The Revolutionary Insight

Traditional ML: Learn patterns from data alone

PINNs: Learn patterns from data AND physics simultaneously

Key Advantages of PINNs

  1. Regularization Effect: Physics constraints prevent overfitting
    • Standard NN can fit any function through the data points
    • PINN is constrained to solutions that satisfy the ODE
  2. Better Interpolation: Smooth, physically meaningful predictions between data points
    • Standard NN: arbitrary interpolation
    • PINN: physics-guided interpolation
  3. Accurate Derivatives: Natural consequence of physics enforcement
    • Automatic differentiation + physics loss = correct derivatives
    • Critical for applications requiring gradients (optimization, control)
  4. Data Efficiency: Less training data needed
    • Physics provides strong inductive bias
    • Can generalize from very sparse measurements

The Universal Approximation Foundation

Why this works theoretically:

  • Neural networks can approximate functions in Sobolev spaces \( H^k \)
  • Sobolev spaces include both functions AND their derivatives
  • With smooth activation functions (\( \tanh \), \( \sin \)), we can approximate solutions to differential equations
  • Automatic differentiation makes this practical

When to Use PINNs

Ideal scenarios:

  • ✅ Known governing equations (PDEs/ODEs)
  • ✅ Sparse, noisy data
  • ✅ Need physically consistent solutions
  • ✅ Require accurate derivatives
  • ✅ Complex geometries (where finite elements struggle)

Limitations:

  • ❌ Unknown physics
  • ❌ Highly nonlinear/chaotic systems
  • ❌ Large-scale problems (computational cost)
  • ❌ Discontinuous solutions

Extensions and Applications

This framework extends to:

  • Partial Differential Equations: Heat equation, wave equation, Navier-Stokes
  • Inverse Problems: Estimate unknown parameters from data
  • Multi-physics: Coupled systems (fluid-structure interaction)
  • High Dimensions: Curse of dimensionality breaking

The Bottom Line

PINNs = Universal Function Approximation + Physics Constraints + Automatic Differentiation

This combination creates a powerful method for solving differential equations with neural networks, particularly when data is sparse and physics is well-understood.

Next Steps: Try this approach on the 1D Poisson equation with hard constraints!

 
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CVW material development is supported by NSF OAC awards 1854828, 2321040, 2323116 (UT Austin) and 2005506 (Indiana University)