CHEM2524Chemical Physics

    06-05 · Week 7

    Mean-field theory: replace the crowd with its average and a transition appears

    Mean-field theory swaps every neighbour interaction for an average one, which turns the Ising magnet into a self-consistency equation that has a sharp transition at T_c = Jd/k.

    • Solve the non-interacting Ising model and get m = N tanh(beta B).
    • State the mean-field idea and apply it to the Ising energy.
    • Derive m/N = tanh(beta J d m/N) and solve it graphically.
    • Say how many solutions exist above and below T_c and what they mean.
    • State what mean-field theory explains and where it is only approximate.

    20 min readJump to the quiz ↓

    When interactions are too hard, replace them with an average

    Intuition

    You are in a crowd at a concert and you want to know whether to sway left or right. Listening to every person around you is hopeless. So you look at the average mood of the crowd and follow that. Mean-field theory does the same for a particle: it stops tracking each neighbour and feels only their average.

    Lecture 21 recaps where things stand. Phase transitions are sharp changes in a macroscopic parameter. They need interactions and the thermodynamic limit. Interacting systems are hard, because the configuration space is enormous and exact solutions are usually impossible. Simulations help, but it can be hard to get an intuitive explanation from them.

    Mean-field theory is an approximate way of including interactions. It is sometimes crude, but it gives qualitative insight and, importantly, it lets us predict phase transitions. The lecture applies it to two systems: the Ising model of the ferromagnetic to paramagnetic transition (this page), and the van der Waals model of the real gas (next page).

    The Ising model is the lattice of ±1\pm 1 spins from the last lecture, with energy

    E=−B∑iσi−J∑⟨ij⟩σiσjE = -B\sum_i \sigma_i - J\sum_{\langle ij\rangle}\sigma_i\sigma_j

    and net magnetisation m=∑iσim = \sum_i \sigma_i. The behaviour is m∼0m \sim 0 for T≫TcT \gg T_c and ∣m∣∼1|m| \sim 1 for T≪TcT \ll T_c. The lecture asks the question: how can we be sure that the transition is actually sharp?

    First the easy case: no interactions at all

    Drop the JJ term. The energy becomes

    E=−B∑iσiE = -B\sum_i\sigma_i

    Now each spin stands alone, so use one-spin quantities. A spin has two states, up (energy −B-B) and down (energy +B+B). The single-spin partition function and the probabilities are

    q=eβB+e−βBp↑=eβBeβB+e−βBp↓=e−βBeβB+e−βBq = e^{\beta B} + e^{-\beta B} \qquad p_\uparrow = \frac{e^{\beta B}}{e^{\beta B} + e^{-\beta B}} \qquad p_\downarrow = \frac{e^{-\beta B}}{e^{\beta B} + e^{-\beta B}}

    Try it: worked example

    Find the net magnetisation m of N non-interacting spins in a field B.

    Show answer and steps

    Answerm = N tanh(beta B).

    1. The magnetisation is the number up minus the number down: m=N↑−N↓m = N_\uparrow - N_\downarrow.
    2. With NN spins, N↑=Np↑N_\uparrow = Np_\uparrow and N↓=Np↓N_\downarrow = Np_\downarrow.
    3. So m=N(eβBeβB+e−βB−e−βBeβB+e−βB)m = N\left(\dfrac{e^{\beta B}}{e^{\beta B}+e^{-\beta B}} - \dfrac{e^{-\beta B}}{e^{\beta B}+e^{-\beta B}}\right).
    4. The two fractions share a denominator: m=N eβB−e−βBeβB+e−βBm = N\,\dfrac{e^{\beta B}-e^{-\beta B}}{e^{\beta B}+e^{-\beta B}}.
    5. That ratio is the definition of the hyperbolic tangent, so m=Ntanh⁡(βB)m = N\tanh(\beta B).
    6. Plain reading: the curve m/Nm/N against BB is S-shaped. A bigger β\beta (colder) makes it steeper and it saturates at ±1\pm 1. There is no sudden jump, so no transition.

    Mean-field turns the neighbours into an extra field

    Keep the interaction, but replace each neighbour’s spin with the average spin ⟨σ⟩\langle\sigma\rangle. dd is the number of nearest neighbours of each spin.

