Β§10.1–10.2Exchange Symmetry; Physical Consequences

Part I Phillips pp. 213–219 Β· ~17 min read

  • identical particles
  • exchange symmetry
  • symmetric state
  • antisymmetric state
  • entangled state

Nothing is added to the Hamiltonian and the particles still avoid each other. The whole effect comes from a requirement on the wave function’s 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 pp and qq, described by a two-particle wave function Ξ¨(rp,rq,t)\Psi(\mathbf r_p, \mathbf r_q, t). The joint probability of finding pp in d3a\mathrm d^3a at a\mathbf a and qq in d3b\mathrm d^3b at b\mathbf b is

∣Ψ(a,b,t)∣2 d3a d3b(10.1)|\Psi(\mathbf a, \mathbf b, t)|^2\,\mathrm d^3a\,\mathrm d^3b\tag{10.1}

If the particles are identical, no measurement can tell ”pp here, qq there” from ”qq here, pp there”. The two must be equally probable:

∣Ψ(a,b,t)∣2=∣Ψ(b,a,t)∣2(10.2)|\Psi(\mathbf a, \mathbf b, t)|^2 = |\Psi(\mathbf b, \mathbf a, t)|^2\tag{10.2}

Two complex numbers with the same modulus differ by a phase, so

Ξ¨(a,b,t)=eiδ Ψ(b,a,t)(10.3)\Psi(\mathbf a, \mathbf b, t) = e^{i\delta}\,\Psi(\mathbf b, \mathbf a, t)\tag{10.3}

and now the argument closes on itself.

Why the phase has only two possible values

step 1 of 4

This is the entire content of section 10.1. It uses nothing but Eq. (10.3) and the fact that swapping twice gets you back where you started.

  1. 1Start from Eq. (10.3): exchanging the two arguments multiplies the wave function by some phase. We do not yet know what the phase is.

    The particles are identical, so the SAME phase must work whichever way round we write it β€” there is nothing to distinguish the two cases.

So every acceptable wave function for two identical particles is either symmetric

Ξ¨(a,b,t)=Ξ¨(b,a,t)(10.5)\Psi(\mathbf a, \mathbf b, t) = \Psi(\mathbf b, \mathbf a, t)\tag{10.5}

or antisymmetric

Ξ¨(a,b,t)=βˆ’Ξ¨(b,a,t)(10.6)\Psi(\mathbf a, \mathbf b, t) = -\Psi(\mathbf b, \mathbf a, t)\tag{10.6}

These are said to have definite exchange symmetry . Nature will turn out to assign one or the other by species, and never to mix them β€” but that is Β§10.4’s 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 mm in the same one-dimensional oscillator, with no interaction between them at all:

H^(xp,xq)=βˆ’β„22mβˆ‚2βˆ‚xp2βˆ’β„22mβˆ‚2βˆ‚xq2+12mΟ‰2xp2+12mΟ‰2xq2(10.7)\hat H(x_p, x_q) = -\frac{\hbar^2}{2m}\frac{\partial^2}{\partial x_p^2} -\frac{\hbar^2}{2m}\frac{\partial^2}{\partial x_q^2} +\tfrac12 m\omega^2x_p^2 + \tfrac12 m\omega^2x_q^2\tag{10.7}

Read that Hamiltonian carefully, because everything below depends on what is absent from it. There is no xpβˆ’xqx_p - x_q anywhere. The two particles do not push, pull, scatter or notice each other. Each independently occupies an oscillator eigenfunction ψn\psi_n with En=(n+12)ℏωE_n = (n + \tfrac12)\hbar\omega (problem 2 verifies this by substitution).

Both particles in the same state β€” and Pauli arrives four pages early

If both sit in state nn, the total energy is E=2En=(2n+1)ℏωE = 2E_n = (2n+1)\hbar\omega and the wave function is

Ξ¨(S)(xp,xq,t)=ψn(xp)β€‰Οˆn(xq) eβˆ’i(En+En)t/ℏ(10.8)\Psi^{(S)}(x_p, x_q, t) = \psi_n(x_p)\,\psi_n(x_q)\,e^{-i(E_n+E_n)t/\hbar}\tag{10.8}

Swap xpx_p and xqx_q: 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 ψn\psi_n with itself is ψnψnβˆ’Οˆnψn=0\psi_n\psi_n - \psi_n\psi_n = 0.

So: particles requiring antisymmetric wave functions can never share a single-particle state. That is the Pauli exclusion principle , 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 nn and one in nβ€²n', the energy is E=(n+nβ€²+1)ℏωE = (n + n' + 1)\hbar\omega. For distinguishable particles you could write

Ξ¨1(D)=ψn(xp)ψnβ€²(xq)eβˆ’i(En+Enβ€²)t/ℏ(10.9)\Psi_1^{(D)} = \psi_n(x_p)\psi_{n'}(x_q)e^{-i(E_n+E_{n'})t/\hbar}\tag{10.9} Ξ¨2(D)=ψn(xq)ψnβ€²(xp)eβˆ’i(En+Enβ€²)t/ℏ(10.10)\Psi_2^{(D)} = \psi_n(x_q)\psi_{n'}(x_p)e^{-i(E_n+E_{n'})t/\hbar}\tag{10.10}

or any combination of them,

Ξ¨(D)=c1Ξ¨1(D)+c2Ξ¨2(D)(10.11)\Psi^{(D)} = c_1\Psi_1^{(D)} + c_2\Psi_2^{(D)}\tag{10.11}

with ∣c1∣2|c_1|^2 the probability that pp is in state nn, and ∣c2∣2|c_2|^2 that qq is. Eq. (10.11) is an entangled state β€” both particles associated with both states β€” and the book coins untangled 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:

