Sample Size Analysis of Energy Detection under Fading Channels

M. López-Benítez, Ogeen H. Toma, Dhaval K. Patel, K. Umebayashi
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Abstract

The performance of energy detection under fading channels has been evaluated in terms of the average probability of detection as a function of the average Signal-to-Noise Ratio (SNR) and the channel fading parameters, assuming that the decision threshold is set to achieve a constant false alarm rate. However, the signal sample size, which is an important design parameter in the configuration of an energy detector and has a significant impact on its performance, has received no attention in the context of fading channels. The mathematical expressions available in the literature to calculate the sample size required to achieve desired target performance are valid for Additive White Gaussian Noise (AWGN) channels only, and the impact of fading on the required sample size remains unknown. In this context, this work fills the existing gap by providing analytical results that establish a direct relation between the channel fading parameters and the required sample size. The results are provided for a broad variety of fading models (Rayleigh, Nakagami-m, Nakagami-q/Hoyt, Nakagami-n/Rice, etaâ€"mu and kappaâ€"mu) in terms of elementary functions, which enables highly efficient numerical evaluations.
衰落信道下能量检测的样本量分析
假设设置决策阈值以实现恒定的虚警率,以平均检测概率作为平均信噪比(SNR)和信道衰落参数的函数来评价衰落信道下的能量检测性能。然而,信号样本大小作为能量探测器配置中的一个重要设计参数,对其性能有重要影响,但在衰落信道中却没有受到重视。文献中可用的用于计算实现预期目标性能所需样本量的数学表达式仅对加性高斯白噪声(AWGN)信道有效,并且衰落对所需样本量的影响仍然未知。在这种情况下,本工作通过提供在信道衰落参数和所需样本量之间建立直接关系的分析结果填补了现有的空白。结果提供了各种各样的衰落模型(Rayleigh, Nakagami-m, Nakagami-q/Hoyt, Nakagami-n/Rice, eta - mu和kappa - mu)的初等函数,从而实现了高效的数值评估。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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