Nothing is added to the Hamiltonian and the particles still avoid each other. The whole effect comes from a requirement on the wave functionβs symmetry, and from nothing physical at all.
Two identical billiard balls are still two different billiard balls: you can watch them, and say which is which. Quantum particles cannot be watched β ch02 removed the trajectory β so identical quantum particles are not merely hard to tell apart. They are indistinguishable in principle, and that single sentence, taken seriously, produces the Pauli principle, the rigidity of matter and the laser.
Β§10.1 turns the sentence into an equation in about half a page. Β§10.2 spends four pages on what it costs, and the answer is startling: identical particles cluster together or avoid each other with no force acting between them.
The argument: three lines, and no third option
Take two particles and , described by a two-particle wave function . The joint probability of finding in at and in at is
If the particles are identical, no measurement can tell β here, thereβ from β here, thereβ. The two must be equally probable:
Two complex numbers with the same modulus differ by a phase, so
and now the argument closes on itself.
So every acceptable wave function for two identical particles identical particles Particles of the same species. In classical physics they can be told apart by watching their trajectories; in quantum physics there are no trajectories, so they are genuinely indistinguishable and any labelling of them must have no physical consequence. defined in ch. 10 β open in glossary is either symmetric symmetric state Ξ¨(a,b) = +Ξ¨(b,a). Required of identical bosons. Any number of bosons may share one single-particle state, and two in the same place are twice as likely as two distinguishable particles would be. defined in ch. 10 β open in glossary
or antisymmetric antisymmetric state Ξ¨(a,b) = βΞ¨(b,a). Required of identical fermions. It vanishes identically if two particles occupy the same single-particle state β which is the Pauli exclusion principle β and it is exactly zero when the two particles are at the same point. defined in ch. 10 β open in glossary
These are said to have definite exchange symmetry exchange symmetry The behaviour of a state when two identical particles are swapped. Consistency of probability forces the wave function to be either unchanged (symmetric) or sign-reversed (antisymmetric) β Eq. (10.4) shows there is no third possibility. defined in ch. 10 β open in glossary . Nature will turn out to assign one or the other by species, and never to mix them β but that is Β§10.4βs news, and it is empirical. What Β§10.1 establishes is only that the choice is binary.
What it costs: two particles in one oscillator
Β§10.2 takes the simplest system that can show the effect β two identical particles of mass in the same one-dimensional oscillator, with no interaction between them at all:
Read that Hamiltonian carefully, because everything below depends on what is absent from it. There is no anywhere. The two particles do not push, pull, scatter or notice each other. Each independently occupies an oscillator eigenfunction with (problem 2 verifies this by substitution).
Both particles in the same state β and Pauli arrives four pages early
If both sit in state , the total energy is and the wave function is
Swap and : nothing changes. The state is symmetric, and it is the only one available β there is no way to build an antisymmetric function out of one single-particle state, because the antisymmetric combination of with itself is .
So: particles requiring antisymmetric wave functions can never share a single-particle state. That is the Pauli exclusion principle pauli exclusion principle At most one fermion per single-particle state. It is not an extra postulate: a state occupied by two identical fermions would have to be symmetric under their exchange, and fermions require antisymmetric states, so such a state is identically zero. defined in ch. 10 β open in glossary , and it has arrived here as a triviality β not as a postulate, not as a rule imposed on the theory, but as the observation that the state you were trying to build is the zero vector. It has no wave function because it is not a state.
Two different states β and the particles become entangled whether you like it or not
With one particle in and one in , the energy is . For distinguishable particles you could write
or any combination of them,
with the probability that is in state , and that is. Eq. (10.11) is an entangled state entangled state A joint state of two or more particles that cannot be written as a product of separate single-particle states β both particles are associated with both states at once. Introduced in ch01 for photon polarization and formalised in ch10, where it turns out that identical particles occupying different single-particle states are NECESSARILY entangled, since only an entangled combination can have definite exchange symmetry. defined in ch. 1 β open in glossary β both particles associated with both states β and the book coins untangled untangled state The book's term for a plain product wave function such as Ο_n(x_p)Ο_nβ²(x_q), available only to distinguishable particles. Identical particles in different states cannot have one. defined in ch. 10 β open in glossary for the plain products (10.9) and (10.10). For distinguishable particles, which one you get depends on how the state was prepared.
