CosmicRIM : Reconstructing Early Universe by Combining Differentiable Simulations with Recurrent Inference Machines
Chirag Modi, Fran\c{c}ois Lanusse, Uro\v{s} Seljak, David N. Spergel,, Laurence Perreault-Levasseur

TL;DR
This paper introduces CosmicRIM, a novel approach combining differentiable N-body simulations with recurrent inference machines to efficiently reconstruct the Universe's initial conditions from cosmological data, outperforming traditional methods in speed and quality.
Contribution
The paper presents a new differentiable simulation-based inference framework using recurrent networks for faster and higher-quality reconstruction of early Universe conditions.
Findings
Recurrent inference machines achieve 40x faster inference than traditional algorithms.
The method produces higher quality initial condition estimates.
Demonstrated effectiveness on realistic cosmological observables.
Abstract
Reconstructing the Gaussian initial conditions at the beginning of the Universe from the survey data in a forward modeling framework is a major challenge in cosmology. This requires solving a high dimensional inverse problem with an expensive, non-linear forward model: a cosmological N-body simulation. While intractable until recently, we propose to solve this inference problem using an automatically differentiable N-body solver, combined with a recurrent networks to learn the inference scheme and obtain the maximum-a-posteriori (MAP) estimate of the initial conditions of the Universe. We demonstrate using realistic cosmological observables that learnt inference is 40 times faster than traditional algorithms such as ADAM and LBFGS, which require specialized annealing schemes, and obtains solution of higher quality.
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Taxonomy
TopicsComputational Physics and Python Applications · Galaxies: Formation, Evolution, Phenomena · Gaussian Processes and Bayesian Inference
