Cosmological Analysis with Calibrated Neural Quantile Estimation and Approximate Simulators
He Jia

TL;DR
The paper introduces a calibrated Neural Quantile Estimation method for efficient cosmological parameter inference, combining approximate and high-fidelity simulations to produce unbiased posteriors with reduced computational cost.
Contribution
It presents a novel SBI approach that guarantees unbiased posteriors using calibration with few high-fidelity simulations, improving efficiency in cosmological analyses.
Findings
Calibrated NQE achieves near-optimal constraints with fewer high-fidelity simulations.
Method accurately infers cosmological parameters from 2D dark matter maps.
Posteriors closely match those from expensive simulations at a fraction of the cost.
Abstract
A major challenge in extracting information from current and upcoming surveys of cosmological Large-Scale Structure (LSS) is the limited availability of computationally expensive high-fidelity simulations. We introduce calibrated Neural Quantile Estimation (NQE), a new Simulation-Based Inference (SBI) method that leverages a large number of approximate simulations for training and a small number of high-fidelity simulations for calibration. This approach guarantees an unbiased posterior regardless of approximate simulation accuracy, while achieving near-optimal constraining power when the approximate simulations are reasonably accurate. As a proof of concept, we demonstrate that cosmological parameters can be inferred at field level from projected 2-dim dark matter density maps up to /Mpc at by training on Particle-Mesh (PM) simulations with…
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