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Optical and Current Noise of GaN-based Light Emitting Diodes
Shayla M.L. Sawyer, S. L. Rumyantsev, N. Pala, M. S. Shur, Yu. Bilenko, J. P. Zhang, X. Hu, A. Lunev, J. Deng, and R. Gaska 10/12/2018
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Agenda Introduction and Motivation LED characteristics
Experimental Setup Experimental Results Optical Noise Current Noise Conclusions 10/12/2018
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Research Map: A Road Less Traveled
New research area Noise of Light Emitting Devices Previously studied Low Frequency Noise Shot Noise Noise, Current Flow, and Light Emitting Mechanisms Light Intensity Fluctuations Current Noise Degradation and Reliability LEDs Laser Diode 10/12/2018
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Motivation: Applications of UV sources
vs. UV UV? Food and Water Sterilization Company: SteriPen currently using Mercury lamps Working with Nichia to replace with LEDs High density optical storage Company: Pioneer 500GB disk Non-line-of-Sight Short Range Communication Research: DARPA/University research Atmospheric scattering in solar blind region for communication Shaw, G. A., et al., Unattended Ground Sensor Technologies and Applications VII, Proc. Of SPIE 5796, 214, (2005). 10/12/2018
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Motivation: Emphasis for LFN
Low noise light sources for biological hazard detection systems Signal-to-noise ratio False negative rate False positive rate Biological experiments to study small and slow variations of transmitted or reflected light Anthrax Spores Letter containing anthrax B.M. Salzberg, P.V. Kosterin, M. Muschol, S.L. Rumyantsev, Yu. Bilenko, and M.S. Shur, Journal of Neuroscience Methods, 141, pp , 2005. From: and 10/12/2018
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Light Sources Investigated
Compared: 1st and 2nd Generation SET UVTOP® 265nm-340nm Nichia 375 nm and 505nm Roithner Lasertechnik 740 nm Halogen Lamp Pd/Ag/Au SLs AlN C-sapphire Superlattice buffer layer n+-AlGaN n-AlGaN AlInGaN MQW p-AlGaN p+-AlInGaN sapphire 2nd Generation MEMOCVDTM grown strain management layer, AlN buffer layer, and MQW Improved surface morphology and defect density for high Al molar fraction layers Schematic of Deep UV LED Structure SET UVTOP® J. Zhang, X. Hu, A. Lunev, J. Deng, Yu. Bilenko, T. M. Katona, M. S Shur, R. Gaska, Submitted to Jap. J. Appl. Phys 10/12/2018
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LED Performance: SET UVTOP®
*World Record* Deep UV LED Output Power Exceeds 2mW Wall plug efficiency>1% 280 nm 1st Gen. J. Zhang, X. Hu, A. Lunev, J. Deng, Yu. Bilenko, T. M. Katona, M. S Shur, R. Gaska, Submitted to Jap. J. Appl. Phys 10/12/2018
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Experimental Setup Optical noise Current noise
UV enhanced Si photodiode UV-100L from UDT Sensors, Inc . Photodiode load resistor, Rphd = 10 k LED load resistor, RLED = 1k Current noise LED load resistor varied from 100 to 10 k Low noise amplifier Signal recovery Model 5184 Network analyzer 10/12/2018
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Experimental Results: Optical 1/f Noise
At low frequencies the noise LEDs is lower than that of Halogen Lamps (traditional light source) 10/12/2018
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Experimental Results: Optical Noise
Dependence of relative noise spectra on LED current, ILED S. L. Rumyantsev, S. Sawyer, N. Pala, M. S. Shur, Yu. Bilenko, J. P. Zhang, X. Hu, A. Lunev, J. Deng, and R. Gaska, Low frequency noise of GaN-based UV LEDs, JOURNAL OF APPLIED PHYSICS 97, (2005) 10/12/2018
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Experimental Results: Optical Noise
First optical Figure-of-Merit, β n is the number of chips connected in series (n=1 for all LEDs studied in this paper) τ is the radiative life-time q is the electronic charge f is frequency. Hooge parameter *New* Optoelectronic device Figure-of-Merit Electronic device Figure-of-Merit S. L. Rumyantsev, M.S. Shur, Yu. Bilenko, P.V. Kosterin, and B.M. Salzberg, J. Appl. Phys. 96, 966 (2004). 10/12/2018
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Experimental Results: βvs. Wavelength
β, LED noise quality factor for various wavelengths β is the same order of magnitude for the best of SET devices and Nichia (InGaN) LEDs of longer wavelength. 10/12/2018
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Experimental Results: Current 1/f Noise
I=5x10-3A I I=5x10-7A Noise spectra SI of the second generation SET UVTOP® 280 nm LED At low currents (ILED<10-4A), the noise spectra is the superposition of 1/f and generation recombination (GR) noise For some LEDs GR noise can be seen within the whole current range, allowing us to make some estimates. 10/12/2018
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Experimental Results: Current GR Noise
Noise spectra times frequency SIf for the second generation SET UVTOP® 280 nm LED I=3x10-3A I I=10-6A Two GR levels with different characteristic times and their dependence on current (shown as A and B) 10/12/2018
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Experimental Results: Current Noise
Dependence of noise spectral density, SI , on ILED current First to find non-monotonic dependence of noise on current in LEDs and other pn junctions At high current, the noise of the second generation LEDs is always smaller than that of the first generation devices due to reduced series resistance (base and contact noise) First to observe noise decrease with an increase in current 10/12/2018
