Maxwell's Equations
Four equations hold all of electromagnetism. Electric field lines start and end on charges, magnetic field lines never end, a changing magnetic field swirls the electric field, and currents and changing electric fields swirl the magnetic field. Each one is a statement about flux or circulation over a whole surface or loop (the integral form), or, shrunk down to a single point, about divergence or curl (the differential form).
What the symbols mean
- Enclosed charge
The total charge inside the closed surface S.
- Charge density
Charge per unit volume at a point, in C/m³.
- Divergence of E
How much E spreads out from a point: the outward flux of a tiny box, per unit volume.
What the symbols mean
- Divergence of B
Zero everywhere: no point is a source or a sink of magnetic field.
What the symbols mean
- Magnetic flux
The flux of B through a surface whose edge is the loop C.
- Curl of E
How much E circulates around a point, per unit area.
What the symbols mean
- Enclosed current
Conduction current through a surface whose edge is C.
- Electric flux
Its rate of change, times ε₀, is the displacement current.
- Current density
Current per unit area at a point, in A/m².
What the symbols mean
- Charge
The charge of the particle the fields act on.
- Velocity
The particle's velocity.
Explanation
Maxwell's equations are simply four rules that describe everything electric and magnetic: where electric fields come from, why magnetic field lines never end, and how a changing field of one kind makes a field of the other kind. They're named after James Clerk Maxwell, who pulled these laws together in the 1860s and added the missing displacement current (the tidy four-equation form came a bit later, from Oliver Heaviside). Every antenna, motor, transformer and fiber-optic cable is designed from them. The symbols are just a few pieces: (divergence, how much a field spreads out from a point), (curl, how much it swirls around a point), (how fast something changes in time) and and (the charges and currents). Four lines full of upside-down triangles look like the hardest thing in the course, but each one is a sentence you've already met in an earlier unit. Bear with it.
One page of physics. Everything in this course so far, from Coulomb's law to LC circuits, follows from four equations about two fields, plus the Lorentz force that says how those fields push on charges. It helps to read them as two pairs.
The divergence pair: where field lines begin.
- Gauss's law. The flux of out of any closed surface counts the charge inside. Electric field lines start on positive charge and end on negative charge (Gauss's law).
- Gauss's law for magnetism. The flux of out of any closed surface is zero. There are no magnetic charges, so magnetic field lines never start or stop: they close on themselves. Cut a bar magnet in half and you get two shorter magnets, never a lone north pole.
The curl pair: what makes fields circulate.
- Faraday's law. A changing magnetic flux drives a circulating , the EMF in every generator and transformer (Faraday's law). The minus sign is Lenz's law.
- Ampère–Maxwell law. Currents and changing electric flux drive a circulating (Ampère's law plus the displacement current).
Integral form ⟺ differential form. The integral forms talk about whole surfaces and loops; the differential forms talk about single points. The divergence theorem converts one into the other. For any small volume with surface ,
Gauss's law says the left sides are equal for every volume, so the integrands must match point by point: . (If they differed at some point, a tiny volume around it would break the law.) Stokes' theorem does the same for the loop laws. For Faraday's law on a fixed surface with edge ,
and the left sides are equal for every surface, so . Use the integral form when symmetry lets you pull or out of the integral (spheres, cylinders, circles), and the differential form to check a proposed field or to find the charges and currents that made it.
Charge conservation is built in. Take the divergence of the Ampère–Maxwell law. The divergence of a curl is zero and , so
Charge can't appear or vanish, only flow. Notice that this only worked because of Maxwell's term. Without it, the equations would contradict charge conservation, which was exactly the puzzle in the last lesson.
The static special cases. When nothing changes, Faraday's law says , so is a gradient (field from potential), and Gauss's law becomes Poisson's equation (Poisson's and Laplace's equations). Electrostatics and magnetostatics are what's left when the time derivatives vanish. The time derivatives are what couple and into one electromagnetic field.
Empty space. With and the equations are nearly symmetric:
A changing makes and a changing makes . So what happens if each keeps making the other? The next lesson shows they can keep each other going forever, and that's light.
A common mistake. After a whole course of electrostatics, it's tempting to assume always, so that every is the gradient of some potential. That's only true when is steady. Around a transformer, circulates and isn't the gradient of any potential. Two smaller slips: reading as "" (it only rules out sources and sinks), and mismatching orientations. The loop's direction and the surface's normal must follow the right-hand rule, or Faraday's minus sign flips.
See it
Worked examples
The field inside a long solenoid of radius cm points along and grows at T/s. (a) Use Faraday's law in integral form to find the induced electric field cm and cm from the axis. (b) Check the differential form.
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By symmetry, circles the axis with the same strength all the way around a circle of radius , so .
In a region of space the fields are steady: and , with and in meters. What charge density and current density produce them?
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Gauss's law: V/m², so C/m³, the same everywhere.
Practice
Type your answer and check it. Solve them all to complete the lesson.
Which of Maxwell's equations rules out magnetic charges, so that magnetic field lines never begin or end?
For what value of is a possible magnetic field? ( and are constants.)
A region holds the electric field , with and in meters. Use Faraday's law to find , in T/s.
In a region of space, V/m, with , and in meters. Find the charge density at the point m, in nC/m³, to 3 significant figures.
A magnetic stimulation coil held against the head makes a field that rises steadily from to T in s. Model the field as uniform over a circle of radius cm and zero outside it. What electric field does it induce cm from the axis, in V/m?
A circular loop of radius cm lies in the -plane in a uniform field that changes at T/s. Find around the loop, counterclockwise as seen from above (), in mV.
In a region where nothing changes with time, which equation guarantees that the electric field can be written as ?
In part of a device, the current density is , with in meters. At cm, how fast is the charge density changing, in C/(m³·s)? (Use the continuity equation that Maxwell's equations imply.)
The hardest one here. Get it, and you've got this lesson.
An electron beam of radius mm carries a current of mA, its electrons moving at m/s. Treat it as a long, uniform cylinder of charge. (a) Use Gauss's law to find the electric field at the beam's edge. (b) Use Ampère's law to find the magnetic field there. (c) An electron at the edge feels an outward electric push and an inward magnetic pull. What percentage of the push does the pull cancel? Enter (V/m), (nT) and the percentage, to 3 significant figures.
Where it's used
Maxwell's equations are what electromagnetic simulation software solves. Engineers designing antennas, phone circuit boards, MRI coils, microwave ovens and radar discretize the differential forms on a grid (finite-difference time-domain and finite-element codes) and step them forward in time. The integral forms are the quick hand checks: Gauss's law for the field near a charged conductor, Ampère's law for the field around a busbar, Faraday's law for the voltage a transformer winding picks up.