Paramagnetism

Paramagnetism is a form of magnetism in which certain materials are weakly attracted to an externally applied magnetic field. Unlike ferromagnetic materials such as iron, paramagnetic materials do not retain their magnetisation once the external field is removed — the effect disappears almost instantly. Common paramagnetic materials include aluminium, platinum, oxygen gas, and many transition-metal salts such as copper sulfate. The origin of paramagnetism lies at the atomic level. Atoms or ions in a paramagnetic material possess permanent magnetic dipole moments arising from unpaired electrons. Each electron behaves like a tiny bar magnet due to its intrinsic spin and its orbital motion around the nucleus. In the absence of an external field, thermal energy causes these atomic dipoles to point in random directions, so the material has zero net magnetisation. When an external magnetic field is applied, the dipoles partially align with the field, producing a small but measurable net magnetisation in the direction of the field. The degree of alignment depends on the competition between magnetic potential energy (which tries to align the dipoles) and thermal energy (which randomises them). This explains why paramagnetism becomes stronger at lower temperatures — a relationship captured quantitatively by Curie's Law. Understanding paramagnetism is essential for applications ranging from MRI contrast agents to the study of electron structure in chemistry and materials science.

Key takeaways
  • Unpaired Electrons as Magnetic Dipoles
  • Thermal Randomisation with No External Field
  • Partial Alignment in an External Field
  • Curie's Law and Magnetic Susceptibility
  • Why Paramagnetism Disappears When the Field Is Removed

Unpaired Electrons as Magnetic Dipoles

Every electron has a quantum property called spin, which gives it an intrinsic magnetic dipole moment. In atoms where all electrons are paired, their spins cancel (+12+\frac{1}{2} and −12-\frac{1}{2}) and no net moment exists — this is diamagnetism. Paramagnetic atoms have at least one unpaired electron, so each atom carries a permanent magnetic dipole moment μ\mu. For a single unpaired electron, the magnitude of the spin magnetic moment is approximately μB=9.274×10−24\mu_B = 9.274 \times 10^{-24} J/T, called the Bohr magneton.

Thermal Randomisation with No External Field

At room temperature, thermal energy kBTk_BT (where kB=1.381×10−23k_B = 1.381 \times 10^{-23} J/K and TT is absolute temperature) is much larger than the magnetic energy of a typical dipole. This means the dipoles are constantly jostled by thermal vibrations and point in essentially random directions. The vector sum of all dipole moments in the material averages to zero, so the bulk magnetisation M=0M = 0.

Partial Alignment in an External Field

When an external magnetic field B\mathbf{B} is applied, each dipole experiences a torque τ=μ×B\boldsymbol{\tau} = \boldsymbol{\mu} \times \mathbf{B} that tries to align it with the field. The potential energy of a dipole in the field is U=−μ⋅B=−μBcos⁡θU = -\boldsymbol{\mu} \cdot \mathbf{B} = -\mu B \cos\theta, where θ\theta is the angle between the dipole and the field. Alignment lowers the energy, but thermal agitation counteracts this. The result is a small net alignment — more dipoles point with the field than against it — producing a weak magnetisation MM parallel to B\mathbf{B}.

Curie's Law and Magnetic Susceptibility

The bulk behaviour is described by Curie's Law: M=CTHM = \frac{C}{T} H, where MM is the magnetisation (A/m), HH is the applied magnetic field intensity (A/m), TT is absolute temperature (K), and CC is the material-specific Curie constant. The magnetic susceptibility is χm=M/H=C/T\chi_m = M/H = C/T. Since χm>0\chi_m > 0 for paramagnets (the induced magnetisation is parallel to HH) but very small (typically 10−610^{-6} to 10−310^{-3}), the attraction to a magnet is real but extremely weak compared to ferromagnetism. Crucially, χm\chi_m increases as temperature decreases, meaning cold paramagnets are more strongly attracted to magnets.

