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2.4. Molecular Partition Functions

Course-wide Conventions & Notation

Overview and Learning Objectives

Molecular partition functions extend the canonical framework from a single particle to many particles, and then to molecules with internal degrees of freedom. This section shows how distinguishability affects counting (and therefore QQ), introduces the 1/N!1/N! correction for identical particles, and motivates factorization into translational, rotational, vibrational, and electronic contributions.

In Sections 2.2 and 2.3, we derived the canonical partition function and ensemble averages for single-particle systems. Here we extend these ideas to closed systems of many identical, independent particles with internal degrees of freedom. We also introduce indistinguishability, which is central to quantum statistical mechanics.

Learning objectives:

Core Ideas and Derivations

Partition Function for Distinguishable Particles

The energy EE of an NN-particle microstate is the sum of the one-particle energies for the occupied states:

El=εia+εjb+εkc+⋯E_l = \varepsilon_i^a + \varepsilon_j^b + \varepsilon_k^c + \cdots

Here i,j,k,…i, j, k, \ldots index the one-particle microstates occupied by particles a,b,c,…a, b, c, \ldots, and ll indexes the corresponding NN-particle microstate of the system.

The canonical partition function QQ for NN distinguishable, independent particles is given by the sum over all possible microstates:

Q=∑le−βEl=∑i=1M∑j=1M∑k=1M⋯exp⁡ ⁣[−β(εia+εjb+εkc+⋯ )]=(∑i=1Me−βεia)(∑j=1Me−βεjb)(∑k=1Me−βεkc)⋯=qaqbqc⋯\begin{aligned} Q &= \sum_l e^{-\beta E_l} \\ &= \sum_{i = 1}^M \sum_{j = 1}^M \sum_{k = 1}^M \cdots \exp\!\left[-\beta\left(\varepsilon_i^a + \varepsilon_j^b + \varepsilon_k^c + \cdots\right)\right] \\ &= \left(\sum_{i = 1}^M e^{-\beta \varepsilon_i^a}\right) \left(\sum_{j = 1}^M e^{-\beta \varepsilon_j^b}\right) \left(\sum_{k = 1}^M e^{-\beta \varepsilon_k^c}\right)\cdots \\ &= \boxed{q_a q_b q_c \cdots} \end{aligned}

where qaq_a, qbq_b, and qcq_c are the canonical partition functions for the particles aa, bb, and cc, respectively.

If the particles share the same one-particle spectrum so that qa=qb=qc=⋯=qq_a=q_b=q_c=\cdots=q, then

Q=qN.Q = q^N.

Partition Function for Indistinguishable Particles

If the particles are indistinguishable and identical, we can write the canonical partition function as

Q=qNN!.Q = \frac{q^N}{N!}.

Partition Function for Molecules

Within the Born–Oppenheimer approximation, the total energy of a molecule is given by the sum of the translational, rotational, vibrational, and electronic energies:

ελ=εitrans+εjrot+εkvib+εmelec\varepsilon_{\lambda} = \varepsilon_i^{\mathrm{trans}} + \varepsilon_j^{\mathrm{rot}} + \varepsilon_k^{\mathrm{vib}} + \varepsilon_m^{\mathrm{elec}}

where ii, jj, kk, and mm are the indices of the (one-degree-of-freedom) microstates of the translational, rotational, vibrational, and electronic energies, respectively, and λ\lambda is the index of the (many-degree-of-freedom) microstate of the molecule.

The canonical partition function qq for a molecule is given by the sum over all possible microstates:

q=∑λe−βελ=∑i∑j∑k∑mexp⁡ ⁣[−β(εitrans+εjrot+εkvib+εmelec)]=∑ie−βεitrans∑je−βεjrot∑ke−βεkvib∑me−βεmelec=qtrans qrot qvib qelec.\begin{aligned} q &= \sum_{\lambda} e^{-\beta \varepsilon_{\lambda}} \\ &= \sum_{i} \sum_{j} \sum_{k} \sum_{m} \exp\!\left[-\beta\left(\varepsilon_i^{\mathrm{trans}} + \varepsilon_j^{\mathrm{rot}} + \varepsilon_k^{\mathrm{vib}} + \varepsilon_m^{\mathrm{elec}}\right)\right] \\ &= \sum_{i} e^{-\beta \varepsilon_i^{\mathrm{trans}}} \sum_{j} e^{-\beta \varepsilon_j^{\mathrm{rot}}} \sum_{k} e^{-\beta \varepsilon_k^{\mathrm{vib}}} \sum_{m} e^{-\beta \varepsilon_m^{\mathrm{elec}}} \\ &= q_{\mathrm{trans}}\,q_{\mathrm{rot}}\,q_{\mathrm{vib}}\,q_{\mathrm{elec}}. \end{aligned}

where qtransq_{\mathrm{trans}}, qrotq_{\mathrm{rot}}, qvibq_{\mathrm{vib}}, and qelecq_{\mathrm{elec}} are the canonical partition functions for the translational, rotational, vibrational, and electronic energies, respectively.

Worked Example

Counting microstates and the 1/N!1/N! factor (single occupancy)

Two particles occupy M=4M=4 one-particle microstates, with at most one particle per microstate.

  1. Distinguishable particles

    The number of distinct arrangements (permutations) is

    Wdist=M!(M−N)!=4!2!=12.W_{\mathrm{dist}}=\frac{M!}{(M-N)!}=\frac{4!}{2!}=12.
  2. Indistinguishable particles

    Exchanging labels does not create a new microstate, so

    Windist=1N!M!(M−N)!=12⋅12=6.W_{\mathrm{indist}}=\frac{1}{N!}\frac{M!}{(M-N)!}=\frac{1}{2}\cdot 12=6.
  3. Connection to partition functions

    If each allowed arrangement has the same energy E0E_0, then the canonical partition function is proportional to the count:

    Qdist=Wdist e−βE0,Qindist=Windist e−βE0=Qdist2!.Q_{\mathrm{dist}} = W_{\mathrm{dist}}\,e^{-\beta E_0},\qquad Q_{\mathrm{indist}} = W_{\mathrm{indist}}\,e^{-\beta E_0}=\frac{Q_{\mathrm{dist}}}{2!}.

Result. The 1/N!1/N! factor corrects overcounting for identical particles and changes the thermodynamics derived from ln⁡Q\ln Q.

Concept Checks

  1. What physical experiment would fail to distinguish two microstates that differ only by swapping particle labels?

  2. Why does QQ factorize for independent particles but not for interacting particles?

  3. What assumption about occupancy is built into the combinatorial formulas in this section?

  4. How would the counting change if multiple occupancy were allowed?

Key Takeaways