Design and Performance Analysis of Non-Coherent Detection Systems with Massive Receiver Arrays

TL;DR

This paper investigates non-coherent energy detection systems with massive receiver arrays in mmWave bands, demonstrating their robustness, scalability, and performance advantages over traditional methods, especially in high SNR regimes.

Contribution

It introduces two energy detection methods based on channel energy, analyzes their scaling laws, and compares their performance to coherent detection, highlighting advantages in complexity and robustness.

Findings

SER decreases linearly with the number of antennas

Performance approaches coherent detection at high SNR

Saturation occurs for high-order PAM due to channel energy uncertainty

Abstract

Harvesting the gain of a large number of antennas in a mmWave band has mainly been relying on the costly operation of channel state information (CSI) acquisition and cumbersome phase shifters. Recent works have started to investigate the possibility to use receivers based on energy detection (ED), where a single data stream is decoded based on the channel and noise energy. The asymptotic features of the massive receiver array lead to a system where the impact of the noise becomes predictable due to a noise hardening effect. This in effect extends the communication range compared to the receiver with a small number of antennas, as the latter is limited by the unpredictability of the additive noise. When the channel has a large number of spatial degrees of freedom, the system becomes robust to imperfect channel knowledge due to channel hardening. We propose two detection methods based on the instantaneous and average channel energy, respectively. Meanwhile, we design the detection thresholds based on the asymptotic properties of the received energy. Differently from existing works, we analyze the scaling law behavior of the symbol-error-rate (SER). When the instantaneous channel energy is known, the performance of ED approaches that of the coherent detection in high SNR scenarios. When the receiver relies on the average channel energy, our performance analysis is based on the exact SER, rather than an approximation. It is shown that the logarithm of SER decreases linearly as a function of the number of antennas. Additionally, a saturation appears at high SNR for PAM constellations of order larger than two, due to the uncertainty on the channel energy. Simulation results show that ED, with a much lower complexity, achieves promising performance both in Rayleigh fading channels and in sparse channels.