Bayesian Deep Gaussian Processes for Correlated Functional Data: A Case Study in Cosmological Matter Power Spectra
Stephen A. Walsh, Annie S. Booth, David Higdon, Jared Clark, Kelly R. Moran, Katrin Heitmann

TL;DR
This paper introduces a Bayesian deep Gaussian process model to estimate and predict correlated functional matter power spectra in cosmology, providing uncertainty quantification and improved predictions for unobserved cosmologies.
Contribution
It extends Bayesian DGPs to handle correlated functional outputs and integrates this with a Gaussian process emulator for cosmological predictions.
Findings
Model performs well on synthetic data
Outperforms benchmark cosmological emulator
Provides effective uncertainty quantification
Abstract
Understanding the structure of our universe and the distribution of matter is an area of active research. As cosmological surveys grow in complexity, the development of emulators to efficiently and effectively predict matter power spectra is essential. We are particularly motivated by the Mira-Titan Universe simulation suite that, for a specified cosmological parameterization (termed a "cosmology"), provides multiple response curves of various fidelities, including correlated functional realizations. Our objective is two-fold. First, we estimate the underlying true matter power spectra, with appropriate uncertainty quantification (UQ), from all of the provided curves. To this end, we propose a novel Bayesian deep Gaussian process (DGP) hierarchical model which synthesizes all the simulation information to estimate the underlying matter power spectra while providing effective UQ. Our…
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Taxonomy
TopicsGaussian Processes and Bayesian Inference · Galaxies: Formation, Evolution, Phenomena · Advanced Bandit Algorithms Research
