# Uncertainty propagation in financial models of photovoltaic systems

**Authors:** Stefan Wieland, Utku Gürsal

PMC · DOI: 10.1038/s41598-026-38053-1 · Scientific Reports · 2026-02-04

## TL;DR

This paper introduces a new method to accurately track uncertainty in financial models for solar energy systems, showing that it can lead to different results than traditional methods.

## Contribution

A numerically inexpensive approach for exact uncertainty propagation in photovoltaic financial models using analytic shortcuts.

## Key findings

- Key financial metrics can differ significantly from standard approximation methods.
- Input uncertainty alone can significantly impact financial analysis outcomes.

## Abstract

Financial analysis has a long history of capturing the stochasticity of real-world phenomena. For informed investment decisions, it is crucial to understand and quantify uncertainty propagation from financial model input to output. Yet to that end, in the photovoltaics sector one has so far relied on coarse-grained approximations or extensive simulations. Here we present a numerically inexpensive approach that exactly traces uncertainty propagation on the level of probability distributions. It leverages analytic shortcuts through switching between different distribution representations, and only assumes independent input variables. With the financial analysis of a typical photovoltaic system as a case study, we use this approach to compute key financial metrics and demonstrate that their values can differ significantly from those obtained by a standard approximation. Moreover, we show with both frameworks that input uncertainty alone can significantly impact the outcome of financial analysis.

## Full-text entities

- **Diseases:** T (MESH:D001260)
- **Chemicals:** PV (-), T (MESH:D014316)

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12877191/full.md

## References

15 references — full list in the complete paper: https://tomesphere.com/paper/PMC12877191/full.md

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Source: https://tomesphere.com/paper/PMC12877191