The Two-Level Paramagnet and the Brillouin Function

Cool a salt of magnetic ions in a field and its magnetization rises, saturates, and — crucially — its low-field susceptibility varies as 1/T1/T: the colder the sample, the more strongly it responds. This is paramagnetism, and it is the single cleanest laboratory for the canonical ensemble. Each ion carries a fixed angular momentum JJ; in a field BB its 2J+12J+1 orientations become 2J+12J+1 energy levels split by −gμBBm-g\mu_B B m. Because the ions are dilute and independent, the whole thermodynamics factorizes into one ion's partition function, and that partition function is a finite geometric series you can sum in closed form. The result is the Brillouin function BJ(x)B_J(x), which gives the magnetization as M=NgμBJ BJ(x)M = Ng\mu_B J\,B_J(x) with x=gμBJB/kBTx = g\mu_B J B/k_BT. This one function contains everything: it reduces to tanh⁡x\tanh x for a spin-12\tfrac12 ion, flows to the classical Langevin function coth⁡x−1/x\coth x - 1/x as J→∞J\to\infty, gives Curie's law χ=C/T\chi = C/T in weak fields, and saturates to full alignment in strong fields. This article derives BJ(x)B_J(x) from the sum over states, proves those four limits, extracts the Curie constant C=Ng2μB2J(J+1)/3kBC = Ng^2\mu_B^2 J(J+1)/3k_B, and works real numbers for a gadolinium-like ion. The magnetic heat capacity of the same level scheme (the Schottky bump) and its use as a refrigerant (adiabatic demagnetization) are named where they belong and treated in their own articles.

Key takeaways
  • NN independent moments of angular momentum JJ in a field BB have 2J+12J+1 levels Em=−gμBBmE_m=-g\mu_B B m; the single-ion partition function sums to Z1=sinh⁡[(2J+1)x/2J]/sinh⁡[x/2J]Z_1 = \sinh[(2J{+}1)x/2J]/\sinh[x/2J] with x=gμBJB/kBTx=g\mu_B J B/k_BT.
  • The magnetization is M=NgμBJ BJ(x)M = Ng\mu_B J\,B_J(x), where the Brillouin function is BJ(x)=2J+12Jcoth⁡(2J+1)x2J−12Jcoth⁡x2JB_J(x)=\tfrac{2J+1}{2J}\coth\tfrac{(2J+1)x}{2J}-\tfrac{1}{2J}\coth\tfrac{x}{2J}.
  • Spin-12\tfrac12: B1/2(x)=tanh⁡xB_{1/2}(x)=\tanh x. Classical limit J→∞J\to\infty: the Langevin function L(x)=coth⁡x−1/xL(x)=\coth x-1/x.
  • Weak field: BJ(x)≈J+13JxB_J(x)\approx\tfrac{J+1}{3J}x, giving Curie's law χ=C/T\chi=C/T with C=Ng2μB2J(J+1)/3kBC=Ng^2\mu_B^2J(J+1)/3k_B.
  • Strong field: BJ→1B_J\to1, so M→Msat=NgμBJM\to M_\text{sat}=Ng\mu_B J — every moment aligned.
  • Key idea: one geometric sum over 2J+12J+1 tilts of a spin produces a universal magnetization curve whose slope is the Curie law and whose plateau is saturation.
The core insight

A paramagnet is NN copies of a single quantum top in a field. Summing the Boltzmann factors over the top's 2J+12J+1 orientations gives a partition function whose field-derivative is the magnetization: M=NgμBJ BJ(x)M = Ng\mu_B J\,B_J(x) with x=gμBJB/kBTx=g\mu_B J B/k_BT. The competition between the alignment energy gμBBg\mu_B B and the thermal energy kBTk_BT is captured entirely by the ratio xx.

