Β§6.3Quantum States of the Oscillator

Part III Phillips pp. 112–118 Β· ~17 min read

  • Hermite polynomial
  • quasi-classical state
  • zero-point energy

The ground state is not the bottom of the well. It sits above it by exactly the amount the uncertainty principle demands, and no state of this potential does better.

Β§6.2 wrote down the eigenvalue equation and stopped. This section takes its answer as given β€” the derivation waits for Β§6.6 β€” and spends its length on what the answer means.

It divides in two. First the stationary states, which turn out to carry an unusual number of exact results: the levels are evenly spaced, the eigenfunctions have a definite parity, and Ξ”x Δp\Delta x\,\Delta p comes out to (n+12)ℏ(n+\frac12)\hbar β€” hitting the uncertainty principle’s floor precisely in the ground state. Then the non-stationary states, and the question Β§6.1 left hanging: if a state of definite energy does not move, how does a quantum oscillator ever manage to look like Acos⁑(Ο‰t+Ξ±)A\cos(\omega t + \alpha)?

Stationary states

The eigenvalues, derived in Β§6.6 and quoted here, are

En=(n+12)ℏω,n=0,1,2,3,…(6.12)E_n = \left(n + \tfrac12\right)\hbar\omega,\qquad n = 0, 1, 2, 3, \dots\tag{6.12}

Equation (6.12) β€” two features, and both are unusual

symbol
is
the half is the whole story of the ground state: Eβ‚€ = Β½Δ§Ο‰, NOT zero. A classical oscillator can sit still at the bottom of the well; a quantum one cannot, and the cost is half a quantum.
units
dimensionless
type
dimensionless; n = 0, 1, 2, …

Click any symbol to see what it is, what units it carries, and what kind of object it is once you put it in an array.

Figure 6.1 β€” the ladder

energy (Δ§Ο‰)Eβ‚€ = Β½Δ§Ο‰0.50E₁ = 3⁄2 Δ§Ο‰1.50Eβ‚‚ = 5⁄2 Δ§Ο‰2.50E₃ = 7⁄2 Δ§Ο‰3.50

Click a gold level for its energy and degeneracy.

No transitions shown in this view.

Evenly spaced rungs at Δ§Ο‰, starting at Β½Δ§Ο‰ rather than at the bottom of the well. Every level is bound and there are infinitely many, because the walls of a parabola never run out.

A particle with energy EnE_n has the wave function

Ξ¨(x,t)=ψn(x) eβˆ’iEnt/ℏ(6.13)\Psi(x,t) = \psi_n(x)\,e^{-iE_nt/\hbar}\tag{6.13}

and the four lowest eigenfunctions are those of Table 6.1: a Gaussian times a polynomial, with the oscillator length a=ℏ/mΟ‰a = \sqrt{\hbar/m\omega} setting the width throughout. The polynomials are the Hermite polynomials Hn(x/a)H_n(x/a) β€” degree nn, and their nn roots are precisely the nn nodes of ψn\psi_n.

Table 6.1 β€” the four lowest eigenfunctions

n⇅energy⇅eigenfunction⇅
β“˜β“˜β“˜
β“˜β“˜β“˜
β“˜β“˜β“˜
β“˜β“˜β“˜

Click any cell for what to notice. Transcribed from page 112; each row is normalized, and the four are mutually orthogonal β€” both verified numerically below.

Figure 6.2 β€” the four lowest eigenfunctions

-6-4-20246-0.500.5position xeigenfunctionn = 0
-6-4-20246-0.500.5position xeigenfunctionn = 1
-6-4-20246-0.500.5position xeigenfunctionn = 2
-6-4-20246-0.500.5position xeigenfunctionn = 3

Solved numerically by the ch00/0.3 matrix recipe, not traced from the printed figure. Note the labels run n = 0…3: the oscillator's ground state is n = 0. Each Οˆβ‚™ has exactly n nodes, and each is even or odd about the origin.

Figure 6.3 β€” and their probability densities

-6-4-2024600.10.20.30.40.50.60.7position xeigenfunctionn = 0
-6-4-2024600.10.20.30.40.50.60.7position xeigenfunctionn = 1
-6-4-2024600.10.20.30.40.50.60.7position xeigenfunctionn = 2
-6-4-2024600.10.20.30.40.50.60.7position xeigenfunctionn = 3

|Οˆβ‚™(x)|Β², the same four states. The density spreads as n grows, and it is non-zero beyond the classical turning points in every one of them.

