
Quantum core · institution-dependent · Interactive lesson
Operators and the measurement postulate
Quantum mechanics splits a measurement in two. Solve one eigenvalue problem and you have every result the meter can ever show. Expand your state on those eigenfunctions and you have how often each one shows. This lesson builds both halves, and marks the line the theory refuses to cross.
UPIV-06.05 · Lesson 5 of 9 in this unit. Position is not a completion score.Quantum core · institution-dependent. Departments differ in how much quantum mechanics they include in Physics IV or teach in a dedicated course. Follow your university’s required mathematical depth and assessment; these numbered units are not automatically optional.
Build the model
The operator supplies the menu; the state supplies the odds.
The key idea
An observable is represented by a Hermitian operator, the possible results of measuring it are exactly that operator's eigenvalues, and the probability of each is the squared modulus of the state's coefficient on the matching eigenfunction.
Example. An electron in a 0.50 nm infinite well prepared as Ψ = (ψ₁ + 2ψ₂)/√5 can read only 1.504 eV or 6.016 eV, with probabilities 1/5 = 0.20 and 4/5 = 0.80 — never the in-between mean of 5.11 eV.
The complete physical model and assumptions
Classical mechanics keeps an observable and its value in the same object: a particle has a position, and measuring it copies that number out. Quantum mechanics breaks the pair apart and gives each half its own mathematical home. The observable becomes a Hermitian operator — position multiplies by x, momentum differentiates as −iħ ∂/∂x, kinetic energy is −(ħ²/2m) ∂²/∂x², and the Hamiltonian is their sum with V(x) — while the value belongs to the state, if it exists at all. Solve Q̂φₙ = qₙφₙ once and the eigenvalues qₙ are the complete menu of readings that observable can ever produce; anything else is not unlikely, it is unavailable. The state Ψ then supplies only odds: expand it as Ψ = Σ cₙφₙ and P(qₙ) = |cₙ|². And the reading rewrites the state — once qₙ comes back, what is left is φₙ, which is why an immediate repeat returns qₙ again. That last clause is where the model charges you. The projection is not a consequence of the Schrödinger equation; it is a second rule, abrupt, random and irreversible, bolted alongside a smooth deterministic one, kept because laboratories behave that way. What it delivers is the statistics of an ensemble of identically prepared runs: it guarantees that the next single run lands on the menu, but unless the state is an eigenstate of what is measured it cannot say which entry.
1Build the operator from the classical expression
Start from the plane wave ψ = A e(i(kx − ωt)), the state de Broglie gave momentum p = ħk. Differentiate it: −iħ ∂ψ/∂x = −iħ(ik)ψ = ħk ψ = p ψ. The derivative pulled the momentum out as a factor, so the operator standing for momentum is p̂ = −iħ ∂/∂x — and the i is not decoration, since without it the eigenvalues come out imaginary. Position needs no derivative at all: x̂ψ = xψ, multiplication by the coordinate. Everything else is assembled by writing the classical expression and substituting. Kinetic energy p²/2m becomes T̂ = −(ħ²/2m) ∂²/∂x², total energy becomes Ĥ = T̂ + V(x). Check units as you go: ħ = 1.055×10⁻³⁴ J s, so ħ ∂/∂x carries J s m⁻¹ = kg m s⁻¹, a momentum. The recipe has one soft spot. Classically xp and px are the same number, but x̂p̂ and p̂x̂ are different operators, so a classical product of position and momentum leaves the ordering undecided and the physics, not the dictionary, has to choose.
2Test whether the state has a value at all
There is exactly one test for whether an observable has a definite value in a given state: act with the operator and see whether what comes back is that same function times a constant. Take an electron in an infinite well of width L = 0.50 nm, in its ground state ψ₁ = √(2/L) sin(πx/L). Apply Ĥ and out comes E₁ψ₁ with E₁ = h²/8mL² = 2.410×10⁻¹⁹ J = 1.504 eV: energy is sharp, and every run of an energy measurement reads 1.504 eV. Apply p̂ and you get −iħ√(2/L)(π/L) cos(πx/L) — a cosine, not a multiple of the sine. Momentum has no value in this state. Writing sin(πx/L) = (e(iπx/L) − e(−iπx/L))/2i tempts you to predict ±ħπ/L half the time each, but the sine stops at the walls, so those truncated waves are not momentum eigenfunctions, and a momentum measurement returns a continuous spread of values, symmetric about zero, not two spikes. What the state does fix are the moments: ⟨p̂⟩ = 0 because ψ₁ is real, and ⟨p̂²⟩ = ħ²∫|dψ₁/dx|² dx = (ħπ/L)², so √⟨p̂²⟩ = ħπ/L = 6.63×10⁻²⁵ kg m s⁻¹ — and p²/2m for that magnitude is 1.504 eV, exactly E₁, as it must be where V = 0.