Where this lives today

The two-level and 2J+12J+1-level paramagnet is the workhorse example in every statistical-mechanics course because it is exactly solvable and physically real. Its low-field 1/T1/T susceptibility underpins the Curie-law thermometry used throughout low-temperature physics: a paramagnetic salt whose susceptibility is calibrated against a known 1/T1/T line becomes a secondary thermometer valid down to the millikelvin range, and cerium magnesium nitrate (CMN) is a standard choice precisely because it follows Curie's law to very low TT. Its saturation curve is measured routinely in SQUID magnetometry of molecular magnets and rare-earth compounds, where fitting BJ(x)B_J(x) extracts the ground-state JJ and gg directly from the shape of the MM-versus-BB curve. The same level scheme carries entropy S(B/T)S(B/T) that decreases as the field aligns the moments, and this field-tunable entropy is precisely what adiabatic demagnetization exploits to reach millikelvin and, with nuclear moments, microkelvin temperatures. When the moments are not independent — when exchange couples them — the same Brillouin function reappears inside mean-field (Weiss) theory as the self-consistency relation for ferromagnetism, with BB replaced by an effective molecular field B+λMB+\lambda M; the paramagnet is thus the dilute seed of the whole theory of ordered magnetism. The heat capacity of this level scheme is the Schottky anomaly, treated in its own article, and the itinerant-electron cousin is Pauli paramagnetism; both are named-and-deferred here so that this article owns just the magnetization function.

The physical picture

Imagine a crystal in which magnetic ions sit far enough apart that they do not talk to each other — a paramagnetic salt like gadolinium sulfate, where each Gd3+^{3+} ion carries a well-defined total angular momentum JJ and magnetic moment μ=−gμBJ/ℏ\boldsymbol\mu = -g\mu_B\mathbf{J}/\hbar. Switch on a field BB along zz. Space quantization allows only 2J+12J+1 projections m=−J,−J+1,…,+Jm=-J,-J+1,\dots,+J, and each has energy Em=−gμBBmE_m=-g\mu_B B m: the moment most aligned with the field (m=+Jm=+J) sits lowest, the most anti-aligned (m=−Jm=-J) highest. Nothing continuous — a ladder of 2J+12J+1 rungs. Temperature blurs the ladder. At high TT the ion visits all 2J+12J+1 orientations almost equally, so the average moment is small and grows only linearly with BB — this is the Curie regime, χ∝1/T\chi\propto1/T. At low TT (or high BB) the ion is pinned in its ground orientation m=+Jm=+J, the average moment reaches its maximum gμBJg\mu_B J, and further field does nothing — saturation. The whole story is the balance of two energies: the Zeeman splitting gμBBg\mu_B B that wants to align the moment, and kBTk_BT that wants to randomize it. Their ratio is the dimensionless field x=gμBJB/kBTx = g\mu_B J B/k_BT.

Figure
Brillouin magnetization curves B_J(x): from tanh (J=½) down to Langevin (J→∞), all saturating to 1
M / M_sat = B_J(x), x = gμ_B J B / k_B T x = gμ_B J B / k_B T B_J(x) 1 (saturation) J = ½ (tanh x) J = 1 J = 5/2 J → ∞ (Langevin) Curie regime: slope (J+1)/3J

There is a decisive prediction hiding in that ratio. Because BJB_J depends on BB and TT only through x=gμBJB/kBTx=g\mu_B J B/k_BT, magnetization data taken at many different fields and temperatures must collapse onto a single master curve when plotted against B/TB/T. W. E. Henry's 1952 measurements on chromium, iron, and gadolinium salts did exactly this — points spanning fields up to several tesla and temperatures down to 1.31.3 K fell on the three theoretical BJB_J curves for J=32,52,72J=\tfrac32,\tfrac52,\tfrac72 with no adjustable parameters. That scaling collapse, and the straight 1/χ1/\chi–versus–TT line it implies at low field, is the fingerprint of independent moments.

Figure
Curie's law: inverse susceptibility is a straight line through the origin
1/χ = T / C (Curie: straight line through the origin) temperature T 1 / χ slope = 1/C = 3k_B / (N g²μ_B² J(J+1)) θ Curie–Weiss: 1/χ = (T−θ)/C (interacting) pure paramagnet passes through T = 0

The core equations

The whole thermodynamics of NN independent moments follows from one ion's partition function, so we build that first and differentiate it for the magnetization.

Em=−gμBB m,m=−J, −J+1, …, +J(1)E_m = -g\mu_B B\,m, \qquad m = -J,\,-J+1,\,\dots,\,+J \qquad (1)

where: EmE_m is the Zeeman energy of the orientation labelled by the magnetic quantum number mm, gg is the Landé gg-factor, μB=eℏ/2me=9.274×10−24 J/T\mu_B=e\hbar/2m_e=9.274\times10^{-24}\,\mathrm{J/T} is the Bohr magneton, BB the applied field, and JJ the total angular momentum. There are exactly 2J+12J+1 levels, equally spaced by gμBBg\mu_B B.

