Investigation of transport properties of ZnO/PbS heterojunction solar cells Y. Cheng, M. C. D. Whitaker, R. Makkia, S. Cocklin, V. R. Whiteside, L. A. Bumm, and I. R. Sellers, E. Adcock-Smith, K. P. Roberts, P. Harikumar Yang Cheng 4/21/2016 Homer L. Dodge Department of Physics & Astronomy, University of Oklahoma, 440 W Brooks Street, Norman, OK 73019 Department of Chemistry and Biochemistry, University of Tulsa, 800 South Tucker Drive Tulsa, OK 74104 Department of Physics and Engineering Physics, University of Tulsa, 600 S. College Ave. Tulsa, OK 74104 Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Introduction • CQDs could potentially offer efficient solar cells using low cost, solution based techniques. • Confinement effects existed in CQDs lead to discrete energy levels which could widen the band gap, allowing the optical and electrical properties to be finely tuned by varying the QD size. • Through Multi-exciton generation (MEG) [1] [2] process and multijunction structure [3] CQDs solar cell has the potential to go beyond Shockley-Queisser limit. • To further increase the efficiencies, it will be beneficial to investigate transport properties. 1. Sambur, et al. Science 330.6000 (2010): 63‐66. 2. Semonin, et al. Science 334.6062 (2011): 1530‐1533. 3. Choi, Joshua J., et al. Advanced Materials 23.28 (2011): 3144‐3148. Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Photo-generated carriers extraction • Device structure Glass/ITO/ZnO/PbS/Au EQE (%) Glass EQE (%) ITO ZnO NP’s 100 10-1 10 10-2 Absorbance of PbS solution PbS QD’s 1 400 Au 500 600 700 800 900 1000 Absorbance (arb.u) 100 10-3 1100 Wavelength (nm) Absorbance and EQE measurements clearly show photo-generated carriers from PbS QDs. , Au ITO ZnO PbS Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Surface states and Interfaces • CQDs • ITO/ZnO , • ZnO/CQDs • CQD/contact Au ITO ZnO PbS Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html 0 -5 Current Density (mA/cm2) Current Density (mA/cm2) Device performance 0.00 -0.01 -0.02 -0.03 -0.04 -0.05 -0.4 -0.2 0.0 Voltage( V) -10 -0.4 -0.2 0.0 0.2 0.4 Voltage( V) Leakage current, shunt paths which also result in low fill factor Low Jsc: Series Resistance Shunt path Cross over: Other barriers create another diode in series shifts the voltag Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Trade offs • Thicker PbS layer will increase the total absorption of photons, but the extraction of the photo-generated carriers is limited by the diffusion length. • Doping the ZnO will change the band alignment of ZnO/PbS, which in return influence the electron transport , from the CQD layer to ZnO. • High doping concentration of ZnO will increase depletion width in CQD layer. However, doping will also introduce defects into ZnO layer which decreases the diffusion length Au ITO ZnO PbS Mott Schottky and Impedance Analysis Mott‐Schottky Analysis Impedance Spectroscopy https://en.wikipedia.org/wiki/Electrical_impedance http://www.stallinga.org/ElectricalCharacterization/2terminal/index.html Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Mott Schottky and Impedance Analysis Capacitance (F/cm2) 0.16 80Hz 100Hz 250Hz 500Hz 1000Hz 0.15 Bulk Capacitance 0.14 Depletion Capacitance 0.13 0.12 0.11 -0.4 -0.2 0.0 0.2 0.4 Voltage (V) • Both Depletion capacitance and bulk capacitance are observed in the C-V plot. • However, increasing the sweeping frequency will lead to the reduction of the capacitance. Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Mott Schottky and Impedance Analysis 1/C2 (1/(F/cm2)) 80 70 80Hz 100Hz 250Hz 500Hz 1000Hz 60 50 • 40 30 -0.4 -0.2 0.0 0.2 0.4 80 Hz 0.896 V 100 Hz 0.856 V 250 Hz 0.866 V 500 Hz 0.993 V 1000 Hz 1.164 V The built in voltage extracted from plot of the1/C different frequencies Voltage (V) The built in voltage is way too large than expected based on the reported Fermi level difference [1]. This could be existence of other capacitance from the interfaces or traps which shifts the depletion capacitance. 1. Pattantyus‐Abraham, Andras G., et al. ACS nano 4.6 (2010): 3374‐3380 Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Mott Schottky and Impedance Analysis Current Density (mA/cm2) Forward Bias 0.5 , PbS Au 0.0 -0.6 -0.4 -0.2 0.0 0.2 0.4 0.6 Reverse Bias Voltage( V) , PbS Kramer, I. J., & Sargent, E. H. Chemical reviews, 114(1), 863‐882. Au Mott Schottky and Impedance Analysis 8.0x104 Z''( /cm2) 6.0x104 0V_Bias 4.0x104 -0.5V_Bias 2.0x104 0.25V_Bias 0.0 0.0 3.0x104 6.0x104 9.0x104 1.2x105 Z'(/cm2) Increasing the forward Bias will shrink the Nyquist cole-cole plot. However, when reverse bias the sample with higher voltage will also reduce the impedance at lower frequency. Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Mott Schottky and Impedance Analysis ‐0.5V 0V 0.25V 0.5V Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Mott Schottky and Impedance Analysis C2 C1 R2 R1 Rs Diode2 Diode1 Rs C1 R1 C2 R2 ‐0.5V 362.13 9.2972 70619 67.924 367.47 0V 850.17 10.675 121220 90.005 534.18 0.25V 333.37 12.137 25657 89.671 299.29 0.5V 376.98 12.805 7176.9 63.26 328.84 Photovoltaics Materials & Device Group, University of Oklahoma: http://www.nhn.ou.edu/~sellers/group/index.html Future goals • Extract more information (eg. Carrier lifetime) from the fitting to investigate the transport mechanism. • Impedance spectroscopy under illumination will also be studied to probe the nature of the second diode behavior. • Influence of different optimization methods on the C-V and impedance will be investigated comprehensively. Acknowledgement This work is supported by NASA Oklahoma EPSCoR grant: NNX15AM75A and NNX13AN01A