdqN

rD )1(

22

0

Voltage(V)

0 5 10 15 20

1/C

2 (F-2

)

0.0

2.0e+20

4.0e+20

6.0e+20

8.0e+20

1.0e+21

1.2e+21

1.4e+21

1.6e+21

220C

100C

-20C

-120C

-210C

-420C

-520C

Page 13: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Depletion Thickness vs Bias Voltage

Page 14: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Impurity Densities

The CV analysis confirm the shallow depletion thicknesses achieved in these devices, and correspond to impurity densities of ~3 x 1013 cm-3 in

sample S16 at low temperature:

Sample Area (mm2) ND (cm-3) Depletionthickness (m)

V = 30V V = 80VT=22C S16 7.1 1.3 x 1014 18 30

S17 3.8 4.3 x 1014 10 16

T=-54C S16 7.1 3.1 x 1013 37 60S17 3.8 2.1 x 1014 14 23

Page 15: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Focussed IR laser scans

Probe the variation in pulse shape as a function of position from the Schottky contact, and

temperature

Page 16: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Scanning optical bench

850nm laser300ns pulse

XY scanning table

cryostat

imaging camera

Page 17: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Laser pulse shapes

T=273K, 20V

At 60m from cathode:

no slow component to signal

At 180m from cathode:

charge drift times are ~350s

IR laser spot appears to have significant beam waist

Page 18: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Laser pulse shapes (2)

T=223K, V=90V

At 60m from cathode:

no slow component to signal

At 180m from cathode:

charge drift times are ~350s

IR laser spot appears to have significant beam waist

Page 19: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

T=273K, V=20V

Position from Schottky (m)

0 50 100 150 200 250

Am

plitu

de

0.0

0.2

0.4

0.6

0.8

1.0

Sig

nal R

iset

ime

(s)

0

100

200

300

400

500

T=223K, V=90V

Position from Schottky (m)

0 20 40 60 80 100 120 140 160 180 200 220

Am

plitu

de

0.0

0.5

1.0

1.5

2.0

2.5

3.0

3.5

Sig

nal R

iset

ime

(s)

0.0

0.5

1.0

1.5

2.0

Pulse risetime and amplitude vs bias

Page 20: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Interaction close to the anode - inside depletion region

Page 21: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Interaction close to n+ substrate - in low field region

Page 22: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Temperature dependent pulse shapes (1)

Laser pulses 60m from Schottky

Time (s)

-100 0 100 200 300 400 500

Am

plitu

de

-3.0

-2.5

-2.0

-1.5

-1.0

-0.5

0.0

273K

223K

248K

248K

198K

223K

V = 60V

V = 20V

Page 23: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Temperature dependent pulse shapes (2)

Laser pulses 180m from Schottky

Time (s)

-100 0 100 200 300 400 500

Am

plitu

de

-1.0

-0.8

-0.6

-0.4

-0.2

0.0

273K

223K

248K

248K198K

223K

V = 60V

V = 20V

Page 24: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Conclusions

The epitaxial GaAs layers studied showed excellent uniformity, and a residual impurity concentration of 1-5 x 1014cm-3

Long electron lifetimes > 300 s were observed in the low field regions - confirms the very low EL2 concentration

Lateral laser scans show: good charge transport in the shallow depleted region long-lived components to the pulse shapes when irradiated close to

n+ substrate - consistent with slow electron diffusion towards the substrate

significant penetration of the depletion region when cooled to -50°C

Future work: further lateral scanning is required with focussed lasers and high

resolution proton microbeams to quantify these phenomena further modest reductions in impurity concentration will produce

significant performance improvements

Page 25: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Acknowledgements

This work was partially funded by the UK’s Engineering and Physics Science Research Council

Page 26: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Alpha particle spectra

Epitaxial GaAs pad detectors were irradiated with an uncollimated 241Am alpha particle source. The detector was mounted in a vacuum cryostat, attached to a peltier cooler to allow operation in the temperature range of +25°C to -55°C. Pulse height spectra (figure 3) were acquired using a conventional charge integrating preamplifier and spectroscopy amplifier (shaping time = 0.5s).

Figure 3: spectra at room temperature, as a function of bias.

S16, -spectra taken at 80V for several temperatures

Channel no.

0 1000 2000 3000

co

unts

1

10

100

1000

10000

Energy deposited (MeV)

0 1 2 3 4 5

-540C

-310C

220C

Page 27: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Interaction in intermediate region

Page 28: Charge Drift in partially-depleted epitaxial GaAs detectors

Paul Sellin, Radiation Imaging Group

Laser pulses 120m from Schottky

Time (s)

-100 0 100 200 300 400 500

Am

plitu

de

-2.5

-2.0

-1.5

-1.0

-0.5

0.0

273K

223K248K

V = 20V

Laser pulses 120m from Schottky

Time (s)

-100 0 100 200 300 400 500

Am

plitu

de

-2.5

-2.0

-1.5

-1.0

-0.5

0.0

273K

223K248K

248K

198K

223K V = 60V

V = 20V

Temperature dependent pulse shapes (2)