Z1=∑m=−JJe−βEm=∑m=−JJeam=sinh⁡ ⁣[(2J+1)x2J]sinh⁡ ⁣[x2J](2)Z_1 = \sum_{m=-J}^{J} e^{-\beta E_m} = \sum_{m=-J}^{J} e^{a m} = \frac{\sinh\!\big[(2J+1)\tfrac{x}{2J}\big]}{\sinh\!\big[\tfrac{x}{2J}\big]} \qquad (2)

where: β=1/kBT\beta=1/k_BT, a≡βgμBBa\equiv\beta g\mu_B B is the level spacing in units of kBTk_BT, and x≡aJ=gμBJB/kBTx\equiv aJ = g\mu_B J B/k_BT is the dimensionless field. The single-ion partition function is a finite geometric series (derived below). For NN independent, distinguishable ions on lattice sites the total factorizes, Z=Z1NZ=Z_1^N — the factorization theorem recalled from Factorization of the Partition Function.

M=−∂F∂B=NgμBJ BJ(x),BJ(x)=2J+12Jcoth⁡ ⁣(2J+1)x2J−12Jcoth⁡ ⁣x2J(3)M = -\frac{\partial F}{\partial B} = N g\mu_B J\, B_J(x), \qquad B_J(x)=\frac{2J+1}{2J}\coth\!\frac{(2J+1)x}{2J}-\frac{1}{2J}\coth\!\frac{x}{2J} \qquad (3)

where: F=−NkBTln⁡Z1F=-Nk_BT\ln Z_1 is the Helmholtz free energy, MM the total magnetization, and BJ(x)B_J(x) the Brillouin function — the central object of this article. Msat=NgμBJM_\text{sat}=Ng\mu_B J is the fully aligned magnetization, reached as BJ→1B_J\to1.

χ=lim⁡B→0∂M∂B/ ⋯  =  CT,C=Ng2μB2 J(J+1)3kB(4)\chi = \lim_{B\to0}\frac{\partial M}{\partial B}\Big/\ \cdots \;=\; \frac{C}{T}, \qquad C = \frac{N g^2\mu_B^2\,J(J+1)}{3k_B} \qquad (4)

where: χ\chi is the low-field magnetic susceptibility, CC the Curie constant, and μeff=gJ(J+1) μB\mu_\text{eff}=g\sqrt{J(J+1)}\,\mu_B the effective moment (so C=Nμeff2/3kBC=N\mu_\text{eff}^2/3k_B). In SI a factor μ0\mu_0 accompanies χ\chi depending on whether one differentiates with respect to BB or HH; the physics — χ∝1/T\chi\propto1/T — is convention-independent.

Derivation ASumming the ladder: the single-ion partition function

The goal is to turn the sum over 2J+12J+1 Boltzmann factors in equation (2) into the compact sinh⁡\sinh-ratio, because every thermodynamic quantity is a derivative of ln⁡Z1\ln Z_1. The only tool needed is the finite geometric series, and the one subtlety is bookkeeping the offset exponent so that the series starts cleanly at zero; the payoff is a closed form valid for every integer and half-integer JJ. We work with a=βgμBBa=\beta g\mu_B B and restore x=aJx=aJ at the end.

Step 1. Write the sum with the substitution a=βgμBBa=\beta g\mu_B B: Z1=∑m=−JJeamZ_1=\sum_{m=-J}^{J}e^{am}. Factor out the lowest term to make it an ordinary geometric series: Z1=e−aJ∑k=02JeakZ_1=e^{-aJ}\sum_{k=0}^{2J}e^{ak}, where k=m+Jk=m+J runs over 0,1,…,2J0,1,\dots,2J.

Step 2. Sum the geometric series: ∑k=02Jeak=ea(2J+1)−1ea−1\sum_{k=0}^{2J}e^{ak}=\dfrac{e^{a(2J+1)}-1}{e^{a}-1}. Hence Z1=e−aJea(2J+1)−1ea−1Z_1=e^{-aJ}\dfrac{e^{a(2J+1)}-1}{e^{a}-1}.

