stanford advanced ligo high-power photodiodes david jackrel, phd candidate dept. of materials...

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STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference, LLO March 17 th -21 st , 2003 IGO-G030069-00-Z

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STANFORD Photodiode Specifications ParameterLIGO IAdvanced LIGO Steady-State Power 0.6 W~1 W Operating Frequency  29 MHz 100 kHz ~ 180 MHz Quantum Efficiency  80%  90% Detector Design Bank of 6(+) PDs 1 PD

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Page 1: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Advanced LIGO High-Power Photodiodes

David Jackrel, PhD CandidateDept. of Materials Science and Engineering

Advisor: James S. Harris

LSC Conference, LLOMarch 17th-21st, 2003

LIGO-G030069-00-Z

Page 2: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Outline

Introduction High-Power Results High Efficiency Process Predictions

Page 3: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Photodiode Specifications

Parameter LIGO I Advanced LIGO

Steady-State Power 0.6 W ~1 WOperating Frequency 29 MHz 100 kHz

~ 180 MHzQuantum Efficiency 80% 90%Detector Design

Bank of 6(+) PDs 1 PD

Page 4: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

GaInNAs vs. InGaAs

GaInNAs

25% InGaAs

53% InGaAs

1064nm light 1.13eV

Page 5: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

InGaAs vs. GaInNAs PD Designs

2 m

GaInNAs lattice-matched to

GaAs!

Page 6: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Heterojunction Band Gap Diagram

N-layer:In.22Al.78As

or GaAs Eg2=2.0-

1.4eV

P-layer:In.22Al.78As

or GaAs Eg2=2.0-

1.4eV

I-layer:In.22Ga.78As, or Ga.88In.12N.01As.99

Eg1=1.1eV

n-

i-

p-

InAlAs and GaAs transparent at 1.064m

Absorption occurs in I-region (in E-field )

Page 7: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Rear-Illuminated PD Advantages

Conventional PD Adv. LIGO Rear-Illuminated PD

High Power Linear

Response High Speed

Page 8: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

DC Device Response

Page 9: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

DC Device EfficiencyEx

t. E

ffic

ienc

y

Optical Power (mW)

Bias (Volts)

Page 10: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

High Efficiency Detector Process (1)1. Deposit and Pattern P-

Contact2. Etch Mesa –

H2SO4:H2O2:H20 and Passivate in (NH4)2S+

3. Encapsulate Exposed Junction

4. Flip-Chip Bond

- N+ GaAs Substrate

- Epitaxial Layers

- Au Contacts

- Polyimide Insulator

- SiNx AR Coating

- AlN Ceramic

Page 11: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

High Efficiency Detector Process (2)

6. Deposit AR Coating & N-Contact

7. Saw, Package and Wire-Bond

- N+ GaAs Substrate

- Epitaxial Layers

- Au Contacts

- Polyimide Insulator

- SiNx AR Coating

- AlN Ceramic

5. Thin N+ GaAs Substrate

Page 12: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Surface Passivation Results

Page 13: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Predictions

Diameters 3mm 4.5mm 150um

Saturation Power    

Devices Old New New

300mW ~1W ~2mW

       

Bandwidth    

Devices Old New New

3MHz ~1MHz ~1GHz

Page 14: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Conclusion

High-Power Results 300mW (@ 3MHz B.W.) 60% External Efficiency

High-Efficiency Process < -30 Volts realized (on un-mounted

devices) Working out processing

Predictions (by Next LSC…) 1 Watt (@ 1MHz B.W.) 90% External Efficiency

Page 15: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

MBE Crystal Growth

Effusion cells for In, Ga, Al

Cracking cell for As Abrupt interfaces Chamber is under

UHV conditions to avoid incorporating contaminants

RHEED can be used to analyze crystal growth in situ due to UHV environment

T=450-600C

N Plasma Source

Atomic source of nitrogen needed Plasma Source!

Page 16: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

P-I-N Device Characteristics

Large E-field in I- region

Depletion Width Width of I- region

RC time constant

Absorbs a specific

1

IW

IsJ

Js

WAKCCR

/0

Page 17: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Full Structure Simulated by ATLAS

Page 18: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

DC Device Efficiency

Page 19: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Free-Carrier Absorption

(1-T-R) and (1-T-R)/(1-R)

-0.2

0

0.2

0.4

0.6

0.8

1

1.2

850 950 1050 1150 1250 1350 1450 1550 1650 1750

Wavelength (nm)

Abs

orpt

ion

(nor

m.)

GaAs N+GaAs S-IGaAs N+ (W)GaAs S-I (W)

32.9%

N+

S-I

Page 20: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

Surface Passivation Results (2)

Page 21: STANFORD Advanced LIGO High-Power Photodiodes David Jackrel, PhD Candidate Dept. of Materials Science and Engineering Advisor: James S. Harris LSC Conference,

STANFORD

(NH4)2S+ Surface States

(Green and Spicer, 1993)

GaAs(111)A GaAs(111)B