Bulletin of the American Physical Society
2018 Annual Fall Meeting of the APS Ohio-Region Section
Volume 63, Number 15
Friday–Saturday, September 28–29, 2018; University of Toledo, Toledo, Ohio
Session A03: Optics and Biophysics
1:30 PM–3:00 PM,
Friday, September 28, 2018
SU
Room: 2591
Chair: Dhurba Raj Sapkota, The University of Toledo
Abstract ID: BAPS.2018.OSF.A03.4
Abstract: A03.00004 : Real Time Spectroscopic Ellipsometry Analysis of the Structural Evolution and Optical Properties of CuInSe2*
2:15 PM–2:30 PM
Presenter:
Dhurba Raj Sapkota
(University of Toledo)
Authors:
Dhurba Raj Sapkota
(University of Toledo)
Prakash Koirala
(University of Toledo)
Puja Pradhan
(University of Toledo)
Robert W. Collins
(University of Toledo)
Thin films of the narrow bandgap solar cell material copper indium diselenide (CuInSe2) have been deposited in one-stage and two-stage thermal co-evaporation processes on c-Si wafer substrates held at temperatures of 300-570 °C. The goal of this study is to apply real time spectroscopic ellipsometry (SE) to analyze the structural evolution and the complex dielectric functions (ε1, ε2) of the CuInSe2 films at the elevated temperatures of deposition. Real time SE provides the structural parameters including the surface roughness and underlying bulk layer thicknesses as functions of time with monolayer level sensitivity during thin film nucleation and coalescence. SE measurements performed in situ during cooling of the deposited film yield (ε1, ε2) at different temperatures. The (ε1, ε2) spectra measured at the deposition temperature and upon cooling provide the room temperature band gap of the CuInSe2 and its temperature coefficient. In two step processes, either In2Se3 or Cu2Se films are deposited first and converted to CuInSe2 upon exposure to either Cu+Se or In+Se evaporant, respectively. Real time SE has been applied to compare the structural evolution that characterizes these two routes for CuInSe2 fabrication.
*Supported by NSF Grant EECS-1665172
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.OSF.A03.4
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