Occupation number


The occupation number nn of a quantum state is the number of particles in that state at a given time. Its behavior differs between kinds of quantum particles. For fermions, it is either 0 or 1, as the Pauli exclusion principle prevents multiple fermions from occupying the same state. For bosons, it is can be any natural number, from 0 to infinity. In symbols,

n={0,1for fermions0,1,2,for bosonsn=\begin{cases} 0,1\quad&\text{for fermions} \\ 0,1,2,\ldots \quad&\text{for bosons} \end{cases}

For a system of NN particles, occupation numbers satisfy

ini=N\sum_{i}n_{i}=N

where ii is some label used to distinguish the states (usually a quantum number).

Average occupation

For an example, consider a system with a discrete energy spectrum {εk}k\{ \varepsilon_{k} \}_{k}. There are infinite discrete energy eigenstates, each labelled by a quantum number kk. Each energy state εk\ket{\varepsilon_{k}} is simultaneously occupied by a number of particles nkn_{k}. Due to the Pauli exclusion principle, this is 0 or 1 for fermions and any natural number for bosons.

If we take the particles to be non-interacting, the canonical partition function of the system can be calculated as follows1:

Z={nk}eβkεknk=knkeβεknkZ=\sum_{\{ n_{k} \}}e^{-\beta \sum_{k}\varepsilon_{k}n_{k}}=\prod_{k}\sum_{n_{k}}e^{-\beta\varepsilon_{k}n_{k}}

What values nkn_{k} can take depends on the kind of particle:

ZF=knk=01eβεknk=k(1+eβεk)Z_{F}=\prod_{k}\sum_{n_{k}=0}^{1}e^{-\beta \varepsilon_{k} n_{k}}=\prod_{k}(1+e^{-\beta \varepsilon_{k}}) ZB=knk=0eβεknk=k11+eβεkZ_{B}=\prod_{k}\sum_{n_{k}=0}^{\infty} e^{-\beta \varepsilon_{k}n_{k}}=\prod_{k} \frac{1}{1+e^{-\beta \varepsilon_{k}}}

where we used the geometric series for bosons. The average occupation number for a certain quantum number kˉ\bar{k} therefore is

nkˉ=1Zknknkˉeβnkεk=knkˉ=01 or nkˉeβnkεkknkˉ=01 or eβnkεk=\langle n_{\bar{k}} \rangle =\frac{1}{Z}\prod_{k}\sum_{n_{k}}n_{\bar{k}}e^{-\beta n_{k}\varepsilon_{k}}=\frac{\prod_{k}\sum_{n_{\bar{k}}=0}^{1\text{ or }\infty}n_{\bar{k}}e^{-\beta n_{k}\varepsilon_{k}}}{\prod_{k}\sum_{n_{\bar{k}}=0}^{1\text{ or }\infty} e^{-\beta n_{k}\varepsilon_{k}}}=\ldots

but all the kk's in the product except kˉ\bar{k} simplify with the denominator, as for them, nkˉ=1n_{\bar{k}}=1:

=Z1Z2nkˉ=0nkˉeβnkεkZ1Z2Zkˉ=1nk=01 or eβnkεknkˉ=01 or nkˉeβnkˉEkˉ\ldots=\frac{\cancel{ Z_{1} }\cancel{ Z_{2} }\ldots\sum_{n_{\bar{k}}=0}^{\infty}n_{\bar{k}}e^{-\beta n_{k}\varepsilon_{k}}\ldots}{\cancel{ Z_{1} }\cancel{ Z_{2} }\ldots Z_{\bar{k}}\ldots}= \frac{1}{\sum_{n_{\overline{k}}=0}^{1\text{ or }\infty} e^{-\beta n_{\overline{k}}\varepsilon_{\overline{k}}}}\sum_{n_{\bar{k}}=0}^{1\text{ or }\infty} n_{\bar{k}}e^{-\beta n_{\bar{k}}E_{\bar{k}}}

For fermions, it becomes

nk=eβεk1+eβεk=1eβεk+1\langle n_{k} \rangle =\frac{e^{-\beta \varepsilon_{k}}}{1+e^{-\beta \varepsilon_{k}}}=\frac{1}{e^{\beta \varepsilon_{k}}+1}

This is the Fermi-Dirac distribution. For bosons, it becomes

nk=111eβεknk=0nkeβnkεk=(1eβεk)(βεk)nk=0eβnkεk=(1eβεk)(βεk)11+eβεk=1eβεk1\begin{align} \langle n_{k} \rangle &=\frac{1}{\frac{1}{1-e^{\beta \varepsilon_{k}}}} \sum_{n_{k}=0}^{\infty} n_{k}e^{-\beta n_{k}\varepsilon_{k}} \\ &=(1-e^{\beta \varepsilon_{k}}) \frac{ \partial }{ \partial (\beta \varepsilon_{k}) } \sum_{n_{k}=0}^{\infty} e^{-\beta n_{k}\varepsilon_{k}} \\ &=(1-e^{\beta \varepsilon_{k}}) \frac{ \partial }{ \partial (\beta \varepsilon_{k}) } \frac{1}{1+e^{-\beta \varepsilon_{k}}} \\ &=\frac{1}{e^{\beta \varepsilon_{k}}-1} \end{align}

This is the Bose-Einstein distribution respectively. Combined, we can write

nk=1eβεk±1\boxed{\langle n_{k} \rangle =\frac{1}{e^{\beta \varepsilon_{k}}\pm 1}}

The sign is determined the kind of particle in play.

Footnotes

  1. The exponential of a sum makes a product, since ea+b=eaebe^{a+b}=e^{a}e^{b}, so exp(knk)=kexp(nk)\exp\left( \sum_{k}n_{k} \right)=\prod_{k}\exp(n_{k}).