TY - JOUR
T1 - Asymptotic comparison of ML and MAP detectors for multidimensional constellations
AU - Alvarado, A.
AU - Agrell, E.
AU - Brännström, F.
PY - 2018/2/1
Y1 - 2018/2/1
N2 - A classical problem in digital communications is to evaluate the symbol error probability (SEP) and bit error probability (BEP) of a multidimensional constellation over an additive white Gaussian noise channel. In this paper, we revisit this problem for nonequally likely symbols and study the behavior of the optimal maximum a posteriori (MAP) detector at asymptotically high signal-to-noise ratios. Exact closed-form asymptotic expressions for SEP and BEP for arbitrary constellations and input distributions are presented. The well-known union bound is proven to be asymptotically tight under general conditions. The performance of the practically relevant maximum likelihood (ML) detector is also analyzed. Although the decision regions with MAP detection converge to the ML regions at high signal-to-noise ratios, the ratio between the MAP and ML detectors in terms of both SEP and BEP approaches a constant, which depends on the constellation and a priori probabilities. Necessary and sufficient conditions for asymptotic equivalence between the MAP and ML detectors are also presented.
AB - A classical problem in digital communications is to evaluate the symbol error probability (SEP) and bit error probability (BEP) of a multidimensional constellation over an additive white Gaussian noise channel. In this paper, we revisit this problem for nonequally likely symbols and study the behavior of the optimal maximum a posteriori (MAP) detector at asymptotically high signal-to-noise ratios. Exact closed-form asymptotic expressions for SEP and BEP for arbitrary constellations and input distributions are presented. The well-known union bound is proven to be asymptotically tight under general conditions. The performance of the practically relevant maximum likelihood (ML) detector is also analyzed. Although the decision regions with MAP detection converge to the ML regions at high signal-to-noise ratios, the ratio between the MAP and ML detectors in terms of both SEP and BEP approaches a constant, which depends on the constellation and a priori probabilities. Necessary and sufficient conditions for asymptotic equivalence between the MAP and ML detectors are also presented.
KW - Additive white Gaussian noise channel
KW - Bit error probability
KW - Error probability
KW - High-SNR asymptotics
KW - Maximum a posteriori
KW - Maximum likelihood
KW - Multidimensional constellations
KW - Symbol error probability
UR - http://www.scopus.com/inward/record.url?scp=85028842918&partnerID=8YFLogxK
U2 - 10.1109/TIT.2017.2727521
DO - 10.1109/TIT.2017.2727521
M3 - Article
SN - 0018-9448
VL - 64
SP - 1231
EP - 1240
JO - IEEE Transactions on Information Theory
JF - IEEE Transactions on Information Theory
IS - 2
M1 - 7982634
ER -