For identical particles there is no choice. Neither (10.9) nor (10.10) has definite exchange symmetry β swapping the arguments turns one into the other β so neither is acceptable. Only the two symmetric combinations survive:
The punchline: put both particles at the same place
Set in each. The untangled functions give , and the two terms of (10.12) and (10.13) become identical, so
Square them. Identical particles with a symmetric wave function are twice as likely to be found at the same point as distinguishable ones; identical particles with an antisymmetric wave function are never found at the same point. The mechanism is interference β constructive in one case, destructive in the other β and the destructive case is total, because at the two terms are not merely similar but exactly equal.
Two views make this concrete. The plane shows over both positions at once, with the dashed line marking ; exchange is reflection across that line, so βsymmetricβ and βantisymmetricβ become properties you can simply look at. The separation view integrates along that line to reproduce Fig. 10.1. Set both quantum numbers equal with antisymmetry selected and the whole map goes blank β that is the exclusion principle, drawn.
Look along the dashed diagonal. Ξ¨ is exactly zero there, because a function equal to minus its own mirror image must vanish on the mirror. That is the Fermi hole: two identical fermions are never found at the same point β and nothing in the Hamiltonian pushes them apart.
The gap that opens along the diagonal in the antisymmetric case has a standard name the book does not use: the Fermi hole fermi hole The region of zero probability along x_p = x_q in an antisymmetric two-particle state β two identical fermions are never found at the same point. The site uses the standard name; the book describes the effect without naming it. It is not caused by any force: the Hamiltonian of Eq. (10.7) has no interaction term, and all three states of Β§10.2 have the same energy. defined in ch. 10 β open in glossary . Its cause is worth being precise about, because the obvious explanation is wrong.
How far apart do they sit?
Take the bookβs own example, and , and change variables to the separation and the centre of mass,
Table 6.1βs eigenfunctions then collapse into a strikingly simple pair:
The difference between them is one factor: carries , and carries . That is the whole story in one symbol β the antisymmetric state has a factor of the separation multiplying it, so it must vanish when the separation does.
Integrating over all leaves the probability of a separation of magnitude between and :
These are the three curves of Fig. 10.1, and the separation view of the widget above draws them from the wave function rather than from these formulas β the two agree to .
Where this is going
The chapterβs own introduction says these concepts βneed not be studied in detail in order to understand atoms which is the topic covered in Chapter 11β. Treat that disclaimer with suspicion. Chapter 11 is the periodic table, and the periodic table is the exclusion principle established above; Hundβs rules are the exchange integral of problem 3. This section is load-bearing for everything that follows it.
Still missing is the physical input. Nothing so far says which particles get Eq. (10.5) and which get Eq. (10.6) β the mathematics permits both and chooses neither. Β§10.3 brings in spin and finds that the spatial symmetry and the spin symmetry are locked together, and Β§10.4 gives the empirical rule that ties the choice to spin itself.
Check yourself
0 / 6 answered
1.Eq. (10.4) allows the exchange phase only the values and . What rules out, say, ?
2.Two identical particles occupy two *different* single-particle states. What does exchange symmetry force?
The Hamiltonian of Eq. (10.7) is a sum of two independent oscillator Hamiltonians, with no term coupling to .
3.So what makes identical bosons cluster and identical fermions avoid each other?
4.Two identical particles requiring antisymmetric wave functions are put into the *same* single-particle state . What is the resulting wave function?
5.Over what range must Eqs. (10.14)β(10.16) be integrated to give 1?
6.The chapter opens by saying its concepts "need not be studied in detail in order to understand atoms which is the topic covered in Chapter 11". How should you take that?