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Scaling Exponent and Moderate Deviations Asymptotics of Polar Codes for the AWGN Channel

Published 8 Jun 2017 in cs.IT and math.IT | (1706.02458v1)

Abstract: This paper investigates polar codes for the additive white Gaussian noise (AWGN) channel. The scaling exponent μ\mu of polar codes for a memoryless channel qY∣Xq_{Y|X} with capacity I(qY∣X)I(q_{Y|X}) characterizes the closest gap between the capacity and non-asymptotic achievable rates in the following way: For a fixed ε∈(0,1)\varepsilon \in (0, 1), the gap between the capacity I(qY∣X)I(q_{Y|X}) and the maximum non-asymptotic rate Rn∗R_n^* achieved by a length-nn polar code with average error probability ε\varepsilon scales as n−1/μn^{-1/\mu}, i.e., I(qY∣X)−Rn∗=Θ(n−1/μ)I(q_{Y|X})-R_n^* = \Theta(n^{-1/\mu}). It is well known that the scaling exponent μ\mu for any binary-input memoryless channel (BMC) with I(qY∣X)∈(0,1)I(q_{Y|X})\in(0,1) is bounded above by $4.714$, which was shown by an explicit construction of polar codes. Our main result shows that $4.714$ remains to be a valid upper bound on the scaling exponent for the AWGN channel. Our proof technique involves the following two ideas: (i) The capacity of the AWGN channel can be achieved within a gap of O(n−1/μlog⁡n)O(n^{-1/\mu}\sqrt{\log n}) by using an input alphabet consisting of nn constellations and restricting the input distribution to be uniform; (ii) The capacity of a multiple access channel (MAC) with an input alphabet consisting of nn constellations can be achieved within a gap of O(n−1/μlog⁡n)O(n^{-1/\mu}\log n) by using a superposition of log⁡n\log n binary-input polar codes. In addition, we investigate the performance of polar codes in the moderate deviations regime where both the gap to capacity and the error probability vanish as nn grows. An explicit construction of polar codes is proposed to obey a certain tradeoff between the gap to capacity and the decay rate of the error probability for the AWGN channel.

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