The Application of Quantum Fourier Transform in Cosmic Microwave Background Data Analysis
Farida Farsian, Tiziana Trombetti, Carlo Burigana, Francesco Schillir\'o, Andrea Bulgarelli, Vincenzo Cardone, Luca Cappelli, Massimo Meneghetti, Giuseppe Murante, Alessandro Rizzo, Giuseppe Sarracino, Irene Graziotti, Roberto Scaramella, Vincenzo Testa

TL;DR
This paper explores replacing the classical FFT with the Quantum Fourier Transform in cosmic microwave background data analysis, highlighting potential speedups at high resolution and discussing current limitations due to data encoding overhead.
Contribution
It investigates the application of QFT in CMB analysis, demonstrating potential advantages and identifying data encoding as a key bottleneck for quantum speedup.
Findings
QFT shows potential advantages over FFT at high resolutions
Classical-to-quantum data encoding overhead limits current efficiency
Future improvements could enhance quantum speedup feasibility
Abstract
The Cosmic Microwave Background (CMB) data analysis and the map-making process rely heavily on the use of spherical harmonics. For suitable pixelizations of the sphere, the (forward and inverse) Fourier transform plays a crucial role in computing all-sky map from spherical harmonic expansion coefficients -- or from angular power spectrum -- and vice versa. While the Fast Fourier Transform (FFT) is traditionally employed in these computations, the Quantum Fourier Transform (QFT) offers a theoretical advantage in terms of computational efficiency and potential speedup. In this work, we study the potential advantage of using the QFT in this context by exploring the substitution of the FFT with the QFT within the \textit{healpy} package. Performance evaluations are conducted using the Aer simulator. Our results indicate that QFT exhibits potential advantages over FFT that are particularly…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Quantum Information and Cryptography