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Theory: Noise Model Proposed Mechanism
Trap level near one of the bands Carrier concentration fluctuates Bimolecular High injection Concentration fluctuations Spectral noise density of current fluctuations Monomolecular Recombination (Low current) Monomolecular Low injection Low injection Higher injection Monomolecular Higher injection Bimolecular Recombination (High current) High injection 10/12/2018
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Correlation between I-Vs and Noise
Maximum corresponds to the light emission threshold 10/12/2018
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Estimates Et<0.19 eV From this equation Nt can be determined
Maximum of noise current dependence corresponds to the level occupancy F=2/3. For ωτcF=1 From this equation Nt can be determined Taking for the estimate the lifetime, , in GaN for the LED with the highest GR noise we obtained Nt=71015 cm-3 If τ is constant like GR process “B” the trap level position can be found τr Nt Et<0.19 eV Et<EF EF=0.19 10/12/2018
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Conclusions Second generation SET UVTOP® LEDs showed reduced current and optical noise The GR noise demonstrated non-monotonic dependence on current, explained by the presence of relatively shallow trap levels in the quantum well The trap level concentration responsible for this GR noise is estimated to be Nt=71015 cm-3 For the shallowest trap level Trap “B” the estimate of the level position yields Et<0.19eV Deep UV LEDs can provide superior S/N ratios for biological hazard detection systems 10/12/2018
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Acknowledgements Advisor: Prof. Michael Shur LFN Group Members at RPI
Department of Homeland Security Fellowship program “This research was performed while on appointment as a U.S. Department of Homeland Security (DHS) Fellow under the DHS Scholarship and Fellowship Program, a program administered by the Oak Ridge Institute for Science and Education (ORISE) for DHS through an interagency agreement with the U.S Department of Energy (DOE). ORISE is managed by Oak Ridge Associated Universities under DOE contract number DE-AC05-00OR All opinions expressed in this paper are the author's and do not necessarily reflect the policies and views of DHS, DOE, or ORISE.” 10/12/2018
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References [1] B.M. Salzberg, P.V. Kosterin, M. Muschol, S.L. Rumyantsev, Yu. Bilenko, and M.S. Shur, “Journal of Neuroscience Methods, 141, pp , (2005). [2] R. DaCosta, H. Andersson, and B. Wilson Photochemistry and Photobiology: 78, 384, (2003). [3] J. Zhang, X. Hu, A. Lunev, J. Deng, Yu. Bilenko, T. M. Katona, M. S Shur, R. Gaska, Submitted to Jap. J. Appl. Phys [4] Yu. Bilenko, A. Lunev, X. Hu, J. Deng, T. M. Katona, J. Zhang, R. Gaska, M. S Shur, W. Sun, V.Adivarahan, M.Shatalov, and A. Khan, 10 milliwatt pulse operation of 265nm AlGaN light emitting diodes, Jap. J. Appl. Phys., v.44, pp. L98-L100 (2005). [5] J. Zhang, X. Hu, Yu. Bilenko, J. Deng, A. Lunev, M. S Shur, and R. Gaska, AlGaN-based 280nm light-emitting diodes with continuous-wave power exceeding 1mW at 25mA, Appl. Phys. Lett., v.85, pp (2004). [6] Chen, C. et al. Jpn. J. Appl. Phys. 41, 1924 (2002). [7] S. L. Rumyantsev, S. Sawyer, N. Pala, M. S. Shur, Yu. Bilenko, J. P. Zhang, X. Hu, A. Lunev, J. Deng, and R. Gaska, Low frequency noise of GaN-based UV LEDs, JOURNAL OF APPLIED PHYSICS 97, (2005) [8] S. L. Rumyantsev, M.S. Shur, Yu. Bilenko, P.V. Kosterin, and B.M. Salzberg, J. Appl. Phys. 96, 966 (2004). 10/12/2018
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Derivation Slides Nt is the trap concentration, n is the electron concentration in the quantum well, τ is the characteristic time of the GR noise, V is the volume, and F is the occupancy of the level. σ is the capture cross section, v is the thermal velocity Concentration fluctuations Characteristic time 10/12/2018
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Derivation Slides F level of occupancy for non-degenerate case
Nc is the effective density of states in the conduction band and Et is the level position (the energy is measured down from the bottom of the conduction band) We now consider two limiting cases for low frequencies wt<<1: 10/12/2018
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Noise SI increases with the current increase
Derivation Slides Monomolecular recombination occurs at low currents where the current is proportional to electron concentration At low currents, the electron concentration n is small and the trap level is almost empty (F<<1). Then the spectral noise density of current fluctuations SI for ωτ<<1 can be expressed as: Noise SI increases with the current increase 10/12/2018
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Noise SI decreases with the current increase
Derivation Slides Monomolecular recombination at higher currents the occupancy of the trap level also increases. Assuming that (1-F)<<1 and that the recombination is still monomolecular, we obtain Noise SI decreases with the current increase 10/12/2018
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Derivation Slides Bimolecular recombination occurs at high currents where its spectral noise density SI can be expressed as where B is radiative recombination coefficient and is the internal quantum efficiency For the case (1-F)<<1, we obtain that the spectral noise density is independent of the current: 10/12/2018
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