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Evidence Networks: simple losses for fast, amortized, neural Bayesian model comparison

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arxiv 2305.11241 v2 pith:MJUQJJ7J submitted 2023-05-18 cs.LG astro-ph.COastro-ph.IMstat.ML

classification cs.LGastro-ph.COastro-ph.IMstat.ML
keywords evidencemodelnetworksbayesiancomparisonbayesdataneural
verification ladder T0 review T1 audit T2 compute T3 formal
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Evidence Networks can enable Bayesian model comparison when state-of-the-art methods (e.g. nested sampling) fail and even when likelihoods or priors are intractable or unknown. Bayesian model comparison, i.e. the computation of Bayes factors or evidence ratios, can be cast as an optimization problem. Though the Bayesian interpretation of optimal classification is well-known, here we change perspective and present classes of loss functions that result in fast, amortized neural estimators that directly estimate convenient functions of the Bayes factor. This mitigates numerical inaccuracies associated with estimating individual model probabilities. We introduce the leaky parity-odd power (l-POP) transform, leading to the novel ``l-POP-Exponential'' loss function. We explore neural density estimation for data probability in different models, showing it to be less accurate and scalable than Evidence Networks. Multiple real-world and synthetic examples illustrate that Evidence Networks are explicitly independent of dimensionality of the parameter space and scale mildly with the complexity of the posterior probability density function. This simple yet powerful approach has broad implications for model inference tasks. As an application of Evidence Networks to real-world data we compute the Bayes factor for two models with gravitational lensing data of the Dark Energy Survey. We briefly discuss applications of our methods to other, related problems of model comparison and evaluation in implicit inference settings.

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Cited by 3 Pith papers

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  1. Microlensing Detection and Inference via Learned Bayes Factors

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    A unified transformer-based pipeline detects 99.9% of recoverable simulated microlensing events and outperforms literature hard cuts in the short-duration finite-source regime with amortized neural posterior inference.

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    A Hamiltonian, energy-conserving optimizer (ECDq=1) reduces initialization dependence and mean error compared to Adam for neural likelihood-ratio estimation in two collider-physics benchmarks.

  3. Machine Learning and the SKA for Cosmic Dawn and the Epoch of Reionization

    astro-ph.IM 2026-07 accept novelty 2.5 of 10

    A multi-author overview of machine-learning algorithms proposed for instrument modelling, data analysis, simulation and inference in SKA Cosmic Dawn and Epoch of Reionization science.

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