2.9
The harmonic oscillator
The most reused model in physics. Solving it with ladder operators is ten times faster than grinding through the differential equation, and it shows the structure far more clearly.
Recommended first
After this section you should be able to
- Obtain the full spectrum and eigenstates with the ladder-operator method
- Explain where the zero-point energy ħω/2 comes from and why it cannot be zero
- Say why the harmonic oscillator turns up in every branch of physics
- Understand the correspondence principle by comparing the wavefunction tails with the classical distribution
Why a parabola
Expand any potential about a minimum at :
The linear term vanishes at a minimum, and the constant can be absorbed into the zero of energy. The leading surviving term is always quadratic. Set and you have a harmonic oscillator.
So any time you study “small vibrations” you are doing harmonic-oscillator physics: the vibrational spectra of diatomic molecules, phonons in a crystal, every mode of the electromagnetic field, LC circuits, the approximate description of a superconducting qubit… the list goes on.
The ladder-operator method
Grinding through the differential equation (series solution plus Hermite polynomials) certainly works, but the algebraic route is faster and far more illuminating.
Derivation: from a commutator to the entire spectrumadvanced~12 min
Step 1: factorise the Hamiltonian.
If and were ordinary numbers we could write . Operators do not commute, so the factorisation is slightly off — off by exactly the commutator. Define
Step 2: compute the commutator. Using :
Similarly . Subtracting,
and
Step 3: show that they raise and lower the energy. Suppose and consider :
Use to move all the way left:
So is also an eigenstate, with energy higher by . Likewise has energy lower by . Hence “ladder operators”.
Step 4: the ladder must have a bottom rung. Applying repeatedly would lower the energy indefinitely. But the energy is bounded below:
(both terms are expectation values of non-negative operators, and they cannot vanish together). The only escape from the contradiction is a ground state satisfying
Step 5: solve for the ground state. This is a first-order equation, far easier than the original second-order one:
(the prefactor comes from normalisation). The ground state is a Gaussian — a fact that becomes important again in the next section.
Step 6: the ground-state energy. From with :
Step 7: the whole spectrum. Climb from the bottom:
The entire solution used only the commutation relation and never once actually solved the second-order differential equation.
The picture
Equally spaced levels. This is unique to the oscillator. The infinite well’s spacing grows with , hydrogen’s shrinks with ; only the oscillator keeps a constant .
Consequence: the oscillator’s spectrum is a single line (every adjacent transition has the same frequency). Real molecules show several vibrational lines, which is precisely the evidence that the well is not exactly parabolic — anharmonicity is a rich source of information in molecular spectroscopy.
Zero-point energy. . Even at absolute zero the oscillator still jitters. This is no theoretical ornament: helium stays liquid at atmospheric pressure all the way down because the zero-point motion is violent enough to prevent freezing, and the Casimir force comes from the zero-point energy of electromagnetic field modes.
The mathematics
with and the Hermite polynomials:
The recurrence is what this site’s simulations use to evaluate them (see appendix C).
Take a look
The one-dimensional harmonic oscillator
Equally spaced levels, zero-point energy, tails reaching into the classically forbidden region, and the one quantum state that really does behave like a classical particle. Units: ħ = m = 1.
- Eₙ = (n+½)ħω
- 0.500
- Level spacing ħω
- 1.00
- Classical turning point ±A
- ±1.00
- Zero-point energy E₀
- 0.500
A steeper well → larger spacing ħω and a narrower wavefunction
nodes = n = 0
Try this
- In the "level ladder" view, push
nup to 8: the levels stay exactlyħωapart. This is unique to the oscillator — look back at the infinite well, where the spacing grows as you climb. - Turn
ωdown to 0.4 and note that the ground-state energyE₀ = ħω/2shrinks but never reaches zero. Making E₀ = 0 would require the particle to sit exactly at x = 0 with p = 0, andΔxΔp ≥ ħ/2forbids it. - Switch to "single eigenstate" with ψ shown and look at the n = 0 curve beyond the two dashed lines (the classical turning points): it has not gone to zero. The particle has a definite probability of being where classical energy conservation forbids — the very same root as tunnelling.
- Show |ψ|², turn on "compare with classical", and take n from 0 to 20: the envelope of the quantum oscillation hugs the classical curve ever more closely (the ends are favoured because a classical particle moves slowest at the turning points).
- Switch to "coherent state" and press play: the packet oscillates back and forth as a whole, keeps its shape, and its period is exactly the classical
T = 2π/ω. Schrödinger found this most classical of quantum states back in 1926; it is also the theoretical description of laser light.
Each of the three views answers one question:
- Level ladder: is the spacing really constant? (Drag and watch the gaps between the lines.)
- Single eigenstate: how much wavefunction lies beyond the classical turning points? (Look at the tails outside the two dashed lines.)
- Coherent state: is there any quantum state that really moves like a classical particle? (Press play.)
Tails: leaking into the classically forbidden region
A classical particle with energy can only reach the turning point . Beyond that the quantum wavefunction decays as , but it is not zero.
Compute it: the probability of finding the ground state in the forbidden regionadvanced~5 min
For the ground state , the turning point follows from :
(in the dimensionless coordinate the turning points sit exactly at ).
About 15.7%. That is not a small number — a ground-state particle has roughly a one-in-six chance of being found where it classically could never be.
What about excited states? The fraction shrinks as grows (about 5% at ), because the classically allowed region widens while the decay length of the tail stays put. Once again, the quantum effect weakens in relative terms as grows — the correspondence principle.
Key formulas
Ladder operators
The whole structure hides in this one commutator
Hamiltonian
â₊â₋ is the number operator n̂
Energy levels
Equally spaced; the zero-point energy ħω/2 cannot be removed
Ground state
A Gaussian — and also a minimum-uncertainty state
General eigenstate
ξ = √(mω/ħ)·x, with Hₙ the Hermite polynomials
Self-check4 questions
- 1.
Why is the harmonic-oscillator model so ubiquitous in physics?
- 2.
Which single basic relation does the ladder-operator method rely on?
- 3.
Which statements about the zero-point energy E₀ = ħω/2 are correct? (Select all that apply.)
Select all that apply
- 4.
In the ground state of a harmonic oscillator, what is the probability of finding the particle in the classically forbidden region (|ξ| > 1)? (Give a decimal, e.g. 0.157.)
6% relative tolerance
What comes next
So far everything has been a bound state: the particle is trapped and the spectrum is discrete. The next section lets go — set the particle free and see what happens. The answer is a little surprising.
Section 17 of 106 · use ← → to turn the page