Читать книгу Quantum Mechanics, Volume 3 - Claude Cohen-Tannoudji - Страница 60

We already gave in Complement C_XIV (Figure 3) the form of the Fermi-Dirac distribution. Figure 1 shows both the variations of this distribution and the Bose-Einstein distribution. For the sake of comparison, it also includes the variations of the classical Boltzmann distribution:

(27)

which takes on intermediate values between the two quantum distributions. For a non-interacting gas contained in a box with periodic boundary conditions, the lowest possible energy e is zero and all the others are positive. Exponential e^{β (ei – μ)} is therefore always greater than e^–βμ. We are now going to distinguish several cases, starting with the most negative values for the chemical potential.

1 (i) For a negative value of βμ with a modulus large compared to 1 (i.e. for μ ≪ —kBT, which corresponds to the right-hand side of the figure), the exponential in the denominator of (25) is always much larger than 1 (whatever the energy e), and the distribution reduces to the classical Boltzmann distribution (27). Bosons and fermions have practically the same distribution; the gas is said to be “non-degenerate”.

2 (ii) For a fermion system, the chemical potential has no upper boundary, but the population of an individual state can never exceed 1. If μ is positive, with μ ≫ kBT:– for low values of the energy, the factor 1 is much larger than the exponential term; the population of each individual state is almost equal to 1, its maximum value.– if the energy ei increases to values of the order μ the population decreases and when ei ≫ μ it becomes practically equal to the value predicted by the Boltzmann exponential (27).

Most of the particles occupy, however, the individual states having an energy less or comparable to μ, whose population is close to 1. The fermion system is said to be “degenerate”.

Figure 1: Quantum distribution functions of Fermi-Dirac (for fermions, lower curve) and of Bose-Einstein (for bosons, upper curve) as a function of the dimensionless variable β(e – μ); the dashed line intermediate curve represents the classical Boltzmann distribution e^{–β (e – μ)}. In the right-hand side of the figure, corresponding to large negative values of μ, the particle number is small (the low density region) and the two distributions practically join the Boltzmann distribution. The system is said to be non-degenerate, or classical. As μ increases, we reach the central and left hand side of the figure, and the distributions become more and more different, reflecting the increasing gas degeneracy. For bosons, μ cannot be larger than the one-particle ground state energy, assumed to be zero in this case. The divergence observed for μ = 0 corresponds to Bose-Einstein condensation. For fermions, the chemical potential μ can increase without limit, and for all the energy values, the distribution function tends towards 1 (but never exceeding 1 due to the Pauli exclusion principle).

1 (iii) For a boson system, the chemical potential cannot be larger than the lowest e0 individual energy value, which we assumed to be zero. As μ tends towards zero through negative values and —kBT ≪ μ < 0, the distribution function denominator becomes very small leading to very large populations of the corresponding states. The boson gas is then said to be “degenerate”. On the other hand, for energies of the order or larger than μ, and as was the case for fermions, the boson distribution becomes practically equal to the Boltzmann distribution.

2 (iv) Finally, for situations intermediate between the extreme cases described above, the gas is said to be “partially degenerate”.