Inverse temperature

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It is often convenient to define a dimensionless inverse temperature, β:

β:=1kBT

This notation likely comes from its origin as a Lagrangian multiplier, for which Greek letters are customarily written.

Indeed, it shown in Ref. 1 (pp. 79-85) that this is the way it enters. The task is to maximize number of ways $N$ particles may be asigned to $K$ space-momentum cells, such that one has a set of occupation numbers ni. Introducing the partition function:

Ω∝N!n1!n2!…nK!,

one could maximize its logarithm (a monotonous function):

logΩ≈logN−N−∑i(logni+ni)+consts,

where Stirling's approximation for large numbers has been used. The maximization must be performed subject to the constraint:

∑ini=N

An additional constraint, which applies only to dilute gases, is:

∑iniei=E,

where E is the total energy and ei=pi2/2m is the energy of cell i.

The method of Lagrange multipliers entails finding the extremum of the function

L=logΩ−α(∑ini−N)−β(∑iniei−E),

where the two Lagrange multipliers enforce the two conditions and permit the treatment of the occupations as independent variables. The minimization leads to

ni=Ce−βei,

and an application to the case of an ideal gas reveals the connection with the temperature,

β:=1kBT.

Similar methods are used for quantum statistics of dilute gases (Ref. 1, pp. 179-185).

References

  1. Kerson Huang, "Statistical Physics" John Wiley and Sons, second edition (1987) ISBN 978-0-471-81518-1