Numerical integration is the family of algorithms that approximate definite integrals and advance differential equations in time when closed-form solutions are unavailable. In physics simulation it denotes the time-stepping schemes (such as explicit and implicit Euler, Verlet, and Runge-Kutta methods) that integrate equations of motion to update positions and velocities each frame. The choice of scheme balances accuracy, numerical stability, and computational cost.

Overview

  • Numerical integration converts continuous differential equations into discrete update rules, allowing computers to evolve a system state forward in fixed or adaptive time steps.
  • In interactive simulation, explicit schemes are cheap but can become unstable at large time steps, whereas implicit schemes are more stable at greater cost.
  • The accuracy of a scheme is characterised by its order; higher-order methods reduce error per step but require more force evaluations.

Mechanisms

  • Explicit Euler: simplest first-order scheme, updating state directly from current derivatives.
  • Semi-implicit and Verlet integration: widely used in games for stable, energy-conserving particle and rigid-body updates.
  • Runge-Kutta family: higher-order multi-stage schemes offering improved accuracy for stiff or sensitive systems.
  • Adaptive step sizing: error estimation drives the step length to maintain a target tolerance.
  • Implicit solvers: solve a system each step for unconditional stability in stiff problems such as cloth and soft bodies.

Applications

  • Advancing equations of motion in real-time game and robotics physics engines.
  • Time integration within finite-element and continuum-mechanics solvers.
  • Trajectory and orbital propagation in scientific and engineering simulation.
  • Particle systems, fluids, and deformable bodies in spatial-computing experiences.

Provenance