Sparse Grassmannian Design for Noncoherent Codes via Schubert Cell Decomposition
Joe Asano, Yuto Hama, Hiroki Iimori, Chandan Pradhan, Szabolcs Malomsoky, Naoki Ishikawa
TL;DR
The paper tackles noncoherent MIMO signaling by introducing sparse Grassmannian constellations that exploit Schubert-cell sparsity to reduce detection complexity while maintaining performance. It provides a rank-aware PEP bound to correctly characterize SER under rank-deficient configurations and derives a closed-form AMI lower bound that leads to a practical design metric. The proposed MCPD-oriented design, combined with Schubert-cell decomposition and pattern lifting, yields sparse constellations that outperform conventional Grassmannian designs and approach optimal performance at high SNR, with linear-time/space complexity in the number of codewords. The approach is demonstrated through theoretical insights and a detailed example at (T,M)=(4,2), showing improved SER/AMI and reduced complexity, with scalable behavior for moderate cardinalities. This framework offers a viable path for robust, low-complexity noncoherent signaling in large-MIMO IoT and beyond-5G/6G systems.
Abstract
In this paper, we propose a method for designing sparse Grassmannian codes for noncoherent multiple-input multiple-output systems. Conventional pairwise error probability formulations under uncorrelated Rayleigh fading channels fail to account for rank deficiency induced by sparse configurations. We revise these formulations to handle such cases in a unified manner. Furthermore, we derive a closed-form metric that effectively maximizes the noncoherent average mutual information (AMI) at a given signal-to-noise ratio. We focus on the fact that the Schubert cell decomposition of the Grassmann manifold provides a mathematically sparse property, and establish design criteria for sparse noncoherent codes based on our analyses. In numerical results, the proposed sparse noncoherent codes outperform conventional methods in terms of both symbol error rate and AMI, and asymptotically approach the performance of the optimal Grassmannian constellations in the high-signal-to-noise ratio regime. Moreover, they reduce the time and space complexity, which does not scale with the number of transmit antennas.
