InGaAs and GaInNAsSb Advanced LIGO Photodiodes - PowerPoint PPT Presentation

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InGaAs and GaInNAsSb Advanced LIGO Photodiodes

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David B. Jackrel, Homan B. Yuen, Seth R. Bank, Mark A. Wistey, ... Sb surfactant effects improve thin strained nitride films. STANFORD. 7 / 18. Conventional PD ... – PowerPoint PPT presentation

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Title: InGaAs and GaInNAsSb Advanced LIGO Photodiodes


1
InGaAs and GaInNAs(Sb)Advanced LIGO Photodiodes
  • 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 LHO
  • August 16th, 2005

LIGO-G050435-00-Z
2
Outline
  • Introduction
  • AdLIGO Photodiode Specifications
  • Device Materials
  • Device Design
  • GaIn(N)As(Sb) Materials Device Results
  • Conclusion

3
Advanced LIGO Schematic
High-Speed Low Power ? Commercial Device
180 W
Low Noise Iph 200 mA Commercial Device?
4
LIGO AS-Photodiode Specifications
5
1 eV Materials InGaAs GaInNAs
GaInNAs(Sb) 25 InGaAs
1064nm light ? 1.13eV
º
Ge
6
Metamorphic-InGaAs vs. GaInNAsDouble
Heterostructres
7
Back-Illuminated Photodiodes
Adv. LIGO Back-Illuminated PD
  • High Power
  • Linear Response
  • High Speed

Conventional PD
8
Outline
  • Introduction
  • GaIn(N)As(Sb) Materials and Device Results
  • Materials Characterization Summary
  • Dark Current
  • Bandwidth
  • Quantum Efficiency
  • Saturation Power Level
  • Conclusion Future Work

9
Materials Characterization Summary
Deep-Level Transient Spectroscopy (DLTS)
XRD-Reciprocal Space Map (224)
Absorption Spectra
Photoluminescence (PL) Spectra
10
Dark Current DensityGaIn(N)As(Sb) Devices
- Jdk (A/cm2)
11
MM-InGaAs 3dB Bandwidth
BW 1/RC BW gt 200 MHz ? 400 ?m Psat 10 mW
AdLIGO PD Specifications 3-dB Bandwidth
Sat. Power DC-Scheme 100 kHz
30 100 mW RF-Scheme 200 MHz
AdLIGO RF-Readout Challenging for PDs!
12
InGaAs GaInNAs PDs IQE(w/ FCA Incomplete
Absorption)
AdLIGO Requirement
Int.
13
GaIn(N)As(Sb) PD QE
InGaAs
GaInNAs
GaInNAsSb
Int.
( scaled to account for FCA in thick substrates)
14
Photodiode Saturation Power
LIGO GW-PD Requirement
InGaAs
GaInNAs
GaInNAsSb
Bias V 3 8 V
( scaled to account for FCA in thick substrates)
15
Photodiode Results Summary
16
Conclusion
17
AdLIGO Photodiode Development Future Work
  • Substrate removal
  • ? 90 QE
  • High-Temperature Packaging
  • LLO or LHO Damage Threshold Tests?
  • Compatible with other experiments (GEO-600, MIT?)
  • Surface Uniformity Noise Characterization
  • GEO-600
  • Multi-Element Sensors?
  • Additional pointing information
  • Spatial mode information
  • Fabricate AdLIGO Photodiodes

18
Acknowledgements
  • National Science Foundation (NSF) this material
    is based on work supported by the NSF under
    grants 9900793 and 0140297.
  • Aaron Ptak, Manuel Romero and Wyatt Metzger at
    National Renewable Energy Labortatory (NREL) in
    Golden, CO
  • Gyles Webster at Accent Optical in San Jose, CA
  • Thank You

19
Extra slides
20
Molecular Beam Epitaxy (MBE)
  • Effusion cells for In, Ga and Al
  • Cracking cell for As and Sb
  • RF-Plasma N cell

Deflection Plates (DP) on Plasma Source ? protect
growth surface from ion damage
21
Double-HeterostructurePIN Photodiodes
2
eV
p-
light
1
i-
0
n-
-1
-2
0 1
2 3 ?m
N- and P- transparent ? Absorption occurs in
I-region where E-field is large
InGaAs DH-PIN device simulated by ATLAS (Silvaco)
22
Lattice-Mismatched Epitaxy
h lt hc
afilm
afilm gt asubstrate
hc ? critical thickness
h gt hc
asubstrate
23
Materials Results Summary
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