(8.1) |
(8.2) |
One of the fundamental postulates of quantum mechanics is the essential indistinguishability of particles of the same species. What this means, in practice, is that we cannot label particles of the same species. In other words, a proton is just a proton--we cannot meaningfully talk of proton number 1, or proton number 2, et cetera. Note that no such constraint arises in classical mechanics. Thus, in classical mechanics, particles of the same species are regarded as being distinguishable, and can, therefore, be labelled. Of course, the quantum-mechanical approach is the correct one.
Suppose that we interchange the th and th particles: that is,
(8.3) | ||
(8.4) |
Suppose that we interchange the th and th particles a second time. Swapping the th and th particles twice leaves the system completely unchanged. In other words, it is equivalent to doing nothing at all to the system. Thus, the wavefunctions before and after this process must be identical. It follows from Equation (8.6) that
(8.7) |
We conclude, from the previous discussion, that the wavefunction, , is either completely symmetric under the interchange of identical particles, or it is completely anti-symmetric. In other words, either
In 1940, the Nobel prize-winning physicist Wolfgang Pauli demonstrated, via arguments involving relativistic invariance, that the wavefunction associated with a collection of identical integer-spin (i.e., spin , etc.) particles satisfies Equation (8.8), whereas the wavefunction associated with a collection of identical half-integer-spin (i.e., spin , etc.) particles satisfies Equation (8.9). The former type of particles are known as bosons [after the Indian physicist S.N. Bose, who first put forward Equation (8.8) on empirical grounds]. The latter type of particles are called fermions (after the Italian physicist Enrico Fermi, who first studied the properties of fermion gases). Common examples of bosons are photons and atoms. Common examples of fermions are protons, neutrons, and electrons.
Consider a gas made up of identical bosons. Equation (8.8) implies that the interchange of any two particles does not lead to a new state of the system. Bosons must, therefore, be considered as genuinely indistinguishable when enumerating the different possible states of the gas. Note that Equation (8.8) imposes no restriction on how many particles can occupy a given single-particle quantum state, .
Consider a gas made up of identical fermions. Equation (8.9) implies that the interchange of any two particles does not lead to a new physical state of the system (because is invariant). Hence, fermions must also be considered genuinely indistinguishable when enumerating the different possible states of the gas. Consider the special case where particles and lie in the same quantum state. In this case, the act of swapping the two particles is equivalent to leaving the system unchanged, so
(8.11) |
Consider, for the sake of comparison, a gas made up of identical classical particles. In this case, the particles must be considered distinguishable when enumerating the different possible states of the gas. Furthermore, there are no constraints on how many particles can occupy a given quantum state.
According to the previous discussion, there are three different sets of rules that can be used to enumerate the states of a gas made up of identical particles. For a boson gas, the particles must be treated as being indistinguishable, and there is no limit to how many particles can occupy a given quantum state. This set of rules is called Bose-Einstein statistics, after S.N. Bose and A. Einstein, who first developed them. For a fermion gas, the particles must be treated as being indistinguishable, and there can never be more than one particle in any given quantum state. This set of rules is called Fermi-Dirac statistics, after E. Fermi and P.A.M. Dirac, who first developed them. Finally, for a classical gas, the particles must be treated as being distinguishable, and there is no limit to how many particles can occupy a given quantum state. This set of rules is called Maxwell-Boltzmann statistics, after J.C. Maxwell and L. Boltzmann, who first developed them.