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Neural Importance Sampling

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arxiv 1808.03856 v5 pith:Y3DG5IJX submitted 2018-08-11 cs.LG cs.GRstat.ML

classification cs.LGcs.GRstat.ML
keywords integrationdensitiesneuralsampleapplicationapplicationsapproachcarlo
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abstract

We propose to use deep neural networks for generating samples in Monte Carlo integration. Our work is based on non-linear independent components estimation (NICE), which we extend in numerous ways to improve performance and enable its application to integration problems. First, we introduce piecewise-polynomial coupling transforms that greatly increase the modeling power of individual coupling layers. Second, we propose to preprocess the inputs of neural networks using one-blob encoding, which stimulates localization of computation and improves inference. Third, we derive a gradient-descent-based optimization for the KL and the $\chi^2$ divergence for the specific application of Monte Carlo integration with unnormalized stochastic estimates of the target distribution. Our approach enables fast and accurate inference and efficient sample generation independently of the dimensionality of the integration domain. We show its benefits on generating natural images and in two applications to light-transport simulation: first, we demonstrate learning of joint path-sampling densities in the primary sample space and importance sampling of multi-dimensional path prefixes thereof. Second, we use our technique to extract conditional directional densities driven by the product of incident illumination and the BSDF in the rendering equation, and we leverage the densities for path guiding. In all applications, our approach yields on-par or higher performance than competing techniques at equal sample count.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Flow-Based Surrogates for High-Dimensional Likelihoods in Experimental Neutrino Physics

    hep-ex 2026-07 accept novelty 6.0 of 10

    A hybrid coupling-plus-autoregressive normalizing flow trained on a 110-parameter T2K-like near-detector likelihood reaches 98% relative ESS versus 5% for the post-fit Gaussian and matches MCMC flux predictions.

  2. Denoising Milky Way stellar survey data with normalizing flow models

    astro-ph.GA 2025-05 conditional novelty 5.0 of 10

    A normalizing flow with importance-sampling denoising partially recovers kinematic substructures (Hercules stream, phase spiral) from mock Gaia data with amplified errors.

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