Quantum Mechanics, Volume 3. Claude Cohen-Tannoudji

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      (40)

Multiplying by 1/[1 — e^{–β (ei – μ)}] the product at the end of the right-hand side of (36) yields the partition function Z, which cancels out the first factor 1/Z. We are then left with:

(41)

This result proves that (35) remains valid even in the case i = j.

       β. Physical discussion: occupation number fluctuations

      For two different physical states i and j, the average value for an ideal gas is simply equal to the product of the average values and ; this is a consequence of the total absence of interaction between the particles. The same is true for the average value .

Now if i = j, we note the factor 2 in relation (41). As we now show, this factor leads to the presence of strong fluctuations associated with the operator , the particle number in the state . The calculations shows that:

(42a)

      The square of the root mean square deviation Δni, is therefore given by:

      (42b)

The fluctuations of this operator are therefore larger than its average value, which implies that the population of each state |ui〉 is necessarily poorly defined¹ at thermal equilibrium. This is particularly true for large : in an ideal boson gas, a largely populated individual state is associated with a very large population fluctuation. This is due to the shape of the Bose-Einstein distribution (24), a decreasing exponential which is maximum at the origin: the most probable occupation number is always ni = 0. Hence it is impossible to get a very large average without introducing a distribution spreading over many ni values. Complement H_XV (§ 4-a) discusses certain consequences of these fluctuations for an ideal gas. It also shows that as soon as a weak repulsive particle interaction is introduced, the fluctuations greatly diminish and almost completely disappear, since their presence would lead to a very large increase in the potential energy.

3-c. Common expression

      To summarize, we can write in all cases:

(43)

      with:

      (44)

As shown in relation (C-19) of Chapter XV, this average value is simply the matrix element 〈1 : uk; 2 : ul1 : ui; 2 : uj〉 of the two-particle reduced density operator. To get the general expression for the average of any symmetric two-particle operator, we simply use (43) in (28). Consequently, for independent particles, the average values of all these operators are simply expressed in terms of the quantum Fermi-Dirac and Bose-Einstein distribution functions.

      Complement C_XVI will show how the Wick theorem allows generalizing these results to operators dealing with any number of particles.

4. Total number of particles

      The operator corresponding to the total number of particles is given by the sum over all the individual states:

      (45)

      and its average value is given by:

(46)

      As fβ increases as a function of μ, the total number of particles is controlled (for fixed β) by the chemical potential.

4-a. Fermions

For the sake of simplicity, we study the ideal gas properties without taking into account the spin, which assumes that all particles are in the same spin state (the spin can easily be accounted for by adding the contributions of the different individual spin states). For a large physical system, the energy levels are very close and the discrete sum in (46) can be replaced by an integral. This leads to:

(47)

      where the function is defined as (the subscript ig stands for ideal gas):

(48)

Figure 2 shows the variations of the function as a function of μ, for fixed values of β

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