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Learning Smooth and Expressive Interatomic Potentials for Physical Property Prediction

ICML 2025 · Probabilistic and scientific modeling › Molecules and proteins · approach: Machine-learned interatomic potentials · 33 citations (OpenAlex)

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Proposes testing MLIPs by energy conservation in NVE molecular dynamics and introduces eSEN, a smooth, conservative equivariant interatomic potential that achieves state-of-the-art Matbench-Discovery, thermal conductivity, and MDR phonon results.

Problem

Lower test-set errors for machine learning interatomic potentials (MLIPs) do not reliably translate into accuracy on downstream physical property prediction tasks such as relaxation, MD, and phonon/thermal conductivity calculations.

Approach

Use energy conservation in NVE MD simulations (with bounded, smooth energy derivatives) as a practical test of whether an MLIP is suitable for property prediction; design eSEN with conservative forces, no discretized nonlinearities (gated SiLU in spherical-harmonic space), no neighbor limit, and envelope functions so that test error correlates better with property accuracy.

Key results

Measured effects reported in the paper

What was changedWhereMeasuredEffect
Use conservative forces instead of direct-force prediction (ablation)eSEN · SPICE-MACE-OFFEnergy MAE: 0.56 -> 0.23Helped
Use conservative forces instead of direct-force prediction (ablation)eSEN · SPICE-MACE-OFFForce MAE: 10.98 -> 6.36Helped
Remove the maximum-neighbor limit (ablation)eSEN · TM23 energy-conservation simulationsenergy conservationHelped
Add an envelope function (ablation)eSEN · TM23 and MD22 energy-conservation simulationsenergy conservationHelped
Use continuous spherical-harmonic processing instead of discrete-grid representation (ablation)eSEN · TM23 and MD22 energy-conservation simulationsenergy conservationHelped
Increase radial basis functions to 512 (ablation)eSEN · TM23 energy-conservation simulationsenergy conservationHurt
Increase radial basis functions to 512 (ablation)eSEN · MD22 energy-conservation simulationsenergy conservationNo clear effect
Replace the default Gaussian radial basis with a Bessel radial basis (ablation)eSEN · TM23 and MD22 energy-conservation simulationsenergy conservationNo clear effect
Pre-train with direct-force prediction, then fine-tune conservatively (ablation)eSEN · MPTrj validationvalidation lossHelped
Pre-train with direct-force prediction, then fine-tune conservatively (ablation)eSEN · MPTrj trainingwallclock training time: 40%Helped
Increase radial basis functions to 512 (ablation)eSEN · SPICE-MACE-OFFEnergy MAE: 0.23 -> 0.19Helped
Increase radial basis functions to 512 (ablation)eSEN · MPTrjEnergy MAE: 17.02 -> 19.87Hurt

Surprising findings

Limitations

Experimental setup

Datasets: MPTrj SPICE-MACE-OFF OMat24 sAlex TM23 MD22 MDR Phonon benchmark SPICE

Benchmarks: Matbench-Discovery MDR Phonon benchmark SPICE-MACE-OFF test set TM23 energy conservation MD22 energy conservation

Metrics: F1 kappa_SRME RMSD MAE energy drift DAF

Baselines: EquiformerV2 / eqV2-S-DeNS MACE-MP-0 CHGNet M3GNet SevenNet-l3i5 GRACE-2L ORB v2 MACE-OFF-L EScAIP-45M eqV2-M-OAM

Builds on: eSCN Equiformer DimeNet DeNS MPTrj

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