LGNov 24, 2025

Row-stochastic matrices can provably outperform doubly stochastic matrices in decentralized learning

arXiv:2511.19513v1
Originality Incremental advance
AI Analysis

This provides theoretical insights for optimizing decentralized learning topologies, though it is incremental as it builds on prior convergence analyses.

The paper tackles the problem of whether row-stochastic matrices can outperform doubly stochastic matrices in decentralized learning with heterogeneous node weights, and finds that row-stochastic designs can converge faster under certain conditions due to penalty terms in a weighted Hilbert-space framework.

Decentralized learning often involves a weighted global loss with heterogeneous node weights $λ$. We revisit two natural strategies for incorporating these weights: (i) embedding them into the local losses to retain a uniform weight (and thus a doubly stochastic matrix), and (ii) keeping the original losses while employing a $λ$-induced row-stochastic matrix. Although prior work shows that both strategies yield the same expected descent direction for the global loss, it remains unclear whether the Euclidean-space guarantees are tight and what fundamentally differentiates their behaviors. To clarify this, we develop a weighted Hilbert-space framework $L^2(λ;\mathbb{R}^d)$ and obtain convergence rates that are strictly tighter than those from Euclidean analysis. In this geometry, the row-stochastic matrix becomes self-adjoint whereas the doubly stochastic one does not, creating additional penalty terms that amplify consensus error, thereby slowing convergence. Consequently, the difference in convergence arises not only from spectral gaps but also from these penalty terms. We then derive sufficient conditions under which the row-stochastic design converges faster even with a smaller spectral gap. Finally, by using a Rayleigh-quotient and Loewner-order eigenvalue comparison, we further obtain topology conditions that guarantee this advantage and yield practical topology-design guidelines.

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