Spatio-temporal, multi-field deep learning of shock propagation in meso-structured media
M. Giselle Fernández-Godino, Meir H. Shachar, Kevin Korner, Jonathan L. Belof, Mukul Kumar, Jonathan Lind, William J. Schill
TL;DR
This work tackles predicting multi-field shock dynamics in meso-structured media, where pore collapse and complex interfacial phenomena challenge traditional surrogates. The authors introduce MSTM, a hybrid CNN–LSTM autoregressive model that evolves seven coupled fields $(\rho, p, T, E, m, u_x, u_y)$ on a $60\times60$ grid using five-frame inputs to predict the next frame, trained on high-fidelity MARBL hydrocode data. Across porous and lattice configurations, MSTM achieves mean errors of $1.4\%$ and $3.2\%$ respectively and delivers greater than $10^3\times$ speedups, while reducing MSE and SSIM dissimilarity by about $94\%$ relative to seven single-field surrogates; the model generalizes across porosity, lattice angle, and loading, and maintains mass-averaged QoIs within ~5\%. These results establish MSTM as a practical, high-fidelity, multi-field surrogate that enables design optimization and uncertainty quantification for meso-structured materials in planetary defense and inertial fusion energy contexts.
Abstract
The ability to predict how shock waves traverse porous and architected materials is a key challenge in planetary defense and in the pursuit of inertial fusion energy. Yet capturing pore collapse, anomalous Hugoniot responses, and localized heating - phenomena that strongly influence asteroid deflection or fusion ignition - has remained a major challenge despite recent advances in single-field and reduced representations. We introduce a multi-field spatio-temporal model (MSTM) that unifies seven coupled fields - pressure, density, temperature, energy, material distribution, and two velocity components - into a single autoregressive surrogate. Trained on high-fidelity hydrocode data, MSTM captures nonlinear shock-driven dynamics across porous and architected configurations, achieving mean errors of 1.4% and 3.2% respectively, all while delivering over three orders of magnitude in speedup. MSTM reduces mean-squared error and structural dissimilarity by 94% relative torelative to single-field spatio-temporal models. This advance transforms problems once considered intractable into tractable design studies, establishing a practical framework for optimizing meso-structured materials in planetary impact mitigation and inertial fusion energy.