What is observable about a state of definite energy

Parity. Because H^\hat H is unchanged under xβ†’βˆ’xx \to -x, each eigenfunction has a definite symmetry:

ψn(βˆ’x)=+ψn(x)Β Β (nΒ even),ψn(βˆ’x)=βˆ’Οˆn(x)Β Β (nΒ odd)\psi_n(-x) = +\psi_n(x)\ \ (n\text{ even}),\qquad \psi_n(-x) = -\psi_n(x)\ \ (n\text{ odd})

Even nn has positive parity , odd nn negative. This is the same property problem 1 of chapter 5 introduced for a symmetric well, and for the same reason: a symmetry of the Hamiltonian becomes a label on its eigenstates.

The density does not move.

∣Ψn(x,t)∣2=∣ψn(x)∣2(6.14)|\Psi_n(x,t)|^2 = |\psi_n(x)|^2\tag{6.14}

The time factor eβˆ’iEnt/ℏe^{-iE_nt/\hbar} has modulus 1, so it cancels β€” exactly as in Β§4.6. And unlike a classical particle, which is confined to βˆ’A<x<A-A < x < A, the quantum particle has non-zero probability everywhere.

Position and momentum. For the nn-th state,

⟨x⟩=0,⟨x2⟩=(n+12)a2,Ξ”x=n+12 a\langle x\rangle = 0,\qquad \langle x^2\rangle = \left(n+\tfrac12\right)a^2,\qquad \Delta x = \sqrt{n+\tfrac12}\,a ⟨p⟩=0,⟨p2⟩=(n+12)ℏ2a2,Ξ”p=n+12 ℏa\langle p\rangle = 0,\qquad \langle p^2\rangle = \left(n+\tfrac12\right)\frac{\hbar^2}{a^2},\qquad \Delta p = \sqrt{n+\tfrac12}\,\frac{\hbar}{a}

and therefore

Ξ”x Δp=(n+12)ℏ\Delta x\,\Delta p = \left(n + \tfrac12\right)\hbar

The energy divides equally. Because both xx and pp are uncertain, so are the potential and kinetic energies, and their expectation values are

12mΟ‰2⟨x2⟩=12Enand⟨p2⟩2m=12En\tfrac12m\omega^2\langle x^2\rangle = \tfrac12E_n\qquad\text{and}\qquad \frac{\langle p^2\rangle}{2m} = \tfrac12E_n

Half the energy is potential, half kinetic β€” in every state, exactly. Their sum is EnE_n, which is sharp even though neither part is.

Non-stationary states

Nothing above moves. To get motion, superpose:

Ξ¨(x,t)=βˆ‘n=0,1,2,…cnψn(x) eβˆ’iEnt/ℏ(6.15)\Psi(x,t) = \sum_{n=0,1,2,\dots} c_n\psi_n(x)\,e^{-iE_nt/\hbar}\tag{6.15}

This is a state of uncertain energy: measuring EE gives 12ℏω\frac12\hbar\omega with probability ∣c0∣2|c_0|^2, 32ℏω\frac32\hbar\omega with probability ∣c1∣2|c_1|^2, and so on. It is also non-stationary, because ∣Ψ∣2|\Psi|^2 now carries interference between different eigenfunctions. The interference of ψm\psi_m with ψn\psi_n oscillates at

Ο‰m,n=∣Emβˆ’Enβˆ£β„(6.16)\omega_{m,n} = \frac{|E_m - E_n|}{\hbar}\tag{6.16}

which for this spectrum is always an integer multiple of Ο‰\omega. So ∣Ψ(x,t)∣2|\Psi(x,t)|^2 can carry Ο‰\omega, 2Ο‰2\omega, 3Ο‰3\omega and so on.

Stationary states do nothing. Mixing them is what moves β€” Eqs. (6.15)–(6.17)

-50500.20.40.60.8position x (units of the oscillator length a)|Ψ(x,t)|²⟨x⟩
0123456-0.500.5Ο‰t (one classical period)⟨x⟩ / a
  • ⟨x⟩(t), from the full Ξ£ c*β‚˜cβ‚™ xβ‚˜β‚™ sum
  • A cos Ο‰t β€” the classical motion, Eq. (6.4)
⟨E⟩ / Δ§Ο‰ 1.000
Ξ”E / Δ§Ο‰ 0.500
Ξ”E / ⟨E⟩ 0.500
amplitude A / a 0.707

Two energies, so the density sloshes. Every pair of levels contributes a beat at Ο‰m,n = |Eβ‚˜ βˆ’ Eβ‚™|/Δ§, which for this potential is always an integer multiple of Ο‰ β€” so |Ξ¨|Β² is exactly periodic with period 2Ο€/Ο‰, unlike the box of Β§4.6, whose nΒ² spectrum gives it a long revival time instead.

