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中国物理学会期刊

空间信道大气湍流环境下量子安全直接通信协议研究

Research on Quantum Secure Direct Communication Protocol in Atmospheric Turbulence Environment of Space Channel

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  • 量子安全直接通信是一种能够在量子信道中直接传输机密信息的通信范式,在自由空间通信中展现出重要的实用潜力与部署前景。然而,大气湍流等环境因素会降低信号传输质量与系统安全性。本文分析了空间信道诱骗态DL04协议,建立了自由空间水平链路量子安全直接通信系统的综合性能分析模型,量化分析了光学系统参数和实际环境因素对系统保密容量的影响规律。仿真结果表明:发射接收孔径与初始光斑尺寸需根据系统条件权衡选取,存在最优配置;与雪崩光电二极管单光子探测器相比,采用超导纳米线单光子探测器可有效提升中短距离下的保密容量,但对最大安全通信距离的提升作用有限;湍流强度与大气可见度是影响系统最大安全通信距离的关键因素;白天强背景光是主要噪声源之一,需通过滤波技术予以抑制。本研究可为实际自由空间量子安全直接通信系统的链路预算与参数优化提供理论依据和设计指导。

     

    This study presents a comprehensive performance evaluation of the decoy state DL04 quantum secure direct communication (QSDC) protocol over near ground free space horizontal links, with particular emphasis on the combined effects of atmospheric turbulence, aerosol extinction, and background radiation. Unlike previous works that often focus on quantum key distribution or treat environmental factors in isolation, we develop an integrated analytical framework that simultaneously accounts for spatial diffraction of Gaussian beams, Beer–Lambert extinction due to molecular and aerosol scattering, and turbulence induced beam broadening and wandering described by the HV 21/HV Night turbulence models. The turbulent instantaneous transmittance is modelled by a Weibull distribution, from which the average turbulence induced loss is derived. The system performance is quantified by the asymptotic secure capacity under collective attacks and photon number splitting attacks, with single and two photon error rates tightly estimated via a four decoy state protocol. The quantum bit error rate is formulated to include detector dark counts, afterpulsing, intrinsic optical errors, and, crucially, the bidirectional background noise contributions from both the forward (Bob–Alice) and round trip (Bob–Alice–Bob) paths.
    Numerical simulations are carried out at 1550 nm wavelength, using typical commercial parameters for both avalanche photodiode (APD) and superconducting nanowire single photon detector (SNSPD). Key quantitative findings are as follows. (1) The receiving aperture and initial beam size exhibit non monotonic optimization: increasing the aperture improves signal collection but also enhances background noise ingress, especially under strong daytime irradiance, leading to an optimum aperture for maximum secure distance; similarly, an optimal initial beam radius exists that balances far field divergence and aperture overfill. (2) SNSPD improves the secure capacity by a factor of 2–3 compared with APD at short to medium ranges, yet the maximum secure communication distance differs marginally between the two detectors. This result indicates that the ultimate range is fundamentally limited by atmospheric channel attenuation rather than detector sensitivity. (3) Turbulence strength and atmospheric visibility are the dominant environmental determinants: below 5 km visibility, extinction overwhelms all other losses and masks day–night differences; above 50 km visibility, further improvement yields diminishing returns as diffraction and turbulence become the residual limiting factors. (4) Daytime background irradiance (~10-5 W/(m2·sr·nm)) severely degrades both secure capacity and range, necessitating aggressive spatial, spectral, and temporal filtering; in contrast, nighttime irradiance (as low as 10-8) contributes negligible noise, making nocturnal operation highly favourable for high rate secure communication. (5) Elevation dependence shows that performance saturates above approximately 700 m during daytime and above 350 m at night, suggesting that modest altitude gain can significantly mitigate near ground turbulence.
    These results provide a quantitative, physically transparent basis for link budget design, site selection, detector choice, and operational scheduling in practical free space QSDC deployments. The model also reveals the distinct regimes where diffraction, extinction, or turbulence dominates, offering guidance for adaptive system optimisation under varying weather and diurnal conditions.

     

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