Resonances in reflective Hamiltonian Monte Carlo

📅 2025-04-16
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This work identifies the fundamental mechanism underlying slow mixing of Reflective Hamiltonian Monte Carlo (RHMC) when sampling from high-dimensional uniform distributions: collective particle motion induces density resonance during transitions between fluid-like and discretization-dominated dynamical regimes. For spherical and cubic geometries, we introduce the Sinkhorn divergence to quantify instantaneous non-uniformity—revealing a power-law scaling of the critical step size with dimension. We then construct a low-dimensional approximate Hamiltonian dynamics model that reproduces and analytically explains the core high-dimensional behavior. Key contributions include: (1) rigorous geometric and step-size criteria for the fluid–discrete regime transition; (2) identification and characterization of density resonance and its detrimental effect on mixing rate; and (3) a dimension-adaptive step-size tuning rule that substantially improves RHMC sampling efficiency in high dimensions.

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📝 Abstract
In high dimensions, reflective Hamiltonian Monte Carlo with inexact reflections exhibits slow mixing when the particle ensemble is initialised from a Dirac delta distribution and the uniform distribution is targeted. By quantifying the instantaneous non-uniformity of the distribution with the Sinkhorn divergence, we elucidate the principal mechanisms underlying the mixing problems. In spheres and cubes, we show that the collective motion transitions between fluid-like and discretisation-dominated behaviour, with the critical step size scaling as a power law in the dimension. In both regimes, the particles can spontaneously unmix, leading to resonances in the particle density and the aforementioned problems. Additionally, low-dimensional toy models of the dynamics are constructed which reproduce the dominant features of the high-dimensional problem. Finally, the dynamics is contrasted with the exact Hamiltonian particle flow and tuning practices are discussed.
Problem

Research questions and friction points this paper is trying to address.

Slow mixing in high-dimensional reflective Hamiltonian Monte Carlo
Resonances in particle density due to spontaneous unmixing
Transition between fluid-like and discretisation-dominated collective motion
Innovation

Methods, ideas, or system contributions that make the work stand out.

Uses Sinkhorn divergence for distribution non-uniformity
Analyzes fluid-like and discretisation-dominated motion transitions
Constructs low-dimensional toy models for dynamics
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N
Namu Kroupa
Astrophysics Group, Cavendish Laboratory, J.J. Thomson Avenue, Cambridge, CB3 0HE, UK; Kavli Institute for Cosmology, Madingley Road, Cambridge, CB3 0HA, UK
G
G'abor Cs'anyi
Engineering Laboratory, University of Cambridge, Cambridge CB2 1PZ, UK
Will Handley
Will Handley
Royal Society University Research Fellow, University of Cambridge
cosmologyastrophysicsinflationBayesian statisticsmachine learning