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STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank,...

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STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao, and James S. Harris, Jr. Solid State Research Lab, Stanford University LSC Meeting – LLO March 22 nd , 2005 IGO-G050116-00-Z
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Page 1: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Advanced LIGO Photodiode Development

______

David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao, and

James S. Harris, Jr.

Solid State Research Lab, Stanford University

LSC Meeting – LLO

March 22nd, 2005LIGO-G050116-00-Z

Page 2: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Outline

AdLIGO Photodiode Specifications

Device Results

Damage Threshold

AdLIGO Devices

Future Directions

Page 3: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Advanced LIGO Schematic

Power Stabilization

Auxiliary Length Sensing

Page 4: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Photodiode Specifications

LIGO I Advanced LIGO

Detector

Bank of 6PDs

Power Stabilizati

on

Aux. Length (RF)

Detection

DC - GW Channel

Steady-State

“Power”0.6 W 200 ~ 300

mA 10 – 100 mW 30 mW

Operating

Frequency

~29 MHz 100 kHz 200 MHz 100 kHz

Quantum

Efficiency

80% > 80% 90%

(300mA)/(0.868A/W

* 0.90 QE) = 385mW

Resonating Tank Circuit Trades w/

Sensitivity

Page 5: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Conventional PD Adv. LIGO Rear-Illuminated PD

High Power Linear

Response High Speed

Rear-Illuminated PD Advantages

Page 6: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Materials Analysis –InGaAs/GaAs vs. GaInNAs/GaAs

X-Ray DiffractionX-Ray Diffraction

Transmission Electron MicroscopyTransmission Electron Microscopy

Surface Roughness MappingSurface Roughness Mapping

PhotoluminescencePhotoluminescence

Deep-Level Transient SpectroscopyDeep-Level Transient Spectroscopy

Absorption SpectraAbsorption Spectra

Etc.Etc.

Page 7: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Device Internal Quantum Efficiency (Low Power ~ 50 mW)

Page 8: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

External Quantum Efficiency –Thick Substrate

Ext.

Eff

icie

ncy

Optical Power (mW)

Bias (Volts)

Page 9: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Damage Threshold – LLO Devices (9/23/03)

P > 2e6 W/cm2 (???)(>180 W in 100 m spot)

Page 10: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

LHO Damaged PDs –Shutter Problems (2/22/05)

Damaged Devices

Undamaged Devices “…acoustic coupling…”

-Robert Schofield

Page 11: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

LHO Damaged PDs –Shutter Problems (2/18/05)

No injected Peak at 280 Hz

Page 12: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Rear-IlluminatedDamage-Threshold Test

Page 13: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Front-IlluminatedDamage-Threshold Test

Page 14: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

AdLIGO Devices

DetectorPower

Stabilization

Aux. Length Sensing

GW Channel

Diameter 3 mm 1.5 mm1 mm

(or larger?)

Steady-State Power

300 mW 100 mW 50 mW

3-dB 1/RC Bandwidth

5 MHz30 MHz

( 180 MHz?)60 MHz

Quantum Efficiency

> 80 % 80 ~ 90 %

Damage Threshold

? Important?!

Page 15: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

AdLIGO Devices: Commercial Vendors

http://www.stanford.edu/~djackrel

Page 16: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

In Progress / Future Directions

Substrate removal GaInNAs(Sb) growth (w/ upgraded

system) ARC 1/f noise experiments

Successor - Zhilong Rao Packaging devices / Testing components Higher saturation power? ( RF

detection?) Surface uniformity?, Backscatter?, etc.

Page 17: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Future Directions – What types of diodes are needed?

Quantum Efficiency? Damage Threshold? Saturation Power?

RF detection AdLIGO laser stabilization

Electronic Noise? DC RF? (180 MHz)

Frequency Response? Commercially available?

Other???

Page 18: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

XRD Reciprocal Space Map (004)

MM-InGaAs GaInNAs

Page 19: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Surface Roughness

MM-InGaAs RMS = 6.2 nm

GaInNAs RMS = 0.8 nm

[110][-110]

Page 20: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Optimizing Post-Growth Anneal

Page 21: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Scanning PhotoluminescenceIntensity

InGaAs:Uniformity: 10.8%

GaInNAsUniformity: 15.9%

Page 22: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Scanning PL Intensity Maps

InGaAs GaInNAs

Page 23: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

GaInNAs Temp. Dependent PL: Localization Energy

Page 24: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Sample Activation Energy (eV)

Trap Density (cm-3)

CaptureCross-Section (cm2)

LM - GaInNAs0.63

1.1 x 1014 9.0 x 10-15

0.273.9 x 1013 2.5 x 10-16

0.227.5 x 1013 3.2 x 10-15

0.151.7 x 1013 5.2 x 10-18

MM - InGaAs0.47

2.0 x 1013 4.9 x 10-15

0.123.1 x 1012 3.2 x 10-12

Deep Level Transient SpectroscopyMajority Carrier Traps

Page 25: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

1 m GaInNAs Film Transmission

Page 26: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

2 m InGaAs Absorption Spectrum

Page 27: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

InGaAs vs. GaInNAs Dark I Density

Page 28: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Dark and Photocurrent (SNR)

Page 29: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Photovoltaic Response

Page 30: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

C-V Curves

GaInNAs: 1/RC 7 MHz

InGaAs: 1/RC 15 MHz

Page 31: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

LCR Resonant Circuit Modeling

FWHM 15 MHz

Page 32: STANFORD Advanced LIGO Photodiode Development ______ David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, Xiaojun Yu, Junxian Fu, Zhilong Rao,

STANFORD

Damage Threshold Tests

LIGO 1

power in each arm (W) ITM transmission Total Power on AS-PD Spot Radius (um) Area (cm2) Power Density (W/cm2)

6000 0.03 360 5.00E+01 7.85398E-05 4.58E+06

6000 0.03 180 5.00E+01 7.85398E-05 2.29E+06

20 1.178511302 4.36E-06 4.58E+06

20 1.666666667 8.73E-06 2.29E+06

AdLIGO

power in each arm (W) ITM transmission Total Power on AS-PD Spot Radius (um) Area (cm2) Power Density (W/cm2)

8.30E+05 0.03 4.98E+04 5.00E+01 7.85398E-05 6.34E+08

20 0.100200602 3.15E-08 6.34E+08


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