Blue-noise sampling is formulated as sampling from a Gibbs distribution over binary lattice occupancies with pairwise repulsive interactions, and the model, the sampler, and these guarantees separately are validated.
Abstract
Blue-noise sampling is widely used in computer graphics, but existing methods separate statistical modeling from scalable generation. Optimization and transport methods produce high-quality point sets by coupling all samples together. Procedural and tile-based samplers are local, but define their output only implicitly. We formulate blue-noise generation as sampling from a Gibbs distribution over binary lattice occupancies with pairwise repulsive interactions. Density, repulsion strength, interaction scale, and kernel hardness are parameters of this distribution. Because the energy sums over pairs, distant interactions can be dropped with a bounded change to the distribution, leaving a Markov random field of bounded degree. To sample it, we trace the Markov chain backward from the state we want, following Coupling Towards The Past, and cut the trace at a fixed depth. This bounds the cost, and it bounds the region each sample depends on. A tile generated on its own, with a sufficient halo, is then bit-identical to the same region generated on any larger domain, in any order and with no communication between tiles. Memory is set by the tile size, not by the output size, and accuracy is traded against cost through parameters with a proven error bound rather than by switching algorithms. We validate the model, the sampler, and these guarantees separately. The ensemble reproduces standard blue-noise spectra and moves continuously between them as its parameters vary. The sampler matches its predicted work and memory. Tiled output is verified bit-identical to full-domain generation. We demonstrate adaptive stippling at 14K, where existing methods need memory proportional to the output, along with multi-class extensions.
Some of the sharpest challenges in sampling from the energy functions of physical systems arise at phase transitions, where the density of states changes abruptly and many sampling algorithms stall. Nested sampling is a particle method that traverses the density of states under a hard energy constraint and is known to...
Sampling from the Boltzmann distribution is central to computational physics, yet hard when the energy is known only through a stochastic estimate, such as with machine-learned molecular potentials, in variational Monte Carlo, or on quantum computers, because a noisy energy biases the sampled distribution. The penalty...
Iwo Sanderski, Gian Gentinetta, Giuseppe Carleo· 0 citations
This work introduces NS-Flows: a single conditional normalizing flow, conditioned on the NS energy bound and trained on a sliding window of recent live sets, that replaces MCMC by direct parallel draws corrected by importance-weighted rejection resampling, allowing flow training without structured priors or a pre-exist...
A. Coretti, N. Unglert, Sebastian Falkner et al.· 0 citations
In Markov chain Monte Carlo sampling, light-tailed target distributions present something of a poisoned chalice: their light tails offer good confinement, and tend to imply good mixing properties for natural continuous-time dynamics, but the steepness of their tail decay means that they often fall outside of the scope...
Normalizing Flow Flow Maps (NF$^2$M), which combines the strengths of recent stochastic flow maps with the tractability of classic normalizing flows to build a Boltzmann Generator, and is evaluated on peptide systems, demonstrating improved sampling efficiency and sample quality.
Louis Grenioux, Rui-Kang Ouyang, Lu-Huan Wu· 0 citations
Nii-MALA is introduced, a high-performance C implementation of the Metropolis-Adjusted Langevin Algorithm, which leverages Message Passing Interface for parallelization and incorporates automatic differentiation backends for gradient evaluation and benchmark it against several other codes using radial velocity data fro...
Jia-Men Jiao, Sheng Jin, Wen-Xin Jiang et al.· Publications of the Astronom...· 0 citations
We use cookies to run the site and, with your consent, for analytics and to show ads.
See our Cookie Policy.