Step 3. Symmetrize by multiplying top and bottom by e−a/2e^{-a/2}: the denominator becomes ea/2−e−a/2=2sinh⁡(a/2)e^{a/2}-e^{-a/2}=2\sinh(a/2), and the numerator becomes e−aJ ⁣(ea(2J+1)−1)e−a/2=ea(J+1/2)−e−a(J+1/2)=2sinh⁡[(J+12)a]e^{-aJ}\!\left(e^{a(2J+1)}-1\right)e^{-a/2}=e^{a(J+1/2)}-e^{-a(J+1/2)}=2\sinh[(J+\tfrac12)a].

Step 4. Collect: Z1=sinh⁡[(J+12)a]sinh⁡(a/2)Z_1=\dfrac{\sinh[(J+\tfrac12)a]}{\sinh(a/2)}. Since (J+12)a=(2J+1)a2(J+\tfrac12)a=(2J+1)\tfrac{a}{2} and a=x/Ja=x/J, this is Z1=sinh⁡[(2J+1)x/2J]sinh⁡[x/2J]Z_1=\dfrac{\sinh[(2J+1)x/2J]}{\sinh[x/2J]}, equation (2). Verified: the companion script sums ∑m=−JJeam\sum_{m=-J}^{J}e^{am} term by term for J=12,1,32,52J=\tfrac12,1,\tfrac32,\tfrac52 and confirms it equals sinh⁡[(2J+1)a/2]/sinh⁡(a/2)\sinh[(2J+1)a/2]/\sinh(a/2) at four values of aa each.

Go deeper · Derivation B · 1 minFrom the partition function to the Brillouin function and Curie's law
Derivation BFrom the partition function to the Brillouin function and Curie's law

Here the aim is to obtain the magnetization (equation 3) and its weak-field limit (equation 4) directly from ln⁡Z1\ln Z_1, and to establish the article's owned result: the single universal function BJ(x)B_J(x) that interpolates between Curie linearity and saturation. The strategy is that the average moment is a logarithmic derivative of Z1Z_1; the subtlety is a chain-rule factor between the variables aa and x=aJx=aJ, which is exactly what produces the prefactor JJ in M=NgμBJ BJM=Ng\mu_B J\,B_J. The small-xx expansion then uses coth⁡y≈1/y+y/3\coth y\approx 1/y+y/3.

Step 1. The average projection is ⟨m⟩=1Z1∑mm eam=∂ln⁡Z1∂a\langle m\rangle=\dfrac{1}{Z_1}\sum_m m\,e^{am}=\dfrac{\partial\ln Z_1}{\partial a}. Differentiating the sinh⁡\sinh-ratio, ∂ln⁡Z1∂a=2J+12coth⁡ ⁣[(2J+1)a2]−12coth⁡ ⁣[a2]\dfrac{\partial\ln Z_1}{\partial a}=\dfrac{2J+1}{2}\coth\!\big[\tfrac{(2J+1)a}{2}\big]-\tfrac12\coth\!\big[\tfrac{a}{2}\big].

Step 2. Convert to x=aJx=aJ (so ∂/∂a=J ∂/∂x\partial/\partial a=J\,\partial/\partial x is not needed here; just substitute a=x/Ja=x/J): ⟨m⟩=J ⁣[2J+12Jcoth⁡(2J+1)x2J−12Jcoth⁡x2J]=J BJ(x)\langle m\rangle=J\!\left[\dfrac{2J+1}{2J}\coth\tfrac{(2J+1)x}{2J}-\dfrac{1}{2J}\coth\tfrac{x}{2J}\right]=J\,B_J(x). The bracket defines BJ(x)B_J(x). Each ion contributes moment gμB⟨m⟩g\mu_B\langle m\rangle, so M=NgμB⟨m⟩=NgμBJ BJ(x)M=Ng\mu_B\langle m\rangle=Ng\mu_B J\,B_J(x).

Step 3. Weak field. Expand each coth⁡y≈1/y+y/3\coth y\approx 1/y+y/3 with y=(2J+1)x2Jy=\tfrac{(2J+1)x}{2J} and y=x2Jy=\tfrac{x}{2J}. The 1/y1/y pieces cancel, leaving BJ(x)=x12J2[(2J+1)2−1]+O(x3)=x(4J2+4J)12J2=J+13J xB_J(x)=\dfrac{x}{12J^2}\big[(2J+1)^2-1\big]+O(x^3)=\dfrac{x(4J^2+4J)}{12J^2}=\dfrac{J+1}{3J}\,x.

