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Finite codelength analysis of the sequential waveform nulling receiver for M-ary PSK

机译:Mary PSK的连续波形调零接收机的有限码长分析

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The conditions for a quantum measurement to discriminate a set of states with the minimum probability of error were specified by Yuen, Kennedy and Lax, and are often termed the YKL conditions [1]. Since light is quantum mechanical, the ultimate limit on minimum-error discrimination of an optical modulation constellation is determined by the YKL bound. Standard optical receivers (i.e., direct, homodyne or heterodyne detection)—even at their respective ideal operation limits—cannot achieve this performance. Recently, it was shown that a ‘sequential waveform nulling’ (SWN) receiver can, not only discriminate an arbitrary M-ary coherent-state (ideal laser-light) constellation asymptotically at the YKL bound in the high-power limit, but that it achieves a factor of 4 better in the asymptotic error-probability exponent compared with heterodyne detection—the only conventional optical receiver that can in principle be employed for detecting an arbitrary phase-and-amplitude modulated constellation [2]. The SWN receiver can be built with standard optical components; i.e., beamsplitters, local-oscillator lasers, delay loops and single-photon detectors. However on the other hand, in the high power regime, heterodyne detection is known to achieve a reliable communication rate that asymptotically approaches the Holevo capacity of a lossy-noisy optical channel (the ultimate limit to the classical capacity of a quantum channel) [3]. In fact, in the high power regime, heterodyne detection was also shown recently to achieve the optimal second-order coding rate, when using the optimal (Gaussian) input distribution [4]. In this paper, we show that when restricted to the M-ary phase-shift keying (PSK) ensemble, that the SWN receiver's superiority over heterodyne detection in its asymptotic error exponent of the demodulation error probability, translates to a slightly higher capacity and a pronouncedly higher finite blocklength reliable-communica- ion rate. We also quantify, via a numerical calculation, the dependence of the SWN receiver's capacity on the order in which the PSK constellation points are nulled. Our results suggest that for short-latency PSK-modulated optical communication in the high spectral efficiency regime—for which heterodyne detection is the conventional receiver choice—that it may be beneficial to employ the SWN receiver, despite the widely-regarded capacity optimality of heterodyne detection in this operating regime.
机译:Yuen,Kennedy和Lax规定了以最小的误差概率来区分一组状态的量子测量条件,这些条件通常称为YKL条件[1]。由于光是量子力学的,因此对光调制星座图的最小误差判别的最终限制由YKL界限确定。即使在它们各自的理想操作极限下,标准光学接收器(即,直接,零差或外差检测)也不能达到这一性能。最近,研究表明,“连续波形调零”(SWN)接收器不仅可以渐近地在高功率限制的YKL边界上渐近地辨别出任意的M元相干态(理想激光)星座,而且与外差检测相比,它在渐近误差概率指数上的系数提高了4倍-外差检测是唯一可以在原则上用于检测任意相位和幅度调制星座的传统光接收器[2]。 SWN接收器可以内置标准光学组件。即分束器,本地振荡器激光器,延迟环路和单光子检测器。但是,另一方面,在高功率状态下,外差检测可实现可靠的通信速率,渐近地接近有噪光信道的Holevo容量(对量子信道经典容量的最终限制)[3 ]。实际上,在高功率状态下,当使用最佳(高斯)输入分布时,最近也显示了外差检测可以实现最佳的二阶编码率[4]。在本文中,我们表明,当限于M元相移键控(PSK)组合时,SWN接收机在解调误差概率的渐近误差指数方面优于外差检测,将转化为稍高的容量和有限块长可靠通信速率明显更高。我们还通过数值计算来量化SWN接收机容量对PSK星座图点为零的顺序的依赖性。我们的结果表明,对于高频谱效率体制中的短时延PSK调制光通信(外差检测是常规接收器的选择),尽管外差器的容量最佳性得到了广泛认可,但使用SWN接收器还是有好处的在这种操作方式下进行检测。

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