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Magnetism and Matter — Notes

6 sections 5 min readBeta

1. The bar magnet and its field lines

  • A freely suspended bar magnet points roughly north–south; its ends are the N and S poles. Like poles repel, unlike attract.
  • Poles always occur in pairs: breaking a magnet gives two complete magnets. No magnetic monopoles have been found.
  • Field lines are continuous closed loops: outside N → S, inside S → N. They never cross; crowding shows strength; the tangent gives the direction of B⃗\vec B.
  • Because lines never start or end, the net magnetic flux through any closed surface is zero.
  • Electric field lines of a dipole start on + and end on −; magnetic lines have no ends.
Traced numerically from the equivalent solenoid (Biot–Savart over its circular turns).

Key terms

Magnetic field line

A closed curve whose tangent gives the direction of the magnetic field.

Magnetic monopole

An isolated N or S pole; none has been observed.

2. The bar magnet as an equivalent solenoid

A current-carrying solenoid produces the same field pattern as a bar magnet (qualitative treatment). Its magnetic moment is m=NIAm = NIA, directed along the axis towards the end where the current appears anticlockwise (the N end).

Inside a magnet, the orbital and spin motion of electrons in its atoms act like tiny aligned current loops; their moments add up to the magnet’s moment m⃗\vec m (from S to N, unit A m²).

Cutting a solenoid in half gives two shorter solenoids, each with N and S ends — the same as breaking a magnet.

Same calculation as the bar-magnet figure, with the turns drawn.

Formulas

  • Equivalent solenoid
    m=NIAm = NIA

Key terms

Magnetic moment

Vector m (A m²) describing the strength and direction of a magnetic dipole; NIA for a coil.

3. Magnetic dipole: field and torque (qualitative)

Field (far away, by analogy with the electric dipole):

  • axial point: along m⃗\vec m, ∝2mr3\propto \dfrac{2m}{r^3};
  • equatorial point: opposite to m⃗\vec m, ∝mr3\propto \dfrac{m}{r^3} — half the axial value at the same rr.

In a uniform field: net force zero; torque τ⃗=m⃗×B⃗\vec\tau = \vec m \times \vec B (τ=mBsin⁡θ\tau = mB\sin\theta) turns the magnet into line with B⃗\vec B. Stable equilibrium when m⃗∥B⃗\vec m \parallel \vec B (energy −mB-mB), unstable when antiparallel (+mB+mB). A slightly displaced magnet oscillates about the field direction — the basis of the compass needle.

Electric dipoleMagnetic dipole
Momentp⃗\vec p (C m)m⃗\vec m (A m²)
Torquep⃗×E⃗\vec p \times \vec Em⃗×B⃗\vec m \times \vec B
Far field∝p/r3\propto p/r^3∝m/r3\propto m/r^3

Formulas

  • Torque on a magnet
    τ⃗=m⃗×B⃗\vec\tau = \vec m \times \vec B

Key terms

Stable equilibrium (dipole)

Moment along the field: a small turn produces a restoring torque.

4. Magnetisation and the magnetic quantities

  • Magnetisation MM: net magnetic moment per unit volume, A m−1^{-1}.
  • Magnetic intensity HH: set by free currents (e.g. H=nIH = nI in a solenoid), A m−1^{-1}.
  • B⃗=μ0(H⃗+M⃗)\vec B = \mu_0(\vec H + \vec M); for linear materials M⃗=χH⃗\vec M = \chi\vec H, so B⃗=μ0μrH⃗\vec B = \mu_0\mu_r\vec H with μr=1+χ\mu_r = 1 + \chi and permeability μ=μ0μr\mu = \mu_0\mu_r.
  • χ\chi and μr\mu_r have no units.

Worked result: an iron core with μr=500\mu_r = 500 in a solenoid with H=2000H = 2000 A m−1^{-1} gives B≈1.26B \approx 1.26 T and M≈1.0×106M \approx 1.0 \times 10^{6} A m−1^{-1}.

Formulas

  • Magnetic quantities
    B⃗=μ0(H⃗+M⃗),M⃗=χH⃗,μr=1+χ\vec B = \mu_0(\vec H + \vec M),\qquad \vec M = \chi\vec H,\qquad \mu_r = 1 + \chi

Key terms

Magnetisation

Net magnetic moment per unit volume of a material.

Susceptibility

χ = M/H; measures how readily a material is magnetised.

Relative permeability

μr = 1 + χ = B/(μ₀H).

5. Dia-, para- and ferromagnetism

DiamagneticParamagneticFerromagnetic
χsmall, negative (≈ −10⁻⁵)small, positive (10⁻⁵–10⁻³)very large (10²–10⁵)
μrslightly < 1slightly > 1≫ 1
Atomic momentsnone (induced, opposing)permanent, randomly orientedpermanent, aligned in domains
In a non-uniform fieldmoves to weaker fieldmoves to stronger fieldstrongly attracted
Rod between polessets across the fieldsets along the fieldsets along the field
ExamplesBi, Cu, Pb, water, N₂, NaClAl, Na, Ca, O₂, CuCl₂Fe, Co, Ni, Gd, alnico
  • Superconductors are perfect diamagnets (χ=−1\chi = -1, Meissner effect).
  • Domains: regions in which atomic moments are spontaneously aligned. In a field, favourably aligned domains grow and others rotate.
  • Soft ferromagnets (soft iron) magnetise and demagnetise easily — electromagnet and transformer cores. Hard ferromagnets (steel, alnico) retain magnetisation — permanent magnets.
Exact field of a long cylinder of relative permeability 0.6, 1.5 and 30 in a uniform field.

Key terms

Domain

A small region of a ferromagnet in which all atomic moments are aligned.

Meissner effect

Complete expulsion of a magnetic field from a superconductor.

6. Effect of temperature

  • Diamagnetism: nearly independent of temperature.
  • Paramagnetism: Curie law χ=CT\chi = \dfrac{C}{T} (TT in kelvin): thermal agitation opposes alignment, so χ falls as T rises; χT\chi T is constant.
  • Ferromagnetism: above the Curie temperature TCT_C the domain alignment is destroyed and the material becomes paramagnetic (Fe ≈ 1043 K, Ni ≈ 631 K, Co ≈ 1394 K). A heated magnet loses its magnetism.
  • paramagnet: χ = C/T (Curie law)
Curie law: χ ∝ 1/T.
  • ferromagnetic below TC
  • paramagnetic above TC
Shape only: the domains disappear at T_C.

Formulas

  • Curie law
    χ=CT\chi = \dfrac{C}{T}

Key terms

Curie law

For a paramagnet, χ = C/T.

Curie temperature

Temperature above which a ferromagnet becomes paramagnetic.

Exam tips

  • Field-line sketches: closed loops with arrows, S → N inside the magnet.
  • Ratio questions on dipole fields: 1/r31/r^3, and axial = 2 × equatorial.
  • Classification questions: give the sign and size of χ, the behaviour in a non-uniform field and two examples.
  • Curie law in kelvin; χT\chi T = constant.