Abstract

In order to analyze grain growth on the basis of a kinetic growth model, this study reports on annealing experiments with thin Cu(In, Ga)Se 2 films. The substrate heater in an ultra-high vacuum chamber serves to anneal Cu(In, Ga)Se 2 films of 1 μm thickness for varying times t and temperatures T. An ultra-high resolution scanning electron microscope visualizes the cross-section of the film in order to determine the average grain radius r. The theory of normal grain growth explains the increase of the average grain radius r in dependence on annealing time t and temperature T. For an annealing time t=3 h at T=610°C the average grain size increases by a factor of 2.4. Grains with a (1 1 2)-surface orientation are slightly energetically preferred and grow at the expense of other orientations. Grain growth is thermally activated. The Cu-content of the film determines the activation energy Q for grain boundary motion. Increasing the Cu-content of the film from 17.9% to 25.7% lowers Q from 3.5 to 3.0 eV.For high-efficiency Cu(In, Ga)Se 2 solar cell absorbers with a Cu-content below 22% the temperature T has to exceed at least 550°C in order to obtain sufficient atomic diffusion and therefore significant grain growth.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.