3The spectrum is the entire menu of readings
Solving Q̂φₙ = qₙφₙ is a one-off cost, paid before any particular state is considered, and what it returns is the whole dial. For the electron in the 0.50 nm well the energies are Eₙ = n²h²/8mL² = 1.504, 6.016, 13.54 and 24.07 eV, …, so an energy measurement on any state of that electron returns one of those numbers. A reading of 3.0 eV is not unlikely; it is not on the dial. Two ingredients fix the list, and students routinely credit only the first. The operator supplies the differential equation; the boundary conditions supply the rest. The same −(ħ²/2m) d²/dx² gives a discrete ladder inside a box and an unbroken continuum for a free electron, where every real p is an eigenvalue of p̂ and the sum over states becomes an integral. It is also why the dial moves when the apparatus does: halve the well to 0.25 nm and every level rises by a factor of four, to 6.016, 24.07 and 54.15 eV.
4Expand the state to get the odds
With the eigenfunctions in hand, any admissible state is a sum over them: Ψ = Σ cₙφₙ. Orthonormality extracts the coefficients — multiply by φₘ* and integrate, and every term but one dies, leaving cₘ = ∫ φₘ* Ψ dx. Born's rule reads the probability straight off: P(qₘ) = |cₘ|². Take Ψ = N(ψ₁ + 2ψ₂) in the well. Normalising gives |N|²(1 + 4) = 1, so N = 1/√5, c₁ = 1/√5 and c₂ = 2/√5, and the table is P(1.504 eV) = 1/5 = 0.20 and P(6.016 eV) = 4/5 = 0.80. Notice that the coefficient 2 became a probability of 0.80, not 2/3: it is the squares that are shared out, not the amplitudes. Notice too what the modulus throws away. Replace c₂ by 2e(iθ)/√5 for any θ and the energy table does not move — but |Ψ(x)|² does, because its cross term 2Re(c₁*c₂ψ₁ψ₂) carries the relative phase. Phase is invisible to one observable's statistics and plainly visible in the density.
5What the reading leaves behind
The postulate has a second clause. When the meter shows qₙ, the state immediately afterwards is φₙ, renormalised. Measure the energy of Ψ = (ψ₁ + 2ψ₂)/√5, read 6.016 eV, and the ψ₁ term is gone: the state is ψ₂, and a second energy measurement made straight away returns 6.016 eV with probability 1. Reproducibility is not a bonus feature; it is what the projection clause exists to deliver. Two refinements matter. If qₙ is degenerate the state does not collapse onto a single eigenfunction but onto its projection into the whole eigenspace, P̂ₙΨ/‖P̂ₙΨ‖, so a measurement can perfectly well leave a superposition standing. And if the second measurement is of an incompatible observable, the projection it performs scrambles the first table again. Set the two kinds of change side by side: Schrödinger evolution is continuous, deterministic and reversible; projection is abrupt, random and irreversible. Nothing in the equation produces the second, which is precisely why it is a separate postulate. Whether that step is a physical event or only an update of our description, the postulate does not say; that question is where the interpretations of quantum mechanics part company.
6Statistics of an ensemble, not a forecast for one run
Because no single outcome is fixed, the content of the postulate is a distribution, and the two numbers usually quoted are its mean and its spread. For the 20/80 state, ⟨Ĥ⟩ = 0.20 × 1.504 + 0.80 × 6.016 = 5.11 eV and σE = |E₂ − E₁|√(P₁P₂) = 4.512 × 0.400 = 1.8 eV. Read that mean carefully: it is the average of a long run of measurements, and it is a number no single measurement can ever display, because it is not in the spectrum. The distribution is also not ignorance. A coherent superposition and a statistical mixture of 20% ψ₁ with 80% ψ₂ give identical energy tables, so no quantity of energy data will separate them; what separates them is the interference term in |Ψ(x, t)|², present in one and absent in the other. Finally, be blunt about the gap. The postulate offers no rule, hidden or otherwise, for whether the next electron will show 1.504 eV or 6.016 eV. Every prediction it makes is a claim about many identically prepared runs.
Key equations
Read the units, assumptions and limits before substituting.
The quantisation dictionary
x̂ψ = xψ, p̂ψ = −iħ ∂ψ/∂x, T̂ψ = −(ħ²/2m) ∂²ψ/∂x²
Write the classical expression, then substitute. Every observable of the spinless particle in this unit is assembled from these two.
