From Continuous to Discrete: a No-U-Turn Sampler for Permutations
Nawaf Bou-Rabee, Zichu Wang
TL;DR
This work introduces a discrete No-Underrun Sampler (NURS) as a permutation-space analogue of No-U-Turn sampling, enabling local adaptivity on the symmetric group $S_n$ for Mallows distributions with $P_\beta(\sigma) \propto e^{-\beta d(\sigma,\sigma_0)}$. By replacing Hamiltonian trajectories with measure-preserving group orbits and employing a randomized dyadic doubling and no-underrun stopping rule, NURS achieves a rejection-free, reversible kernel via a Gibbs Self-Tuning (GIST) framework. The authors prove reversibility, develop a shift-coupling argument, and establish a path-coupling based mixing-time bound of $O(n^2\log n)$ in a high-temperature, Lipschitz-energy regime, with explicit edge-wise contraction factors. Numerical experiments across Kendall, $L^1$, $L^2$, Hamming, Cayley, and Ulam distances corroborate the theory, demonstrating effective exploration in warm regimes and revealing the impact of direction laws (uniform, block-shuffle, local) on mixing. The framework paves the way for orbit-based reversible sampling beyond permutations, linking discrete analogues of Hamiltonian ideas to structured discrete spaces.
Abstract
We introduce a discrete-space analogue of the No-U-Turn sampler on the symmetric group $S_n$, yielding a locally adaptive and reversible Markov chain Monte Carlo method for $\mathrm{Mallows}(d,σ_0)$. Here $d:S_n\times S_n\to[0,\infty)$ is any fixed distance on $S_n$, $σ_0\in S_n$ is a fixed reference permutation, and the target distribution on $S_n$ has mass function $π(σ)\propto e^{-βd(σ,σ_0)}$ where $β>0$ is the inverse temperature. The construction replaces Hamiltonian trajectories with measure-preserving group-orbit exploration. A randomized dyadic expansion is used to explore a one-dimensional orbit until a probabilistic \emph{no-underrun} criterion is met, after which the next state is sampled from the explored orbit with probability proportional to the target weights. On the theory side, embedding this transition within the Gibbs self-tuning (GIST) framework provides a concise proof of reversibility. Moreover, we construct a \emph{shift coupling} for orbit segments and prove an explicit edge-wise contraction in the Cayley distance under a mild Lipschitz condition on the energy $E(σ)=d(σ,σ_0)$. A path-coupling argument then yields an $O(n^2\log n)$ total-variation mixing-time bound.
