Physics · Glossary

What is Magnetisation, bound currents, and H?

Definition 22.6 University Physics — Year 3 · Chapter 22 — Electromagnetism in Matter

The magnetic story runs in parallel. Matter is full of microscopic current loops — orbiting and spinning electrons, each a magnetic dipole μ\vect\mu; their density is the magnetisation M=nμ\vect M = n\langle\vect\mu\rangle. A uniformly magnetised block is equivalent to a bound surface current circulating around its sides (interior loops cancel pairwise; a bar magnet is a solenoid of bound current). Splitting currents into free and bound, Ampère’s law rearranges around the auxiliary field

H=Bμ0M,H ⁣d=Ifree:\vect H = \frac{\vect B}{\mu_0} - \vect M , \qquad \oint \vect H\cdot\dd\vect\ell = I_{\text{free}} :

H\vect H is sourced by the currents in our wires (units A/m\mathrm{A}/\mathrm{m}), while B\vect B keeps the physics — forces, flux, induction. Linear media have M=χmH\vect M = \chi_{\text{m}}\vect H and B=μ0(1+χm)H=μ0μrH\vect B = \mu_0(1 + \chi_{\text{m}})\vect H = \mu_0\mu_{\text{r}}\vect H.

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