Ξ¨(S)=12[ψn(xp)ψnβ€²(xq)+ψn(xq)ψnβ€²(xp)]eβˆ’i(En+Enβ€²)t/ℏ(10.12)\Psi^{(S)} = \tfrac{1}{\sqrt2}\left[\psi_n(x_p)\psi_{n'}(x_q) + \psi_n(x_q)\psi_{n'}(x_p)\right]e^{-i(E_n+E_{n'})t/\hbar}\tag{10.12} Ξ¨(A)=12[ψn(xp)ψnβ€²(xq)βˆ’Οˆn(xq)ψnβ€²(xp)]eβˆ’i(En+Enβ€²)t/ℏ(10.13)\Psi^{(A)} = \tfrac{1}{\sqrt2}\left[\psi_n(x_p)\psi_{n'}(x_q) - \psi_n(x_q)\psi_{n'}(x_p)\right]e^{-i(E_n+E_{n'})t/\hbar}\tag{10.13}

The punchline: put both particles at the same place

Set xp=xq=x0x_p = x_q = x_0 in each. The untangled functions give ψn(x0)ψnβ€²(x0)\psi_n(x_0)\psi_{n'}(x_0), and the two terms of (10.12) and (10.13) become identical, so

Ξ¨(S)(x0,x0,t)=2β€‰Οˆn(x0)ψnβ€²(x0) eβˆ’i(En+Enβ€²)t/ℏandΞ¨(A)(x0,x0,t)=0\Psi^{(S)}(x_0,x_0,t) = \sqrt2\,\psi_n(x_0)\psi_{n'}(x_0)\,e^{-i(E_n+E_{n'})t/\hbar} \qquad\text{and}\qquad \Psi^{(A)}(x_0,x_0,t) = 0

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 xp=xqx_p = x_q the two terms are not merely similar but exactly equal.

Two views make this concrete. The plane shows ∣Ψ(x1,x2)∣2|\Psi(x_1,x_2)|^2 over both positions at once, with the dashed line marking x1=x2x_1 = x_2; exchange is reflection across that line, so β€œsymmetric” and β€œantisymmetric” 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.

Two identical particles: exchange is reflection across the diagonal
x₁ = xβ‚‚xβ‚‚x₁
max |Ξ¨| on the diagonal x₁ = xβ‚‚: 0.00000
state: n = 0 and nβ€² = 1

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 . Its cause is worth being precise about, because the obvious explanation is wrong.

How far apart do they sit?

Take the book’s own example, n=0n = 0 and nβ€²=1n' = 1, and change variables to the separation and the centre of mass,

x=xpβˆ’xqandX=xp+xq2x = x_p - x_q \qquad\text{and}\qquad X = \frac{x_p + x_q}{2}

Table 6.1’s eigenfunctions then collapse into a strikingly simple pair:

Ξ¨(S)(x,X,t)=2a2π eβˆ’x2/4a2 X eβˆ’X2/a2 eβˆ’i(E0+E1)t/ℏ\Psi^{(S)}(x,X,t) = \frac{2}{a^2\sqrt\pi}\,e^{-x^2/4a^2}\,X\,e^{-X^2/a^2}\,e^{-i(E_0+E_1)t/\hbar} Ξ¨(A)(x,X,t)=βˆ’1a2π x eβˆ’x2/4a2 eβˆ’X2/a2 eβˆ’i(E0+E1)t/ℏ\Psi^{(A)}(x,X,t) = \frac{-1}{a^2\sqrt\pi}\,x\,e^{-x^2/4a^2}\,e^{-X^2/a^2}\,e^{-i(E_0+E_1)t/\hbar}

The difference between them is one factor: Ξ¨(S)\Psi^{(S)} carries XX, and Ξ¨(A)\Psi^{(A)} carries xx. 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 ∣Ψ∣2|\Psi|^2 over all XX leaves the probability of a separation of magnitude between ∣x∣|x| and ∣x+dx∣|x + \mathrm dx|:

P(S)(x) dx=2a2π eβˆ’x2/2a2 dx(10.14)P^{(S)}(x)\,\mathrm dx = \frac{2}{a\sqrt{2\pi}}\,e^{-x^2/2a^2}\,\mathrm dx\tag{10.14} P(A)(x) dx=2a2π x2a2 eβˆ’x2/2a2 dx(10.15)P^{(A)}(x)\,\mathrm dx = \frac{2}{a\sqrt{2\pi}}\,\frac{x^2}{a^2}\,e^{-x^2/2a^2}\,\mathrm dx\tag{10.15} P(D)(x) dx=1a2Ο€(1+x2a2)eβˆ’x2/2a2 dx(10.16)P^{(D)}(x)\,\mathrm dx = \frac{1}{a\sqrt{2\pi}}\left(1 + \frac{x^2}{a^2}\right)e^{-x^2/2a^2}\,\mathrm dx\tag{10.16}

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 4Γ—10βˆ’114\times10^{-11}.

Where this is going

The chapter’s own introduction says these concepts β€œneed not be studied in detail in order to understand atoms which is the topic covered in Chapter 11”. Treat that disclaimer with suspicion. Chapter 11 is the periodic table, and the periodic table is the exclusion principle established above; Hund’s 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. 1.Eq. (10.4) allows the exchange phase only the values and . What rules out, say, ?

  2. 2.Two identical particles occupy two *different* single-particle states. What does exchange symmetry force?

  3. 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. 4.Two identical particles requiring antisymmetric wave functions are put into the *same* single-particle state . What is the resulting wave function?

  5. 5.Over what range must Eqs. (10.14)–(10.16) be integrated to give 1?

  6. 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?