Step 4. Curie constant. Insert x=gμBJB/kBTx=g\mu_B J B/k_BT: M≈NgμBJ⋅J+13J⋅gμBJBkBT=Ng2μB2J(J+1)3kBBTM\approx Ng\mu_B J\cdot\dfrac{J+1}{3J}\cdot\dfrac{g\mu_B J B}{k_BT}=\dfrac{Ng^2\mu_B^2 J(J+1)}{3k_B}\dfrac{B}{T}. Thus χ∝1/T\chi\propto1/T with C=Ng2μB2J(J+1)/3kBC=Ng^2\mu_B^2J(J+1)/3k_B, equation (4). Verified: the script confirms ⟨m⟩=J BJ(x)\langle m\rangle=J\,B_J(x) numerically for J=12,52J=\tfrac12,\tfrac52, the slope BJ′(0)=(J+1)/3JB_J'(0)=(J+1)/3J symbolically (giving 1,23,7151,\tfrac23,\tfrac{7}{15} for J=12,1,52J=\tfrac12,1,\tfrac52), and that Msmall=C B/TM_\text{small}=C\,B/T with CC as quoted.

Limiting cases

Each limit of BJ(x)B_J(x) is a physical check on the construction.

CaseResultMeaning
Spin-12\tfrac12, J=12J=\tfrac12B1/2(x)=tanh⁡xB_{1/2}(x)=\tanh xTwo levels only; M=NgμB12tanh⁡(μB/kBT)M=Ng\mu_B\tfrac12\tanh(\mu B/k_BT) — the textbook two-state paramagnet.
Classical, J→∞J\to\inftyBJ(x)→coth⁡x−1x=L(x)B_J(x)\to\coth x-\dfrac1x=L(x)A freely rotating classical moment; Langevin's 1905 result recovered as the continuum limit.
Weak field, x≪1x\ll1BJ≈J+13JxB_J\approx\dfrac{J+1}{3J}xLinear response; Curie's law χ=C/T\chi=C/T, susceptibility diverging as T→0T\to0.
Strong field, x≫1x\gg1BJ→1B_J\to1, M→NgμBJM\to Ng\mu_B JEvery moment pinned to m=+Jm=+J; saturation, field-independent.

Worked examples

Example 1 — A gadolinium-like ion in a modest field. Take Gd3+\mathrm{Gd}^{3+}: half-filled 4f4f shell, L=0L=0, so g=2g=2 and J=S=72J=S=\tfrac72. Put it in B=1B=1 T at T=300T=300 K. How aligned is it, and what is its effective moment?

Step 1. Dimensionless field: x=gμBJBkBT=2 (9.274×10−24) (3.5)(1)(1.381×10−23)(300)=0.0157x=\dfrac{g\mu_B J B}{k_BT}=\dfrac{2\,(9.274\times10^{-24})\,(3.5)(1)}{(1.381\times10^{-23})(300)}=\mathbf{0.0157}. This is tiny — we are deep in the Curie regime.

Step 2. Fractional alignment: M/Msat=B7/2(0.0157)≈J+13Jx=4.510.5(0.0157)=0.0067M/M_\text{sat}=B_{7/2}(0.0157)\approx\dfrac{J+1}{3J}x=\dfrac{4.5}{10.5}(0.0157)=\mathbf{0.0067}. Only about 0.7%0.7\% of the moments' worth of alignment at room temperature and 11 T — which is why paramagnets look magnetically inert unless you go cold or strong.

Step 3. Effective moment: μeff=gJ(J+1) μB=23.5×4.5 μB=63 μB=7.94 μB\mu_\text{eff}=g\sqrt{J(J+1)}\,\mu_B=2\sqrt{3.5\times4.5}\,\mu_B=\sqrt{63}\,\mu_B=\mathbf{7.94\,\mu_B}, the standard tabulated value for Gd3+\mathrm{Gd}^{3+}. The Curie constant per mole then follows from C=NAμeff2/3kBC=N_A\mu_\text{eff}^2/3k_B. The takeaway: at ordinary temperatures a paramagnet responds linearly and weakly; the 1/T1/T growth of χ\chi is what makes it a useful thermometer and refrigerant at low TT.

Example 2 — The same ion, cold and strong: approaching saturation. Now cool to T=1T=1 K and raise the field to B=5B=5 T.

