Statistical Physics by Mandl Franz
Author:Mandl, Franz [Mandl, Franz]
Language: eng
Format: epub
Publisher: Wiley
Published: 2013-05-26T22:00:00+00:00
7.3 VALIDITY CRITERION FOR THE CLASSICAL REGIME
In the last section we characterized the classical regime by the properties that most of the single-particle states are empty, a very few contain one molecule and an insignificantly small number contain more than one molecule. We now want to formulate this condition mathematically and see what it means physically.
The probability that a molecule is in a particular state s of translational motion (with energy εstr, see Eq. (7.12)) is given, according to the Boltzmann distribution (2.22), by
(7.29)
(Do not confuse ps with a momentum variable!) If the gas consists of N molecules, the mean number s of molecules which are in the translational state s is given by
(7.30)
For each translational state s, the molecule can still be in any one of many different states of internal motion. It follows that if each of the mean occupation numbers s of the translational states is very small compared to unity, the classical regime holds, i.e. we obtain as a sufficient condition for the classical regime
(7.31) for all s
From Eqs. (7.30), (7.29) and (7.19) this condition can be written
(7.32)
for all s, and this will certainly be the case if
(7.33)
Eq. (7.33) is the condition for the classical regime to hold. (It is a sufficient condition.) The inequality (7.33) would certainly hold in the limit h → 0. This is of course the classical limit used by Maxwell and Boltzmann. For this reason the statistics which were derived in sections 7.1 and 7.2 are called classical or Maxwell-Boltzmann statistics. We see from Eq. (7.33) that classical statistics will hold better at high temperatures and low densities, just as expected, so that the perfect gas laws should hold. Before obtaining quantitative estimates of the inequality (7.33), we shall rewrite it to bring out its physical meaning.
According to quantum mechanics, a particle of momentum p has associated with it a de Broglie wavelength
(7.34)
where we used Eq. (7.16) for the translational kinetic energy εtr. We shall show below (see Eq. (7.42)) that under classical conditions the mean kinetic energy of a gas molecule is
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