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Principled Probabilistic Imaging using Diffusion Models as Plug-and-Play Priors

NeurIPS 2024 · Probabilistic and scientific modeling › Variational and generative sampling · approach: Importance sampling and quadrature · 11 citations (OpenAlex)

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Proposes PnP-DM, an MCMC posterior sampler that runs split Gibbs sampling with a likelihood Langevin/Gaussian step and a prior step solved exactly via EDM-formulated diffusion models, applied to linear, nonlinear, and black hole imaging inverse problems.

Problem

Existing diffusion-model inverse solvers approximate the intractable likelihood score, so their samples deviate from the true Bayesian posterior for general (linear and nonlinear) imaging inverse problems.

Approach

Reduce posterior sampling to a Gaussian denoising posterior sampling problem solved by split Gibbs sampling, and solve the denoising step rigorously by running the reverse SDE of any diffusion model converted to the unified EDM formulation, with an annealed coupling parameter rho.

Key results

Measured effects reported in the paper

What was changedWhereMeasuredEffect
Use PnP-DM (EDM) instead of DPnPGaussian deblurring · FFHQ validation, Gaussian deblurPSNR: 29.24 -> 29.66Helped
Use PnP-DM (VE) instead of DPnPMotion deblurring · FFHQ validation, motion deblurPSNR: 30.21 -> 30.38Helped
Use PnP-DM (EDM) instead of DPnPSuper-resolution · FFHQ validation, super-resolution (4×)PSNR: 29.32 -> 29.60Helped
Use PnP-DM (iDDPM) instead of DPSCoded diffraction patterns · FFHQ test, coded diffraction patternsPSNR: 33.43 -> 33.35Hurt
Use PnP-DM (EDM) instead of DPnPFourier phase retrieval · FFHQ test, Fourier phase retrievalPSNR: 29.28 -> 31.14Helped
Replace the VP diffusion prior with the VE diffusion prior (ablation)PnP-DM · FFHQ validation, Gaussian deblurPSNR: 29.46 -> 29.65Helped
Replace the VP diffusion prior with the EDM diffusion prior (ablation)PnP-DM · FFHQ validation, motion deblurPSNR: 30.06 -> 30.35Helped
Replace the VP diffusion prior with the EDM diffusion prior (ablation)PnP-DM · FFHQ validation, super-resolution (4×)PSNR: 29.40 -> 29.60Helped
Replace the VP diffusion prior with the iDDPM diffusion prior (ablation)PnP-DM · FFHQ test, coded diffraction patternsPSNR: 32.91 -> 33.35Helped
Replace the VP diffusion prior with the EDM diffusion prior (ablation)PnP-DM · FFHQ test, Fourier phase retrievalPSNR: 30.36 -> 31.14Helped

Surprising findings

Limitations

Experimental setup

Datasets: FFHQ CelebA EHT 2017 M87 observations GRMHD black hole simulations

Benchmarks: FFHQ 100 validation images (Gaussian deblur, motion deblur, super-resolution, CDP, Fourier phase retrieval) black hole imaging (simulated Sgr A* and real M87 data) synthetic Gaussian prior with known posterior

Metrics: PSNR SSIM LPIPS uncertainty calibration (3-sigma coverage) data mismatch chi-squared

Baselines: PnP-ADMM DPIR DDRM DPS PnP-SGS DPnP HIO

Builds on: Split Gibbs Sampler EDM DPS DPnP PnP-SGS

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