Abstract
Diffusion of from the window layer into the absorber improves the short circuit current density by narrowing the band gap and increasing the carrier lifetime. Thicker layers, however, show a dramatic loss in photocurrent collection due to over-alloying. Electron microscopy investigations show that this decrease in performance is due to the formation of small grains (∼783 nm average diameter), which exhibit grain boundary porosity in the inter-diffusion region. The larger grain boundary area and void free surfaces give rise to higher levels of nonradiative recombination, and therefore, a lower photocurrent. It is proposed that the small grain size is due to a drag force exerted by segregated solute atoms on a moving grain boundary, while faster diffusion along the grain boundaries results in vacancy build up and porosity due to the Kirkendall effect. The results indicate that the device processing conditions must be carefully controlled such that the negative effects of alloying (i.e., smaller grains, Kirkendall voids) do not undermine its benefits.
5 More- Received 12 January 2024
- Revised 20 March 2024
- Accepted 26 April 2024
DOI:https://doi.org/10.1103/PRXEnergy.3.023002
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.
Published by the American Physical Society
Physics Subject Headings (PhySH)
Popular Summary
Cadmium telluride () solar cells are attractive for their cost-effectiveness and relatively high efficiency. By incorporating a cadmium selenide () window layer, selenium can diffuse into the absorber, enhancing the short circuit current density. In this study, the authors explore the impact of varying layer thickness on the structure and chemistry of solar cells. Thicker layers lead to over-alloying of selenium, causing a notable decline in photocurrent. Electron microscopy shows that the decline can be attributed to the formation of small grains with porous grain boundaries in the selenium inter-diffusion region. The small grain size may arise from a drag force exerted by segregated selenium solute atoms on moving grain boundaries. Faster diffusion along the grain boundaries lead to accumulation of vacancies and subsequent porosity. In conclusion, device processing conditions should be carefully considered to optimize selenium alloying for maximum performance benefits in solar cells.