PlanetPhysics/Maxwells Equations

Maxwell's equations are a set of four partial differential equations first combined by James Clerk Maxwell. Together, they completely describe classical electromagnetic phenomena, just as Newton's laws completely describe classical mechanical phenomena. All four are named after persons other than Maxwell, but Maxwell was the first to add the displacement current term to Amp\`ere's Law, which led to the association of electromagnetic waves with light and paved the way for the discovery of special relativity. All four equations can be written in both integral and differential forms, with both forms convenient for specific problems. Note that strictly speaking these are Maxwell's equation in vacuo, with different forms for interaction with matter.

NotationEdit

Throughout this article SI units are adopted for clarity, but the interesting mathematical aspects of the equations are independent of the constants   and  , and indeed of the physical meaning of the equations.

 

 

Failed to parse (syntax error): {\displaystyle \mathbf{J} = \mbox{Current density, SI units Amp\`ere m}^{-3} }

 

 

Gauss' Law of ElectrostaticsEdit

Differential form

 

Integral form

 

where   is the charge enclosed in the volume bounded by the surface  .

Gauss' Law of MagnetostaticsEdit

 

 

This law can be interpreted as a statement of the non-existence of magnetic monopoles, a fact confirmed by all experiments to date.

Faraday's LawEdit

Differential form

 

Amp\`ere's LawEdit

Differential form

 

Integral form

Properties of Maxwell's EquationsEdit

These four equations together have several interesting properties:

  • Lorentz invariance
  • Gauge invariance
  • Invariance under the transformation Failed to parse (syntax error): {\displaystyle B \rightarrow \frac{E}} ,