Why Paramagnetism Disappears When the Field Is Removed

Unlike ferromagnets, paramagnets have no cooperative interaction between neighbouring atomic dipoles (no exchange coupling). Once the external field is switched off, thermal energy immediately re-randomises the dipole orientations, and MM returns to zero. This is why paramagnets are described as having no magnetic memory or remanence. The relaxation time is extraordinarily short — on the order of nanoseconds to microseconds — making paramagnets behave as if they are magnetically 'neutral' in everyday conditions.

The Key Equation

$$M = \frac{C}{T} H
- **M** — Magnetisation (A m⁻¹): The magnetic dipole moment per unit volume of the material; indicates how strongly the material is magnetised. - **C** — Curie Constant (A m⁻¹ K A⁻¹ m = K): A material-specific constant that depends on the density of magnetic dipoles and their individual magnetic moments. - **T** — Absolute Temperature (K): Temperature measured in Kelvin from absolute zero. Higher temperatures reduce alignment of dipoles. - **H** — Magnetic Field Intensity (A m⁻¹): The applied magnetic field intensity, related to the magnetic flux density by $B = \mu_0(H + M)$. ## Worked Example **Problem.** A paramagnetic salt has a Curie constant $C = 1.8 \times 10^{-3}$ K and is placed in a magnetic field of intensity $H = 1.2 \times 10^5$ A/m at a temperature of $T = 300$ K. (a) Calculate the magnetic susceptibility $\chi_m$. (b) Calculate the magnetisation $M$. (c) How does $M$ change if the temperature is reduced to 150 K?

\chi_m(300\,\text{K}) = 6.0 \times 10^{-6},\quad M(300\,\text{K}) = 0.72\,\text{A/m};\quad M(150\,\text{K}) = 1.44\,\text{A/m}

∗∗Answer.∗∗At300K:susceptibility=6.0×10−6,magnetisation=0.72A/m.At150K:susceptibility=1.2×10−5,magnetisation=1.44A/m.**Answer.** At 300 K: susceptibility = 6.0 \times 10⁻⁶, magnetisation = 0.72 A/m. At 150 K: susceptibility = 1.2 \times 10⁻⁵, magnetisation = 1.44 A/m.
Figure
Diagram
Paramagnetism: Dipole AlignmentNo External FieldRandom orientationsNet M = 0External Field AppliedNSB →Partial alignment with BSmall net M > 0Red arrows: no field (random). Green arrows: field applied (mostly aligned). Dashed box = magnet poles.
Origins · 1 minPierre Curie and how this was discovered
PC
Pierre Curie
1859–1906 · French

Pierre Curie discovered the quantitative law governing paramagnetism in 1895 during his doctoral research. He showed experimentally that the magnetic susceptibility of paramagnetic materials is inversely proportional to absolute temperature — the relationship now known as Curie's Law (χm=C/T\chi_m = C/T). He also discovered the Curie temperature, the point above which ferromagnetic materials lose their ferromagnetism and become paramagnetic. Pierre Curie was so absorbed in scientific work that he forgot his own wedding date. He was later awarded the Nobel Prize in Physics in 1903 (shared with his wife Marie Curie and Henri Becquerel) — but for radioactivity research, not magnetism!

  • Diamagnetism — Diamagnetism is the contrasting magnetic behaviour where materials with no unpaired electrons are weakly repelled by magnetic fields; comparing both helps clarify how electron configuration determines magnetic response.
  • Ferromagnetism — Ferromagnetism involves strong, permanent magnetisation from cooperative alignment of dipoles; understanding it alongside paramagnetism shows why exchange interactions between atoms change magnetic strength by many orders of magnitude.
  • Magnetic Susceptibility — Magnetic susceptibility χm\chi_m is the key quantity that distinguishes paramagnets (0<χm≪10 < \chi_m \ll 1) from diamagnets (χm<0\chi_m < 0) and ferromagnets (χm≫1\chi_m \gg 1).
  • Electron Spin — Paramagnetism originates from unpaired electron spins; understanding quantum spin and the Bohr magneton is essential for explaining why only certain atoms are paramagnetic.
  • Thermal Energy and Temperature — The competition between magnetic potential energy and thermal energy kBTk_BT determines the degree of dipole alignment, directly explaining why Curie's Law has temperature in the denominator.