A graphical multi-fidelity Gaussian process model, with application to emulation of heavy-ion collisions

TL;DR

This paper introduces a Graphical Multi-fidelity Gaussian Process model that leverages scientific dependency graphs for efficient emulation of complex simulations, demonstrated on heavy-ion collision data.

Contribution

The paper proposes a novel GMGP model embedding DAG structures into Gaussian processes, with scalable algorithms and a new experimental design methodology for multi-fidelity data.

Findings

Demonstrates the GMGP's effectiveness through numerical experiments.

Shows the model's applicability to emulating heavy-ion collisions.

Provides a scalable recursive computation algorithm for the model.

Abstract

With advances in scientific computing and mathematical modeling, complex scientific phenomena such as galaxy formations and rocket propulsion can now be reliably simulated. Such simulations can however be very time-intensive, requiring millions of CPU hours to perform. One solution is multi-fidelity emulation, which uses data of different fidelities to train an efficient predictive model which emulates the expensive simulator. For complex scientific problems and with careful elicitation from scientists, such multi-fidelity data may often be linked by a directed acyclic graph (DAG) representing its scientific model dependencies. We thus propose a new Graphical Multi-fidelity Gaussian Process (GMGP) model, which embeds this DAG structure (capturing scientific dependencies) within a Gaussian process framework. We show that the GMGP has desirable modeling traits via two Markov properties, and admits a scalable algorithm for recursive computation of the posterior mean and variance along at each depth level of the DAG. We also present a novel experimental design methodology over the DAG given an experimental budget, and propose a nonlinear extension of the GMGP via deep Gaussian processes. The advantages of the GMGP are then demonstrated via a suite of numerical experiments and an application to emulation of heavy-ion collisions, which can be used to study the conditions of matter in the Universe shortly after the Big Bang. The proposed model has broader uses in data fusion applications with graphical structure, which we further discuss.