ħ = 1.055×10⁻³⁴ J s, so ħ ∂/∂x carries kg m s⁻¹ and T̂ψ carries joules × ψThe Hamiltonian
Ĥ = T̂ + V(x) = −(ħ²/2m) d²/dx² + V(x)
One operator does two jobs: its eigenvalues are the energies you can read, its eigenfunctions the stationary states.
V(x) in joules, multiplying ψ; Ĥ is the total-energy observable and also the generator of the evolutionEigenvalue problem: the whole dial
Q̂φₙ = qₙφₙ, qₙ real
Solved once, before any state is named. A number outside (qₙ) is not improbable — it cannot be read.
φₙ is the eigenfunction, n labels the spectrum; the boundary conditions decide whether n is discrete or continuousExpansion and Born's rule
Ψ = Σₙ cₙφₙ, P(qₙ) = |cₙ|², Σₙ |cₙ|² = 1
Converts a wavefunction into a probability table over the dial. If the squares miss 1, a term or a normaliser was dropped.
cₙ = ∫ φₙ* Ψ dx, complex, and dimensionless when Ψ and φₙ are both normalisedState update on reading qₙ
Ψ → φₙdegenerate case Ψ → P̂ₙΨ / ‖P̂ₙΨ‖
The only reason a repeated measurement reproduces itself — and the one step no Schrödinger evolution supplies.
P̂ₙ projects onto the whole eigenspace of qₙ; the update is instantaneous, non-unitary and irreversibleEnsemble mean and spread
⟨Q̂⟩ = ∫ Ψ* Q̂Ψ dx = Σₙ qₙ|cₙ|²
The average of many runs. It need not be an eigenvalue, so it is often a number no single run can ever show.
carries the unit of q; the variance is Σₙ qₙ²|cₙ|² − ⟨Q̂⟩², and σ is its square rootInteractive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Drive the ψ₂ and ψ₃ sliders to zero: one bar goes to 1.000 and the dashed mean snaps exactly onto the 1.504 eV rung, because only an eigenstate has a definite energy. Then set the weights to 2.2, 0 and 1.7: the mean reads 6.00 eV, almost on the 6.016 eV rung, while that reading has probability zero, so a mean that meets a rung is still not a reading.
Live results
- MEAN ⟨E⟩
- 5.11 eV
- P(E₁) = |c₁|²
- 0.200
- P(E₂) = |c₂|²
- 0.800
- P(E₃) = |c₃|²
- 0.000
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Weight on ψ₁, before normalising: 1.0; Weight on ψ₂, before normalising: 2.0; Weight on ψ₃, before normalising: 0.0
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The commonest error is to read the superposition as ignorance: the electron is really in ψ₁ or ψ₂ and the measurement merely uncovers which. That picture gets the energy table right and everything else wrong. A genuine 20/80 mixture has density 0.20|ψ₁|² + 0.80|ψ₂|², while the superposition carries an extra cross term 2Re(c₁*c₂ψ₁ψ₂) that beats at (E₂ − E₁)/ħ = 6.86×10¹⁵ rad s⁻¹ — a measurable difference in where the electron is found, produced by exactly the coefficients the ignorance story discards. The second half of the error is treating ⟨Ĥ⟩ = 5.11 eV as a typical reading. It is the mean of readings that are only ever 1.504 eV or 6.016 eV, and it is not one of them.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
A free electron is described by the plane wave ψ(x) = A e(ikx) with k = 1.20×10¹⁰ m⁻¹. Show that momentum has a definite value in this state while position does not, and find the momentum and the kinetic energy.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 4 steps revealed.
- Apply the momentum operator: p̂ψ = −iħ dψ/dx = −iħ(ik)A e(ikx) = ħk ψ. What comes back is ψ times a constant, so ψ is an eigenfunction of p̂ and the eigenvalue is p = ħk.
- p = 1.055×10⁻³⁴ J s × 1.20×10¹⁰ m⁻¹ = 1.266×10⁻²⁴ kg m s⁻¹. Every run of a momentum measurement on this state returns that one number, so the spread is zero.
- Kinetic energy is built from the same operator, T̂ = p̂²/2m, so ψ is an eigenfunction of it too: T = p²/2m = (1.266×10⁻²⁴)²/(2 × 9.11×10⁻³¹) = 8.80×10⁻¹⁹ J = 5.49 eV.