Step 1. Dimensionless field: x=2(9.274×10−24)(3.5)(5)(1.381×10−23)(1)=23.5x=\dfrac{2(9.274\times10^{-24})(3.5)(5)}{(1.381\times10^{-23})(1)}=\mathbf{23.5}. We are now far into the strong-field regime, x≫1x\gg1.

Step 2. Alignment: B7/2(23.5)=87coth⁡ ⁣(87⋅23.5)−17coth⁡ ⁣(23.57)=0.9997B_{7/2}(23.5)=\dfrac{8}{7}\coth\!\big(\tfrac{8}{7}\cdot23.5\big)-\dfrac{1}{7}\coth\!\big(\tfrac{23.5}{7}\big)=\mathbf{0.9997}. The moments are essentially fully aligned; further field buys almost nothing.

Step 3. Contrast: raising the temperature back to 300300 K at fixed 55 T would drop xx by a factor 300300 to ≈0.078\approx0.078, and M/MsatM/M_\text{sat} back to a few percent. Saturation is a low-temperature, high-field corner. The takeaways: the magnetization is controlled entirely by x=gμBJB/kBTx=g\mu_B J B/k_BT — 0.7%0.7\% aligned at 11 T/300300 K, but 99.97%99.97\% aligned at 55 T/11 K.

Origins · 1 minléon brillouin and how this was discovered
LB
léon brillouin
1889–1969 · French physicist who quantized the theory of paramagnetism, giving the magnetization function that bears his name

Léon Brillouin, working in Paris in the late 1920s, replaced Langevin's classical freely-rotating moment with a quantum top restricted to 2J+12J+1 orientations, and in 1927 obtained the quantized magnetization curve BJ(x)B_J(x) now universally called the Brillouin function. It was an early, concrete triumph of space quantization: the same discreteness that Stern and Gerlach had seen in a beam now dictated the bulk magnetization of a salt. Brillouin's name recurs across physics — Brillouin zones in solids, Brillouin scattering of light by sound, and the "B" in the WKB(J)/Brillouin semiclassical method — and late in life he wrote influentially on the link between entropy and information (his "negentropy" principle). His paramagnet remains the standard first worked example of the canonical ensemble applied to a finite-level system.

History
1895
— Pierre Curie measures the paramagnetic susceptibility and finds χ ∝ 1/T
1905
— Paul Langevin builds the classical statistical theory of paramagnetism and the Langevin function
1907
— Pierre Weiss adds the molecular field, extending the picture to ferromagnetism
1922
— Stern and Gerlach demonstrate space quantization of magnetic moments
1927
— Léon Brillouin derives the quantized magnetization curve, the Brillouin function B_J(x)
1952
— W. E. Henry's paramagnetic-salt data collapse onto the B_J curves confirms the theory across J and B/T

Going further

References. Reif, Fundamentals of Statistical and Thermal Physics, §7.8 (ideal paramagnet) · Kittel, Introduction to Solid State Physics, ch. 11 (paramagnetism, the Henry data collapse) · Kardar, Statistical Physics of Particles, §4 · Ashcroft & Mermin, Solid State Physics, ch. 31 · Blundell, Magnetism in Condensed Matter, ch. 2.

Provenance. A verifier reproduces: (1) the geometric-sum identity Z1=sinh⁡[(2J+1)a/2]/sinh⁡(a/2)Z_1=\sinh[(2J{+}1)a/2]/\sinh(a/2) for J=12,1,32,52J=\tfrac12,1,\tfrac32,\tfrac52; (2) B1/2(x)=tanh⁡xB_{1/2}(x)=\tanh x and B1/2(1)=0.76159B_{1/2}(1)=0.76159; (3) the J→∞J\to\infty Langevin limit coth⁡x−1/x\coth x-1/x with L(2)=0.53731L(2)=0.53731; (4) the small-xx slope (J+1)/3J(J+1)/3J giving 1,23,7151,\tfrac23,\tfrac{7}{15}; (5) ⟨m⟩=J BJ(x)\langle m\rangle=J\,B_J(x); (6) the Curie constant C=Ng2μB2J(J+1)/3kBC=Ng^2\mu_B^2J(J+1)/3k_B and μeff=7.94 μB\mu_\text{eff}=7.94\,\mu_B for Gd3+\mathrm{Gd}^{3+}; (7) the worked values x=0.0157x=0.0157, M/Msat=0.0067M/M_\text{sat}=0.0067 at 11 T/300300 K and x=23.5x=23.5, M/Msat=0.9997M/M_\text{sat}=0.9997 at 55 T/11 K.

