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Quantum Fourier Transform Based Kernel for Solar Irrandiance Forecasting

Nawfel Mechiche-Alami, Eduardo Rodriguez, Jose M. Cardemil, Enrique Lopez Droguett

TL;DR

The paper tackles the challenge of improving short-term solar irradiance forecasting by leveraging a quantum kernel that incorporates a Quantum Fourier Transform (QFT). It introduces an amplitude-encoded, QFT-based kernel with a protective rotation layer and fuses per-feature kernels via convex weights within kernel ridge regression, benchmarked against classical RBF and polynomial kernels across 30 BSRN stations and Köppen climate classes. The study reports consistent gains in $nRMSE$ and $R^{2}$, near-zero $nMBE$, and tighter MAE/ERMAX when using the quantum kernel, while acknowledging limitations from noiseless simulation and fixed classical hyperparameters. The findings suggest that frequency-aware quantum embeddings can capture diurnal/seasonal patterns more effectively in time-series forecasting and could be extended to other periodic domains and eventual NISQ deployments with further robustness and scalability work.

Abstract

This study proposes a Quantum Fourier Transform (QFT)-enhanced quantum kernel for short-term time-series forecasting. Each signal is windowed, amplitude-encoded, transformed by a QFT, then passed through a protective rotation layer to avoid the QFT/QFT adjoint cancellation; the resulting kernel is used in kernel ridge regression (KRR). Exogenous predictors are incorporated by convexly fusing feature-specific kernels. On multi-station solar irradiance data across Koppen climate classes, the proposed kernel consistently improves median R2 and nRMSE over reference classical RBF and polynomials kernels, while also reducing bias (nMBE); complementary MAE/ERMAX analyses indicate tighter average errors with remaining headroom under sharp transients. For both quantum and classical models, the only tuned quantities are the feature-mixing weights and the KRR ridge alpha; classical hyperparameters (gamma, r, d) are fixed, with the same validation set size for all models. Experiments are conducted on a noiseless simulator (5 qubits; window length L=32). Limitations and ablations are discussed, and paths toward NISQ execution are outlined.

Quantum Fourier Transform Based Kernel for Solar Irrandiance Forecasting

TL;DR

The paper tackles the challenge of improving short-term solar irradiance forecasting by leveraging a quantum kernel that incorporates a Quantum Fourier Transform (QFT). It introduces an amplitude-encoded, QFT-based kernel with a protective rotation layer and fuses per-feature kernels via convex weights within kernel ridge regression, benchmarked against classical RBF and polynomial kernels across 30 BSRN stations and Köppen climate classes. The study reports consistent gains in and , near-zero , and tighter MAE/ERMAX when using the quantum kernel, while acknowledging limitations from noiseless simulation and fixed classical hyperparameters. The findings suggest that frequency-aware quantum embeddings can capture diurnal/seasonal patterns more effectively in time-series forecasting and could be extended to other periodic domains and eventual NISQ deployments with further robustness and scalability work.

Abstract

This study proposes a Quantum Fourier Transform (QFT)-enhanced quantum kernel for short-term time-series forecasting. Each signal is windowed, amplitude-encoded, transformed by a QFT, then passed through a protective rotation layer to avoid the QFT/QFT adjoint cancellation; the resulting kernel is used in kernel ridge regression (KRR). Exogenous predictors are incorporated by convexly fusing feature-specific kernels. On multi-station solar irradiance data across Koppen climate classes, the proposed kernel consistently improves median R2 and nRMSE over reference classical RBF and polynomials kernels, while also reducing bias (nMBE); complementary MAE/ERMAX analyses indicate tighter average errors with remaining headroom under sharp transients. For both quantum and classical models, the only tuned quantities are the feature-mixing weights and the KRR ridge alpha; classical hyperparameters (gamma, r, d) are fixed, with the same validation set size for all models. Experiments are conducted on a noiseless simulator (5 qubits; window length L=32). Limitations and ablations are discussed, and paths toward NISQ execution are outlined.

Paper Structure

This paper contains 21 sections, 28 equations, 13 figures, 1 table.

Figures (13)

  • Figure 1: General quantum circuit used to compute the kernel value between the two datapoints x and y.
  • Figure 2: QFT based quantum kernel using n qubits.
  • Figure 3: Example of the protective layer $V(\cdot)$ on 3 qubits
  • Figure 4: Protective layer $V(\cdot)$ on n qubits where $a+b$ is odd
  • Figure 5: Feature combination scheme using toy datasets.
  • ...and 8 more figures