Modern Physics · Advanced Topics

Magnetism in Condensed Matter

Magnetism arises from spin — quantum mechanical angular momentum with no classical analog. From ferromagnetism to frustrated magnets to quantum spin liquids, magnetic materials display a rich variety of quantum phases driven by exchange interactions.

PrerequisitesSolidstatephysics(Ch.SS)Statisticalmechanics(Ch.S)Quantummechanics(Ch.20Solid-state physics (Ch. SS) \cdot Statistical mechanics (Ch. S) \cdot Quantum mechanics (Ch. 20 Grouptheory(Ch.GT\cdot Group theory (Ch. GT
Learning Goals
  • Derive the Brillouin function and Curie law for a paramagnet and identify when saturation occurs.
  • Explain the origin oftheexchangeinteractionandusemeanfieldtheorytocomputetheCurietemperatureTCof the exchange interaction and use mean-field theory to compute the Curie temperature T_{C}
  • Derivethemagnondispersionωkk2foraHeisenbergferromagnetandpredicttheBlochTDerive the magnon dispersion \omega_k \propto k^{2} for a Heisenberg ferromagnet and predict the Bloch T^(3/2) heat capacity.
  • Distinguish ferromagnetic, antiferromagnetic, and frustrated geometries and explain how frustration produces spin liquids.
  • Apply Larmor precession to describe NMR signal generation and spatial encoding in MRI.

MG.1 Paramagnetism and Diamagnetism

In an external field H, a free spin-J atom acquires energy −g_J μ_B m_J H. The partition function Z = Σ e^(g_J μ_B m_J H/(k_BT)) gives the magnetization:

M=NgJμBJBJ(x)wherex=gJμBJH/(kBT)andBJistheBrillouinfunctionM = N g_{J} \mu_B J B_{J}(x) \qquad where x = g_{J} \mu_B J H / (k_{B} T) and B_{J} is the Brillouin function(MG.1)

At high T (x ≪ 1): M ≈ N g_J² μ_B² J(J+1) H/(3k_BT) — Curie law: χ = C/T. At low T (x ≫ 1): M → N g_J μ_B J (saturation).

Diamagnetism: all materials are weakly diamagnetic. The orbital response of closed shells to H gives χ_dia = −Ze²⟨r²⟩/(6m_e c²) per atom (Langevin). Negative susceptibility: induced magnetization opposes applied field. Superconductors are perfect diamagnets (Meissner effect): χ = −1.

MG.2 Exchange Interaction and the Heisenberg Model

Magnetism in solids comes from the exchange interaction — a purely quantum mechanical effect arising from the overlap of wavefunctions and the Pauli exclusion principle. For two electrons on adjacent atoms:

Hex=2JS1S2(HeisenbergexchangeHamiltonian)H_{ex} = -2J S_{1} \cdot S_{2} \qquad (Heisenberg exchange Hamiltonian)(MG.2)

J > 0: ferromagnetic exchange (parallel spins lower energy — triplet state preferred). J < 0: antiferromagnetic exchange (antiparallel spins — singlet preferred). Exchange integral: J = ⟨↑↓|1/r₁₂|↑↓⟩ − ⟨↑↓|1/r₁₂|↓↑⟩ (direct vs exchange term).

The full Heisenberg modelon a lattice: H = −J Σ_(ij) S_i · S_j − g μ_B H Σᵢ S_i^z. For J > 0: ferromagnet. For J < 0: antiferromagnet. The Ising model (1D solvable): H = −J Σ σᵢ σᵢ₊₁.

MG.3 Ferromagnetism — Mean-Field Theory

In mean-field theory, replace S_j · S_i → ⟨S_j⟩ · S_i = m S_i^z (Weiss molecular field approximation). Each spin sees an effective field H_eff = H + λm where λ = 2zJ/(g μ_B)² is the Weiss constant (z = coordination number).

Self-consistency equation: m = B_J(g μ_B J H_eff/(k_BT)). Curie temperature: T_C = 2zJ J(J+1)/(3k_B) (for J→1/2 Ising: T_C = zJ/(2k_B)).

TC=2zJJ(J+1)/(3kB)(CurieWeisstemperature,meanfield)T_{C} = 2zJ J(J+1)/(3k_B) \qquad (Curie-Weiss temperature, mean field)(MG.3)

Below T_C: spontaneous magnetization m ≠ 0. Near T_C: m ∝ (T_C − T)^β with mean-field β = 1/2. Actual 3D Ising: β ≈ 0.326 (fluctuations matter). Curie-Weiss law above T_C: χ = C/(T − T_C).

Example MG.1Iron Ferromagnetism — Curie Temperature

IronhasTC=1043K,spinS=1,g2.2,BCClattice(z=8).EstimateJfrommeanfielIron has T_{C} = 1043 K, spin S = 1, g \approx 2.2, BCC lattice (z = 8). Estimate J from mean-field theory and compare to the actual exchange energy.

Mean-field:TC=2zJS(S+1)/(3kB).WithS=1,z=8:TC=2×8\timesJ×2/(3×1.38×1023T_{C} = 2zJ S(S+1)/(3k_B). With S=1, z=8: T_{C} = 2\times8\timesJ\times2/(3\times1.38\times10^{-23}.
Solve for J:J=3kBTC/(2zS(S+1))=3×1.38×1023×1043/(2×8×1×2)=4.31×1020/32=1.35×1021J=0.0J = 3k_B T_{C}/(2zS(S+1)) = 3\times1.38\times10^{-23}\times1043/(2\times8\times1\times2) = 4.31\times10^{-20}/32 = 1.35\times10^{-21} J = 0.0084 eV.
Compare:Thisistheeffectiveexchangeperbond.Theactual3dexchangeinFeis 100meV10×laThis is the effective exchange per bond. The actual 3d exchange in Fe is ~100 meV — 10\times larger.MeanfieldoverestimatesTCbyincludingallfluctuationsasiftheyallpointintrger. Mean-field overestimates T_{C} by including all fluctuations as if they all point in themeanfielddirection.ActualquantumMonteCarlogivescorrectTCwithpropertreatmenhe mean-field direction. Actual quantum Monte Carlo gives correct T_{C} with proper treatment of fluctuations.
Spin waves:The low-T excitations of a ferromagnet are magnons — collective spin-wave modes with dispersion \omega_quadratic,unlikephononswhicharelinear).Magnoncontributiontoheatcapacity:CVTquadratic, unlike phonons which are linear). Magnon contribution to heat capacity: C_{V} \propto T^(3/2) (Bloch T^(3/2) law).

MG.4 Antiferromagnetism and Frustration

For J < 0 on a bipartite lattice (two sublattices A and B), the ground state has spins on A pointing up and B pointing down — antiferromagnetism. Néel temperature T_N = 2z|J|S(S+1)/(3k_B) (same formula as T_C). Neutron scattering (magnetic Bragg peaks) detects the antiferromagnetic order.

Geometric frustration: on a triangular or kagome lattice, you cannot simultaneously satisfy all antiferromagnetic bonds. For three spins on a triangle: two can be antiparallel but the third cannot be antiparallel to both. This frustration prevents conventional magnetic order and can give rise to:

Spin liquid: highly entangled state with no long-range order even at T = 0. Ground state is a superposition of many configurations (resonating valence bonds, proposed by Anderson 1973 for high-T_c). Characterized by fractional excitations (spinons) and topological order. Candidate materials: herbertsmithite (ZnCu₃(OH)₆Cl₂), RVB models of cuprate superconductors.

MG.5 Spin Dynamics and NMR

A spin in a magnetic field H precesses (Larmor precession):

dS/dt=γS×H(Larmorprecession,γ=gyromagneticratio)dS/dt = \gamma S \times H \qquad (Larmor precession, \gamma = gyromagnetic ratio)(MG.4)

For protons: γ = 2.675×10⁸ rad/(s·T) → Larmor frequency ν_L = γH/(2π). At H = 3 T (clinical MRI): ν_L = 127 MHz (RF range).

NMR (Nuclear Magnetic Resonance): RF pulse at ν_L tips the magnetization. Relaxation times T₁ (longitudinal, spin-lattice) and T₂ (transverse, spin-spin) encode local chemical environment. MRI adds a gradient field to encode spatial position in the Larmor frequency: frequency encodes location. Fourier transform of FID (free induction decay) → image. Nobel Prizes: Bloch & Purcell 1952, Lauterbur & Mansfield 2003.

Definition MG.1Common Traps
  • Magnetization is material response: it is not the same quantity as applied H or total B.
  • Exchange is quantum mechanical: ferromagnetism is not caused by classical dipole alignment alone.
  • Domains reduce magnetic energy: a demagnetized sample can still have ordered domains.
  • Curie temperature marks collective order: above it, thermal disorder destroys spontaneous magnetization.
Exercises — MG.1–MG.5 Magnetism
1.
Gadolinium(Gd3+,J=7/2,g=2)hasTC=292K.UsetheCurieWeisslawtoestimatetheGadolinium (Gd^{3+}, J = 7/2, g = 2) has T_{C} = 292 K. Use the Curie-Weiss law to estimate the exchangeintegralJforaz=12lattice.WhatistheCurieconstantexchange integral J for a z = 12 lattice. What is the Curie constant
eV
Straightforward
2.Derivethemagnondispersionωkk2foraHeisenbergferromagnetandshowthatthelowtDerive the magnon dispersion \omega_k \propto k^{2} for a Heisenberg ferromagnet and show that the low-temperatureheatcapacityisCT(3/2emperature heat capacity is C \propto T^(3/2.
Intermediate
3.
ExplainthephysicsofMRI.Howdoesspatialencodingwork?WhydoesSNRscaleasH02?WhaExplain the physics of MRI. How does spatial encoding work? Why does SNR scale as H_{0}^{2}? What is achievable resolution at 3 T?
Hz
Intermediate
4.Describe the Kitaev honeycomb model and its exact solution via Majorana fermions. Why is this a quantum spin liquid and what physical materials realize it?
Challenging
Key Takeaways
  • Paramagnetism:M=NgμBJBJ(x).Curielawχ=C/TathighT.SaturationatlowTParamagnetism: M = N g\mu_B J B_{J}(x). Curie law \chi = C/T at high T. Saturation at low T.
  • Exchange interaction J: J>0 ferromagnet, J<0 antiferromagnet. From wavefunction overlap + Pauli.
  • Curietemperature:TC=2zJS(S+1)/(3kB)frommeanfield.CurieWeiss:χ=C/(TTCCurie temperature: T_{C} = 2zJS(S+1)/(3k_B) from mean field. Curie-Weiss: \chi = C/(T-T_{C}.
  • Magnondispersion:ωk2(ferromagnet).LowTheatcapacityCT3/2(BlochMagnon dispersion: \omega \propto k^{2} (ferromagnet). Low-T heat capacity C \propto T^{3/2} (Bloch.
  • Frustration(triangular/kagome):preventslongrangeorderquantumspinliquid,fractionFrustration (triangular/kagome): prevents long-range order \to quantum spin liquid, fractional excitations.
  • Larmorprecession:dS/dt=\gammaS\timesH.NMR/MRIusesωL=\gammaHtoprobematterLarmor precession: dS/dt = \gammaS\timesH. NMR/MRI uses \omega_L = \gammaH to probe matter.