Builds on: Canonical Partition Function · Boltzmann Factor · Factorization of the Partition Function. Leads to: The Schottky Anomaly · Adiabatic Demagnetization and Magnetic Cooling · Pauli Paramagnetism.

Why are there exactly 2J+1 energy levels?

Because a quantum angular momentum JJ has 2J+12J+1 allowed projections along any chosen axis, m=−J,−J+1,…,+Jm=-J,-J+1,\dots,+J — this is space quantization. In a field the energy depends only on that projection, Em=−gμBBmE_m=-g\mu_B B m, so each projection is one energy level. For a spin-12\tfrac12 ion that is two levels; for Gd3+\mathrm{Gd}^{3+} with J=72J=\tfrac72 it is eight. The count 2J+12J+1 is exactly what makes the partition function a finite geometric series rather than an integral.

Where does the Landé g-factor come from and why is it often about 2?

The gg-factor relates the magnetic moment to the angular momentum, μ=−gμBJ/ℏ\boldsymbol\mu=-g\mu_B\mathbf{J}/\hbar. For pure spin g≈2g\approx2 (the Dirac value, 2.00232.0023 with QED corrections); for pure orbital motion g=1g=1; for a general ion with both, the Landé formula interpolates using JJ, LL, and SS. Gd3+\mathrm{Gd}^{3+} has L=0L=0 (half-filled shell), so it is pure spin and g=2g=2 exactly to good approximation, which is why it is the cleanest textbook paramagnet.

Why does the magnetization depend only on B/T and not on B and T separately?

Because the only place BB and TT enter the single-ion problem is through the Boltzmann factor e−Em/kBT=egμBBm/kBTe^{-E_m/k_BT}=e^{g\mu_B B m/k_BT}, and there BB and TT appear solely as the ratio B/TB/T (inside x=gμBJB/kBTx=g\mu_B J B/k_BT). Everything thermodynamic is built from that partition function, so it too can depend only on B/TB/T. This is why data at many fields and temperatures collapse onto one curve when plotted against B/TB/T — a direct, parameter-free test that the moments are independent.

How is this different from Curie–Weiss behavior in a ferromagnet?

Curie's law χ=C/T\chi=C/T is for independent moments and its 1/χ1/\chi line passes through the origin. When moments interact (exchange), mean-field theory replaces BB by B+λMB+\lambda M, and the susceptibility becomes χ=C/(T−θ)\chi=C/(T-\theta) — the Curie–Weiss law, whose 1/χ1/\chi line intercepts the temperature axis at the Weiss temperature θ\theta (positive for ferromagnets). Above θ\theta the material is still paramagnetic but "assisted"; at θ\theta it orders. The Brillouin function reappears there as the self-consistency equation, so this article's machinery is the seed of the theory of magnetism, not just its dilute limit.

What sets the saturation magnetization, and can you exceed it?

Saturation is reached when every moment sits in its lowest Zeeman level m=+Jm=+J, giving Msat=NgμBJM_\text{sat}=Ng\mu_B J — the maximum the localized moments can provide. You cannot exceed it by raising the field further; BJ(x)B_J(x) approaches 11 but never surpasses it. (You can get additional magnetization from other sources — conduction electrons, orbital contributions, or induced moments — but those are separate mechanisms, not more of the same localized alignment.)

Is the classical Langevin theory just wrong, then?

Not wrong — incomplete. Langevin's 1905 model of a freely rotating classical moment gives M=NgμBJ L(x)M=Ng\mu_B J\,L(x) with L(x)=coth⁡x−1/xL(x)=\coth x-1/x, which is exactly the J→∞J\to\infty limit of the quantum result. For ions with large JJ it is an excellent approximation. What it misses is the discreteness: for small JJ (especially spin-12\tfrac12, where BJ=tanh⁡B_J=\tanh) the finite number of levels changes both the initial slope (J+1)/3J(J+1)/3J and the detailed shape of the approach to saturation. The quantum Brillouin function contains Langevin as one limit and the two-state tanh⁡\tanh as the other.

Before this

Where this leads