Ensembles and the statistics of matter

Derive equilibrium predictions through counting, partition functions, ensemble transformations, and the distinct statistics of classical and quantum particles.

10 published lessons1 module320 min of guided study
  1. 01
    Ensembles and the statistics of matteradvanced · 10 lessons

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Ensembles and the statistics of matter

Derive equilibrium predictions through counting, partition functions, ensemble transformations, and the distinct statistics of classical and quantum particles.

  1. 01

    Count physical states in phase space

    Normalize classical counting with Planck cells and remove permutation overcounting without confusing dilution with distinguishability.

    32 min
  2. 02

    Find temperature by sharing a fixed energy

    Derive thermal equilibrium from state multiplicities and distinguish bounded-spectrum negative temperatures from ordinary cooling.

    32 min
  3. 03

    Derive Boltzmann weights from a reservoir

    Expand reservoir entropy to obtain canonical probabilities, finite-reservoir corrections, and energy-fluctuation identities.

    32 min
  4. 04

    Turn a state sum into an energy integral

    Derive density-of-states normalization and use a Laplace transform to distinguish available states from occupied states.

    32 min
  5. 05

    Let particles exchange with a reservoir

    Derive grand-canonical weights and occupation laws while distinguishing an imposed chemical potential from a fixed particle number.

    32 min
  6. 06

    Specify what ensemble equivalence means

    Connect concentration and entropy concavity to bulk equivalence while preserving finite-size correlations and constraint-dependent fluctuations.

    32 min
  7. 07

    Locate the ideal Bose condensation threshold

    Separate the ground state from the continuum and state the dimensional and thermodynamic assumptions behind a condensation temperature.

    32 min
  8. 08

    Expand about a filled Fermi sea

    Derive zero-temperature filling and controlled low-temperature corrections at fixed particle density.

    32 min
  9. 09

    Count thermal photons with zero chemical potential

    Derive Planck energy density from mode counting and connect cavity energy, isotropic pressure, and surface emission.

    32 min
  10. 10

    Read interactions through virial coefficients

    Derive the second virial correction from a pair potential and keep density truncation separate from uncontrolled dense-fluid extrapolation.

    32 min
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