English

Laplace priors and spatial inhomogeneity in Bayesian inverse problems

Statistics Theory 2022-10-27 v2 Statistics Theory

Abstract

Spatially inhomogeneous functions, which may be smooth in some regions and rough in other regions, are modelled naturally in a Bayesian manner using so-called Besov priors which are given by random wavelet expansions with Laplace-distributed coefficients. This paper studies theoretical guarantees for such prior measures - specifically, we examine their frequentist posterior contraction rates in the setting of non-linear inverse problems with Gaussian white noise. Our results are first derived under a general local Lipschitz assumption on the forward map. We then verify the assumption for two non-linear inverse problems arising from elliptic partial differential equations, the Darcy flow model from geophysics as well as a model for the Schr\"odinger equation appearing in tomography. In the course of the proofs, we also obtain novel concentration inequalities for penalized least squares estimators with 1\ell^1 wavelet penalty, which have a natural interpretation as maximum a posteriori (MAP) estimators. The true parameter is assumed to belong to some spatially inhomogeneous Besov class B11αB^{\alpha}_{11}, α>0\alpha>0. In a setting with direct observations, we complement these upper bounds with a lower bound on the rate of contraction for arbitrary Gaussian priors. An immediate consequence of our results is that while Laplace priors can achieve minimax-optimal rates over B11αB^{\alpha}_{11}-classes, Gaussian priors are limited to a (by a polynomial factor) slower contraction rate. This gives information-theoretical justification for the intuition that Laplace priors are more compatible with 1\ell^1 regularity structure in the underlying parameter.

Keywords

Cite

@article{arxiv.2112.05679,
  title  = {Laplace priors and spatial inhomogeneity in Bayesian inverse problems},
  author = {Sergios Agapiou and Sven Wang},
  journal= {arXiv preprint arXiv:2112.05679},
  year   = {2022}
}
R2 v1 2026-06-24T08:12:37.294Z