Yet ⟨x⟩ below is a pure cosine at Ο‰ alone, with no 2Ο‰ component even for the three-level mix. That is the selection rule: the matrix xβ‚˜β‚™ is tridiagonal, so only neighbouring levels can contribute to the average position, and neighbours are always exactly Δ§Ο‰ apart.

Natural units Δ§ = m = Ο‰ = 1, so a = 1 and Eβ‚™ = n + Β½. Eigenfunctions from the stable recurrence Οˆβ‚™ = √(2/n)Β·xΒ·Οˆβ‚™β‚‹β‚ βˆ’ √((nβˆ’1)/n)Β·Οˆβ‚™β‚‹β‚‚ (no factorials, so nΜ„ = 16 is as safe as nΜ„ = 1). ⟨x⟩(t) is the full double sum over all pairs β€” the harmonics are absent because xβ‚˜β‚™ makes them zero, not because they were left out.

Why the average position oscillates at Ο‰\omega and nothing else

∣Ψ∣2|\Psi|^2 carries harmonics, so one expects ⟨x⟩\langle x\rangle to carry them too. It does not. Evaluating ⟨x(t)⟩=βˆ«Ξ¨βˆ—xΨ dx\langle x(t)\rangle = \int\Psi^*x\Psi\,\mathrm dx produces terms in cmβˆ—cnxm,neiΟ‰m,ntc_m^*c_nx_{m,n}e^{i\omega_{m,n}t} with

xm,n=βˆ«βˆ’βˆž+∞ψmβˆ—(x) xβ€‰Οˆn(x) dxx_{m,n} = \int_{-\infty}^{+\infty}\psi_m^*(x)\,x\,\psi_n(x)\,\mathrm dx

and xm,nx_{m,n} vanishes unless ∣mβˆ’n∣=1|m - n| = 1 (problem 11). Adjacent levels are exactly ℏω\hbar\omega apart, so the only surviving frequency is Ο‰\omega:

⟨x(t)⟩=Acos⁑(Ο‰t+Ξ±),⟨p(t)⟩=βˆ’mΟ‰Asin⁑(Ο‰t+Ξ±)(6.17)\langle x(t)\rangle = A\cos(\omega t + \alpha),\qquad \langle p(t)\rangle = -m\omega A\sin(\omega t + \alpha)\tag{6.17}

Quasi-classical states

Equation (6.17) says the average moves like a classical oscillator, but says nothing about the spread around that average, which may be large and may change through the cycle. The states that look most classical are the quasi-classical states , with energy amplitudes following a Poisson distribution:

∣cn∣2=nˉ nn!eβˆ’nΛ‰,nˉ≫1|c_n|^2 = \frac{\bar n^{\,n}}{n!}e^{-\bar n},\qquad \bar n \gg 1

Using the mean and standard deviation of the Poisson distribution from problem 1 of chapter 3,

⟨E⟩=(nΛ‰+12)ℏω,Ξ”E=nˉ ℏω\langle E\rangle = \left(\bar n + \tfrac12\right)\hbar\omega,\qquad \Delta E = \sqrt{\bar n}\,\hbar\omega

so the relative energy uncertainty is

Ξ”E⟨E⟩=nΛ‰nΛ‰+12⟢1nΛ‰\frac{\Delta E}{\langle E\rangle} = \frac{\sqrt{\bar n}}{\bar n + \frac12} \longrightarrow \frac{1}{\sqrt{\bar n}}

Where this goes next

Β§6.4 puts these results to work on a real system: two nuclei vibrating in a chemical bond, where ℏω\hbar\omega becomes an infrared photon and Eq. (6.12) becomes a way of weighing the bond. Then Β§6.5 takes the oscillator into three dimensions, where the evenly spaced ladder acquires degeneracies. Β§6.6 finally derives Eq. (6.12), by an algebraic method that will reappear in chapter 8 as the whole theory of angular momentum.

Check yourself

0 / 6 answered

  1. Select "ground state alone" in the widget and press play.

    1.Nothing moves. What is the wave function doing while nothing moves?

  2. 2.Why is exactly, and not merely close to it, in the oscillator's ground state?

  3. Switch to "Οˆβ‚€ + Οˆβ‚ + Οˆβ‚‚" and look at the lower panel.

    3. visibly carries a component, yet is a clean cosine at . Why?

  4. Switch to "quasi-classical" and drag nΜ„ from 0.5 up to 16.

    4. grows as β€” it gets *bigger*. In what sense is the state becoming more classical?

  5. 5.A superposition in a box eventually reassembles after a long revival time; an oscillator superposition repeats every exactly. What is responsible?

  6. 6.In every oscillator eigenstate, and each equal . What is the classical counterpart, and where does the analogy fail?