- Now the position operator: x̂ψ = x A e(ikx). The result is ψ multiplied by the variable x, not by a constant, so ψ is not an eigenfunction of x̂ and position has no value here. Consistently, |ψ|² = |A|² is flat — no position is favoured and none of them is the value. The same flatness makes ∫|ψ|² dx diverge, so no choice of A normalises the plane wave: it is the idealised limit of a very long wave packet, not a state an electron can occupy exactly.
Answer. p = ħk = 1.266×10⁻²⁴ kg m s⁻¹ and T = 5.49 eV, both sharp; position has no value at all, since x̂ψ is not a multiple of ψ.
MediumExample 2
The electron is now trapped in an infinite well of width L = 0.50 nm and prepared as Ψ = N(ψ₁ + 2ψ₂), with ψₙ the normalised energy eigenfunctions. Normalise the state, write the table of possible energy readings with their probabilities, and find the mean and standard deviation of the energy.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- Normalise using orthonormality: ∫|Ψ|² dx = |N|²(1 + 4) = 1, because the cross terms ∫ψ₁*ψ₂ dx vanish. So N = 1/√5, giving c₁ = 1/√5 and c₂ = 2/√5.
- Born's rule: P(E₁) = |c₁|² = 1/5 = 0.20 and P(E₂) = |c₂|² = 4/5 = 0.80. They sum to 1, as any complete table must.
- The eigenvalues come from the well, not from the state: E₁ = h²/8mL² = (6.626×10⁻³⁴)²/(8 × 9.11×10⁻³¹ × (5.0×10⁻¹⁰)²) = 2.410×10⁻¹⁹ J = 1.504 eV, and E₂ = 4E₁ = 6.016 eV.
- Mean: ⟨Ĥ⟩ = Σ Eₙ|cₙ|² = 0.20 × 1.504 + 0.80 × 6.016 = 0.301 + 4.813 = 5.11 eV.
- Spread, from the two-outcome shortcut: σE = |E₂ − E₁|√(P₁P₂) = 4.512 × √0.16 = 4.512 × 0.400 = 1.8 eV. Check it the long way: Σ Eₙ²|cₙ|² − ⟨Ĥ⟩² = 29.41 − 26.15 = 3.26 eV², whose root is 1.8 eV.
Answer. N = 1/√5; the readings are 1.504 eV with probability 0.20 and 6.016 eV with probability 0.80; ⟨Ĥ⟩ = 5.11 eV with σE = 1.8 eV, and 5.11 eV is itself never a reading.
HardExample 3
That same state is left alone for 1.0 ps, then its energy is measured and reads 6.016 eV, and the energy is measured again immediately afterwards. (a) Do the outcome probabilities drift during the 1.0 ps? (b) What does the second reading give, and with what probability? (c) What are ⟨Ĥ⟩ and σE after it?
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- Each eigenstate picks up its own phase, cₙ → cₙ e(−iEₙt/ħ). That factor has unit modulus, so |cₙ|² is untouched: the table is still 0.20 / 0.80 at t = 1.0 ps and at every other time. So the answer to (a) is no.
- What does move is the density. Its cross term oscillates at ω₂₁ = (E₂ − E₁)/ħ, and E₂ − E₁ = 4.5124 eV = 7.230×10⁻¹⁹ J, so ω₂₁ = 7.230×10⁻¹⁹ / 1.0546×10⁻³⁴ = 6.86×10¹⁵ rad s⁻¹ — a period of 0.92 fs, about 1100 sloshes in 1.0 ps while the energy statistics stood perfectly still.
- The first reading returns 6.016 eV, an outcome of probability 0.80, and the projection clause then replaces the state by the matching eigenfunction: Ψ → ψ₂, up to a global phase. The ψ₁ amplitude is deleted, not merely made small.
- Expand that new state on the energy eigenbasis: c₂ = 1 and every other coefficient is 0. The second reading therefore gives 6.016 eV with probability |1|² = 1, which answers (b).
- For (c), a single term leaves ⟨Ĥ⟩ = 6.016 eV and σE = 0. The mean jumped from 5.11 eV to 6.016 eV at the instant of the first reading — a change no solution of the Schrödinger equation produces, which is exactly why projection has to be posted as a separate rule.
Answer. (a) No: the phases have unit modulus, so the table stays 0.20 / 0.80. (b) 6.016 eV, with probability 1. (c) ⟨Ĥ⟩ = 6.016 eV and σE = 0.
Quick check
Select an answer and explain it before checking.
Review & continue
An observable is represented by a Hermitian operator, the possible results of measuring it are exactly that operator's eigenvalues, and the probability of each is the squared modulus of the state's coefficient on the matching eigenfunction.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.