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Consider a gas consisting of
identical non-interacting particles
occupying volume
and in thermal equilibrium at temperature
.
Let us label the possible quantum states of a single particle by
(or
).
Let the energy of a particle in state
be denoted
.
Let the number of particles in state
be written
. Finally,
let us label the possible quantum states of the whole gas by
.
The particles are assumed to be non-interacting, so the
total energy of the gas in state
, where there are
particles
in quantum state
, etc., is simply
 |
(579) |
where the sum extends over all possible quantum states
. Furthermore,
since the total number of particles in the gas is known to be
, we must
have
 |
(580) |
In order to calculate the thermodynamic properties of the gas (i.e.,
its internal energy or its entropy), it is necessary to
calculate its partition function,
 |
(581) |
Here, the sum is over all possible states
of the whole gas:
i.e., over all the various possible values of the
numbers
.
Now,
is
the relative probability of finding the gas in a particular state in which
there are
particles in state 1,
particles in state 2, etc.
Thus, the mean number of particles in quantum state
can be written
![\begin{displaymath}
\bar{n}_s = \frac{\sum_R n_s\,\exp[-\beta\,(n_1\,\epsilon_1+...
...sum_R \exp[-\beta\,(n_1\,\epsilon_1+n_2\,\epsilon_2+\cdots)]}.
\end{displaymath}](img1387.png) |
(582) |
A comparison of Eqs. (581) and (582) yields the result
 |
(583) |
Here,
.
Next: Fermi-Dirac statistics
Up: Quantum statistics
Previous: An illustrative example
Richard Fitzpatrick
2006-02-02