    E=−B∑iσi−J∑⟨ij⟩σiσj⟶E=−B∑iσi−J∑iσi⟨σ⟩dE = -B\sum_i \sigma_i - J\sum_{\langle ij\rangle}\sigma_i\sigma_j \quad\longrightarrow\quad E = -B\sum_i \sigma_i - J\sum_i \sigma_i\langle\sigma\rangle d

    Collect the terms:

    E=−(B+J⟨σ⟩d)∑iσiE = -\left(B + J\langle\sigma\rangle d\right)\sum_i \sigma_i

    This looks exactly like the non-interacting model. The neighbours act as an extra field J⟨σ⟩dJ\langle\sigma\rangle d. Now set the applied field to zero, B=0B = 0, and use ⟨σ⟩=m/N\langle\sigma\rangle = m/N:

    E=−JmdN∑iσiE = -\frac{Jmd}{N}\sum_i \sigma_i

    This is the non-interacting model with “field” Jmd/NJmd/N. Take the non-interacting answer m=Ntanh⁡(βB)m = N\tanh(\beta B) and swap in that field:

    mN=tanh⁡(βJd mN)\frac{m}{N} = \tanh\left(\beta J d\,\frac{m}{N}\right)

    The self-consistency equation has one solution when hot and three when cold

    This is an odd equation, with m/Nm/N on both sides. The lecture solves it graphically. Let x=βJd m/Nx = \beta J d\, m/N, so m/N=x kT/(Jd)m/N = x\,kT/(Jd). The equation becomes

    kTJd x=tanh⁡(x)\frac{kT}{Jd}\,x = \tanh(x)

    The left side is a straight line through the origin with slope kT/JdkT/Jd. The right side is the S-shaped tanh curve. The solutions are where they cross.

    x/2 (cold)x (T_c)2x (hot)tanh(x)x

    The sketch follows slide 10. Read it like this.

    • High TT. The line is steep (the 2x2x line). It meets the curve only at x=0x = 0, so m=0m = 0. This is the unmagnetised phase.
    • Low TT. The line is shallow (the x/2x/2 line). It meets the curve at three points: x=0x = 0 and two non-zero solutions near x≈±1.9x \approx \pm 1.9 (read from the plot). The two non-zero solutions are the magnetic phases, spin-up and spin-down. The lecture notes that x=0x = 0 is a free-energy maximum, so the system does not stay there.
    • At TcT_c. The line of slope 1 meets the curve only at 00.

    The line has slope kT/JdkT/Jd, so slope 1 means kT=JdkT = Jd:

    Tc=JdkT_c = \frac{Jd}{k}

    The slide wording is unclear here. It says the critical temperature “corresponds to m=1m = 1”, but the figure shows the xx line touching the curve only at 00 when kT/Jd=1kT/Jd = 1. This page follows the figure and the formula Tc=Jd/kT_c = Jd/k. Check the wording against the lecture recording.

    Try it: worked example

    Which line in the slide 10 figure is the cold magnet, and what are its solutions?

    Show answer and steps

    AnswerThe x/2 line, slope kT/Jd = 1/2. Three solutions: x = 0 and about x = plus or minus 1.9.

    1. The line has slope kT/JdkT/Jd. A cold magnet has small TT, so a small slope.
    2. Slopes 1/2, 1 and 2 correspond to kT/Jd=1/2kT/Jd = 1/2, 11 and 22.
    3. The shallow line (slope 1/2) cuts the S-curve near the origin and again once on each flat arm. That gives three crossings.
    4. The crossings on the arms sit at about x≈±1.9x \approx \pm 1.9 (read from the plot), meaning ∣m∣|m| is close to NN.
    5. The middle crossing, x=0x = 0, is a free-energy maximum. The system sits in one of the two outer ones.

    Mean-field gets the shape right and the numbers wrong

    Mean-field theory explains two important facts. There is a sudden transition from the magnetised to the unmagnetised phase as the Curie temperature TcT_c is crossed. And spin-down and spin-up are equally likely solutions. The limitation is stated plainly: mean-field theory is an approximation, so its numerical predictions are incorrect.

    Exam detail

    Learning outcomes on slide 23: explain the approximations and assumptions in mean-field models, and understand what mean-field theory predicts for the Ising model and the van der Waals fluid. Know the chain: EE, then mean-field EE, then m/N=tanh⁡(βJd m/N)m/N = \tanh(\beta Jd\,m/N), then Tc=Jd/kT_c = Jd/k.

    Recall

    Why does the mean-field equation have three solutions only at low temperature?

    At low TT the line kTx/(Jd)kT x/(Jd) is shallow enough to cut the tanh curve three times: at 00 and on each arm. At high TT the line is steep and cuts it only at 00.

    Check yourself

    Select all that apply