# Quantitative theory of the grain boundary impact on the open-circuit   voltage of polycrystalline solar cells

**Authors:** Benoit Gaury, Paul M. Haney

arXiv: 1902.03587 · 2019-02-12

## TL;DR

This paper develops a quantitative model linking grain boundary properties in polycrystalline solar cells to their impact on open-circuit voltage, aiding understanding of defect effects on device performance.

## Contribution

The work extends previous models to include tilted and intersecting grain boundaries, providing a comprehensive analytical tool for predicting photovoltaic performance.

## Key findings

- Model accurately predicts open-circuit voltage considering grain boundary networks.
- Analytical model applies to inhomogeneous grain boundary systems.
- Bridges nanoscale characterization data with macroscale device performance.

## Abstract

Thin film polycrystalline photovoltaics are a mature, commercially-relevant technology. However, basic questions persist about the role of grain boundaries in the performance of these materials, and the extent to which these defects may limit further progress. In this work, we first extend previous analysis of columnar grain boundaries to develop a model of the recombination current of "tilted" grain boundaries. We then consider systems with multiple, intersecting grain boundaries and numerically determine the parameter space for which our analytical model accurately describes the recombination current. We find that for material parameters relevant for thin film photovoltaics, our model can be applied to compute the open-circuit voltage of materials with networks of inhomogeneous grain boundaries. This model bridges the gap between the distribution of grain boundary properties observed with nanoscale characterization and their influence on the macroscale device open-circuit voltage.

## Full text

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## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1902.03587/full.md

## References

32 references — full list in the complete paper: https://tomesphere.com/paper/1902.03587/full.md

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Source: https://tomesphere.com/paper/1902.03587