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The dispersion of infinite constellations

机译:无限星座的色散

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In the setting of a Gaussian channel without power constraints, proposed by Poltyrev, the codewords are points in an n-dimensional Euclidean space (an infinite constellation) and their optimal density is considered. Poltyrev''s “capacity” is the highest achievable normalized log density (NLD) with vanishing error probability. This capacity as well as error exponents for this setting are known. In this work we consider the optimal NLD for a fixed, nonzero error probability, as a function of the codeword length (dimension) n. We show that as n grows, the gap to capacity is inversely proportional (up to the first order) to the square-root of n where the proportion constant is given by the inverse Q-function of the allowed error probability, times the square root of 1 over 2. In an analogy to similar result in channel coding, the dispersion of infinite constellations is 1 over 2 nat2 per channel use. We show that this optimal convergence rate can be achieved using lattices, therefore the result holds for the maximal error probability as well. Connections to the error exponent of the power constrained Gaussian channel and to the volume-to-noise ratio as a figure of merit are discussed.
机译:在由Poltyrev提出的无功率约束的高斯信道的设置中,码字是n维欧几里德空间(无限星座)中的点,并考虑了它们的最佳密度。 Poltyrev的“容量”是可实现的最高归一化对数密度(NLD),误差概率消失了。已知此设置的容量以及错误指数。在这项工作中,我们考虑了固定的非零错误概率的最佳NLD,它是码字长度(维)n的函数。我们表明,随着n的增长,容量的差距与n的平方根成反比(直到第一阶),其中比例常数由允许的误差概率的反Q函数给出,乘以平方根类似于信道编码中的1个结果。无限星座的离散度是每个信道使用2个nat 2 中的1个。我们表明,使用晶格可以实现最佳收敛速度,因此结果也适用于最大错误概率。讨论了与功率受限高斯信道的误差指数以及作为品质因数的体积噪声比的关系。

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