| Astrophysics (Index) | About |
Maxwell's equations are four equations that James Clerk Maxwell gathered and refined or created himself that describe the behavior and interaction of electricity and magnetism. This behavior includes the conditions for propagating waves, i.e., electromagnetic waves, explaining electromagnetic radiation, including visible light. The equations are (in their CGS differential-equation form):
| Gauss's law | ∇ · E = 4πρ | Electric field lines begin and end at charged particles. |
| Gauss's law for magnetism | ∇ · B = 0 | Magnetic field lines don't end: they form circuits. If magnetic monopoles existed, a non-zero value could be on the right side of this equation. |
| Maxwell-Faraday equation | ∇ × E = - (1/c) ∂B/∂t | The magnetic field is shifting when/where the electric field curls around. |
| Ampere's law | ∇ × B = (1/c)(4πJ + ∂E/∂t) | When/where the magnetic field curls around, you get electric current, or a shift in the electric field, or some of each. |
(SI units treat electromagnetism somewhat differently, incorporating another factor which includes some of the constants.)