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Statistical Mechanics: Ensembles

Microcanonical, canonical, grand canonical — and why they agree at large N.

Statistical mechanics counts microstates. Three principal ensembles:

  • Microcanonical $(N,V,E)$: $S = k_B \ln\Omega$.
  • Canonical $(N,V,T)$: $Z = \sum_n e^{-\beta E_n}$, $\beta = 1/k_BT$.
  • Grand canonical $(\mu,V,T)$: $\Xi = \sum_N e^{\beta\mu N} Z_N$.

Helmholtz free energy $F = -k_BT \ln Z$, mean energy $\langle E\rangle = -\partial_\beta \ln Z$. Relative fluctuations vanish as $1/\sqrt N$, so all ensembles agree in the thermodynamic limit.

Interactive: Boltzmann distribution

Probability $p(E) \propto e^{-\beta E}$ for energy levels $E_n = n$. Adjust temperature to see the population shift.

Quiz

1. Canonical partition function:
2. Helmholtz free energy:
3. Relative fluctuations in the canonical ensemble scale as:
4. Equipartition theorem: each quadratic degree of freedom contributes (classically) to the mean energy:
5. Boltzmann's entropy formula is: