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 comes out to β hitting the uncertainty principleβs 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 ?
Stationary states
The eigenvalues, derived in Β§6.6 and quoted here, are
A particle with energy has the wave function
and the four lowest eigenfunctions are those of Table 6.1: a Gaussian times a polynomial, with the oscillator length oscillator length a = β(Δ§/mΟ), the only length a harmonic oscillator possesses. It sets the width of every eigenfunction, and β¨xΒ²β© = (n+Β½)aΒ². defined in ch. 6 β open in glossary setting the width throughout. The polynomials are the Hermite polynomials hermite polynomial The degree-n polynomial Hβ multiplying the Gaussian in the oscillator eigenfunction Οβ β Hβ(x/a)e^(βxΒ²/2aΒ²). Its n roots are exactly the n nodes of Οβ. defined in ch. 6 β open in glossary β degree , and their roots are precisely the nodes of .
What is observable about a state of definite energy
Parity. Because is unchanged under , each eigenfunction has a definite symmetry:
Even has positive parity parity Whether a wave function is unchanged (even parity) or changes sign (odd parity) under reflection through the origin β x β βx in one dimension, r β βr in three. A reflection-symmetric Hamiltonian always has eigenfunctions of definite parity. For a central potential the parity is even when l is even and odd when l is odd, which is what forces the Ξl = Β±1 selection rule. defined in ch. 5 β open in glossary , odd 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.
The time factor has modulus 1, so it cancels β exactly as in Β§4.6. And unlike a classical particle, which is confined to , the quantum particle has non-zero probability everywhere.
Position and momentum. For the -th state,
and therefore
The energy divides equally. Because both and are uncertain, so are the potential and kinetic energies, and their expectation values are
Half the energy is potential, half kinetic β in every state, exactly. Their sum is , which is sharp even though neither part is.
Non-stationary states
Nothing above moves. To get motion, superpose:
This is a state of uncertain energy: measuring gives with probability , with probability , and so on. It is also non-stationary, because now carries interference between different eigenfunctions. The interference of with oscillates at
which for this spectrum is always an integer multiple of . So can carry , , and so on.
Why the average position oscillates at and nothing else
carries harmonics, so one expects to carry them too. It does not. Evaluating produces terms in with
and vanishes unless (problem 11). Adjacent levels are exactly apart, so the only surviving frequency is :
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 quasi-classical state A superposition of oscillator states whose |cβ|Β² is Poisson-distributed about a large mean nΜ. Its β¨xβ© traces classical simple harmonic motion, and its relative energy spread falls as 1/βnΜ. defined in ch. 6 β open in glossary , with energy amplitudes following a Poisson distribution:
Using the mean and standard deviation of the Poisson distribution from problem 1 of chapter 3,
so the relative energy uncertainty is
Where this goes next
Β§6.4 puts these results to work on a real system: two nuclei vibrating in a chemical bond, where 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
Select "ground state alone" in the widget and press play.
1.Nothing moves. What is the wave function doing while nothing moves?
2.Why is exactly, and not merely close to it, in the oscillator's ground state?
Switch to "Οβ + Οβ + Οβ" and look at the lower panel.
3. visibly carries a component, yet is a clean cosine at . Why?
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.A superposition in a box eventually reassembles after a long revival time; an oscillator superposition repeats every exactly. What is responsible?
6.In every oscillator eigenstate, and each equal . What is the classical counterpart, and where does the analogy fail?