The wave equation, given by $\partial_t^2 u-c^2 \nabla^2 u=f$, is a crucial partial differential equation in physics defined by its second-order time derivative, which enables the description of propagating waves unlike the diffusion equation. Its application depends on the physical context: for transversal waves on a string or a membrane, the equation arises from applying Newton's second law under a small deviation approximation ( $|\nabla u| \ll 1$ ), with the wave speed squared determined by the ratio of tension to density ( $c^2=S / \rho_{\ell}$ or $c^2=\sigma / \rho_A$ ). In contrast, for electromagnetic fields, the wave equation for the magnetic field $B$ is a direct and exact consequence of Maxwell's equations, where the wave speed is precisely the speed of light, $c=1 / \sqrt{\varepsilon_0 \mu_0}$.
General Form and Distinction
The general, sourced wave equation is:
$$ \partial_t^2 u-c^2 \nabla^2 u=f $$
Defining Feature: The appearance of the second-order time derivative $\left(\partial_t^2 u\right)$ fundamentally distinguishes it from the diffusion equation, leading to propagating wave solutions.
Parameters: $c$ is the wave velocity, and $f$ is the source term.
Derivations and Wave Speed (c)
The text provides derivations for three key physical scenarios, showing how the wave speed $c$ is determined by the system's material properties.
| Scenario | Nature of Derivation | Resulting PDE Term | Wave Speed Squared ( $c^2$ ) | Key Dependencies |
|---|---|---|---|---|
| Transversal String (1D) | Approximative (Small Deviation) | $\begin{aligned}& \partial_t^2 u- \\& \frac{S}{\rho_t} \partial_x^2 u\end{aligned}$ | $c^2=\frac{S}{\rho_{\ell}}$ | $c \propto \sqrt{\text { Tension/Linear Density }}$ |
| Transversal Membrane (2D) | Approximative (Small Deviation) | $\begin{aligned}& \partial_t^2 u- \\& \frac{\sigma}{\rho_A} \nabla^2 u\end{aligned}$ | $c^2=\frac{\sigma}{\rho_A}$ | $c \propto$$\sqrt{\text { Surface Tension/Surface Density }}$ |
| Electromagnetic Field (B) (3D) | Exact (Maxwell's Equations) | $\begin{aligned}& \partial_t^2 B- \\& c^2 \nabla^2 B\end{aligned}$ | $\begin{aligned}& c^2= \\& \frac{1}{\varepsilon_0 \mu_0}\end{aligned}$ | $c$ is the Speed of Light (constant) |
Role of Approximations
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