Space-time autocoding constellations with pairwise-independent signals

T. Marzetta, B. Hassibi, B. Hochwald
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Abstract

Summary form only given. The space-time autocoding effect implies that arbitrarily reliable communication is possible within a single coherence interval in Rayleigh flat fading as the symbol-duration of the coherence interval and the number of transmit antennas grow simultaneously. For relatively short (e.g., 16-symbol) coherence intervals, a codebook of isotropically random unitary space-time signals theoretically supports transmission rates that are a significant fraction of autocapacity with an extremely low probability of error. However a constellation of the required size (typically L=2/sup 80/) is impossible to generate and store, and due to lack of structure there is little hope of finding a fast decoding scheme. We propose a random, but highly structured, constellation that is completely specified by log/sub 2/ L independent isotropically distributed unitary matrices. The distinguishing property of this construction is that any two signals in the constellation are pairwise statistically independent and isotropically distributed. Thus, the pairwise probability of error, and hence the union bound on the block probability of error, of the structured constellation is identical to that of a fully random constellation of independent signals.
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具有两两无关信号的时空自编码星座
只提供摘要形式。时空自编码效应意味着在瑞利平坦衰落中,随着相干间隔的符号持续时间和发射天线数量的同时增加,在单个相干间隔内可以实现任意可靠的通信。对于相对较短的相干间隔(例如,16个符号),各向同性随机统一时空信号的码本理论上支持的传输速率是自动容量的很大一部分,错误概率极低。然而,所需大小的星座(通常为L=2/sup 80/)是不可能生成和存储的,并且由于缺乏结构,找到快速解码方案的希望很小。我们提出了一个随机但高度结构化的星座,它完全由log/sub 2/ L独立的各向同性分布酉矩阵指定。这种结构的显著特性是星座中的任何两个信号在统计上是两两独立的,并且是各向同性分布的。因此,结构化星座的成对误差概率,以及块误差概率的联合界,与具有独立信号的完全随机星座的误差概率相同。
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