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Ensemble Kalman Diffusion Guidance: A Derivative-free Method for Inverse Problems

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When solving inverse problems, one increasingly popular approach is to use pre-trained diffusion models as plug-and-play priors. This framework can accommodate different forward models without re-training while preserving the generative capability of diffusion models. Despite their success in many imaging inverse problems, most existing methods rely on privileged information such as derivative, pseudo-inverse, or full knowledge about the forward model. This reliance poses a substantial limitation that restricts their use in a wide range of problems where such information is unavailable, such as in many scientific applications. We propose Ensemble Kalman Diffusion Guidance (EnKG), a derivative-free approach that can solve inverse problems by only accessing forward model evaluations and a pre-trained diffusion model prior. We study the empirical effectiveness of EnKG across various inverse problems, including scientific settings such as inferring fluid flows and astronomical objects, which are highly non-linear inverse problems that often only permit black-box access to the forward model. We open-source our code at https://github.com/devzhk/enkg-pytorch.

Hongkai Zheng, Wenda Chu, Austin Wang, Nikola Kovachki, Ricardo Baptista, Yisong Yue• 2024

Related benchmarks

TaskDatasetResultRank
MRI ReconstructionfastMRI Brain (test)
SSIM0.953
18
Fluid Data Assimilationvorticity fields 128x128 (test)
Relative L2 Error0.32
12
Black Hole ImagingInverseBench Black-Hole Imaging (test)
PSNR26.21
9
Image InpaintingFFHQ 95% missing random mask 100 images (val)
PSNR22.64
9
Image DeblurringFFHQ Gaussian deblurring 100 images (val)
PSNR20.84
9
Image Super-resolutionFFHQ 4x super-resolution 100 images (val)
PSNR21.72
9
Navier–Stokes inverse problemInverseBench 128 x 128 (test)
NRMSE (σnoise=0)0.12
6
JPEG restorationFFHQ JPEG QF=5 100 images (val)
PSNR20.89
5
Black Hole ImagingBlack Hole Imaging 100% observation ratio
PSNR23.03
4
Black Hole ImagingBlack Hole Imaging 10% observation ratio
PSNR22.77
4
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