BPINNs

Model Overview

BPINNs (Bayesian Physics-Informed Neural Networks) incorporate physical-equation constraints into Bayesian neural networks to jointly estimate equation solutions and predictive uncertainty from noisy data. This model package provides an example for solving a one-dimensional Laplace equation:

u_xx + pi^2 sin(pi x) = 0,  x in [0, 1]
u(x) = sin(pi x)

Paper: B-PINNs: Bayesian physics-informed neural networks for forward and inverse PDE problems with noisy data
https://doi.org/10.1016/j.jcp.2020.109913

Model Description

BPINNs are trained jointly on observational data, boundary conditions, and PDE residuals. By default, the model is optimized with Adam and then refined with L-BFGS. During inference, predictive means and standard deviations can be computed from multiple parameter states stored in a checkpoint. The default training workflow produces only one optimized state; full Bayesian uncertainty quantification requires posterior parameter states obtained through Hamiltonian Monte Carlo (HMC), variational inference, or ensemble sampling.

Use Cases

Use Case Description
One-dimensional Laplace equation Train the solution jointly from observation points, boundary points, and collocation points
PDE modeling with noisy data Fit noisy observations subject to physical constraints
Optimizer comparison Compare the effects of Adam and L-BFGS on PINN convergence
Posterior prediction Compute predictive means and standard deviations from multiple parameter states

Usage

1. OneCode

Use the online OneCode environment for an intelligent, one-click AI for Science (AI4S) programming experience:

Launch OneCode for one-click AI4S programming

2. Manual Setup

Hardware Requirements

  • A GPU or DCU can accelerate full training; a CPU is sufficient for pipeline validation.
  • DCU users must install DTK and a PyTorch environment compatible with the target cluster.

Download the Model Package

modelscope download --model OneScience/BPINNs --local_dir ./BPINNs
cd BPINNs

Set Up the Runtime Environment

DCU Environment

# Activate DTK and Conda first
conda create -n onescience311 python=3.11 -y
conda activate onescience311
pip install onescience[cfd-dcu] -i http://mirrors.onescience.ai:3141/pypi/simple/ --trusted-host mirrors.onescience.ai

GPU Environment

# Activate Conda first
conda create -n onescience311 python=3.11 -y libstdcxx-ng=12 libgcc-ng=12 gcc_linux-64=12 gxx_linux-64=12
conda activate onescience311
pip install onescience[cfd-gpu] -i http://mirrors.onescience.ai:3141/pypi/simple/ --trusted-host mirrors.onescience.ai

Training Data

This example automatically generates interior observation points, boundary points, PDE collocation points, and a test grid from the analytical solution; no external data files are required. The number of observation and collocation points, noise level, and computational domain can be configured in conf/config.yaml.

Training

python scripts/train.py

By default, training produces the base weights at weight/bpinn_laplace1d.pt and saves the training history to result/training_history.npz.

Model Weights

This repository provides weights trained on the one-dimensional Laplace equation in the weight/ directory.

L-BFGS Refinement

python scripts/refine.py

By default, refinement produces weight/bpinn_laplace1d_refined.pt.

Inference, Evaluation, and Visualization

python scripts/inference.py

Inference loads the refined weights when available and otherwise falls back to the base weights. Predictions and visualizations are saved to result/. Model, training, loss, and inference parameters can all be modified in conf/config.yaml.

Official OneScience Resources

Citations and License

  • Yang, L., Meng, X., and Karniadakis, G. E. B-PINNs: Bayesian physics-informed neural networks for forward and inverse PDE problems with noisy data. Journal of Computational Physics, 425, 109913, 2021.
  • This model package is released under the Apache-2.0 license and retains attribution to the original paper.
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