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arXiv:2605.23611

Single-Photon Fourier Transform

Zhen Yang, Zeng‐Quan Yan, Li Wang, Xiao‐Wei Wang, Ka-Di Zhu, Xian-Min Jin

Published May 22, 2026• 0 citations
arXivHTMLPDF

Abstract

The extraction of information carried by light plays an increasingly important role in optical communication, imaging, and detection. However, the information can only be successfully extracted when the light pulse is comparably strong, leaving untouched scenarios where survived photons are extremely sparse. Here, we propose and experimentally demonstrate a single-photon Fourier transform scheme. By retrieving the implicit correlation shared in the sparse singlephoton stream globally, we are able to precisely classify each photon and synchronously extract multiple ultra-weak signals with high fidelity against extreme environments. Our experiment results give a full picture of the scheme in terms of multi-terminal expandability, wide frequency adaptability, 125 dB loss tolerance, and -10.4 dB signal-to-noise ratio robustness. Even when the pulse repetition frequencies of all terminals are the same, we can still recognize the free-running clock drift and separate different messages. Our work can be a general scheme to extend the capability boundary for all the extremely low-light-flux scenarios, and makes many challenging tasks possible, such as in-orbit optical communication network with complex topology, navigation in extremely lossy and noisy environments, and wide-range single-photon imaging with multi-source illumination.

DOI
10.48550/arxiv.2605.23611

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Abstract Accurate detection and identification of space-based faint targets under strong background is a pressing challenge for all‑weather deep space exploration. However, active deep space detection is often hampered by the disturbances of intense stellar stray light and multi-source heterogeneous noise, making it difficult to achieve noise‑blind source separation and accurate identification of weak target signals under extremely low signal-to-noise ratio. To address these challenges, we develop a random dynamic mask modulation scheme to enhance higher-order coherence, unveiling power-law photon number distributions and super-bunching correlations that enable higher-order photon correlation imaging with a single-photon detector array (SPDA). The imaging scheme decouples the target signal from multi-source disturbances including coherent, thermal, and super-bunching light, as well as multiple background noises such as shot noise, environmental stray light, and dark counts. Here, we experimentally demonstrate a super-bunching light with a fiftieth-order photon correlation of 1.45×10 72 at a mean photon number , achieving a 10 42 enhancement in the high-to-second-order correlation ratio. The super-bunching light source enables continuously tunable output intensity from ultra‑weak to extremely bright, overcoming the limitation of conventional sources that produce only ultra‑weak photon numbers. Strikingly, we observe the ratio R n >2 of the multiphoton probability between the signal power-law light and a noise coherent laser reaching 5.29×10 269 at for 281 photons. The contrast in higher-order photon correlation imaging reaches 0.99, increasing by 0.26 over the second-order case. At an imaging exposure time of 5 µs and a mean photon number , we achieve 512×512‑pixel SPDA imaging with a dynamic range of 252.93 dB despite simultaneous photon‑starved signal and intense background. Our noise‑blind scheme establishes ultra‑wide dynamic range, high‑speed, sub-megapixel single‑photon imaging under multi‑source noise and intense optical disturbances, opening new routes for space surveillance and quantum‑enhanced detection.