
Quantum core · institution-dependent · Interactive lesson
Separation of variables and the time-independent equation
The time-dependent equation is a partial differential equation in two variables, and you will not integrate it by hand. This topic buys the trick that makes it tractable — split x from t — then charges you honestly: it works only for a static potential, and it delivers only the states whose density never moves.
UPIV-06.03 · Lesson 3 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
One ansatz, one separation constant, and the constant turns out to be the energy.
The key idea
Separation of variables writes a solution as a function of position alone multiplied by a function of time alone, which reduces the time-dependent Schrödinger equation to the eigenvalue equation Ĥψ = Eψ — but only when the potential has no explicit time dependence.
Example. For an electron in the n = 1 state of a 1.00 nm infinite well, E₁ = h²/8mL² = 6.02 × 10⁻²⁰ J = 0.376 eV, so the factor e(−iEt/ħ) turns through a full 2π every h/E₁ = 1.10 × 10⁻¹⁴ s while |Ψ|² never changes at all.
The complete physical model and assumptions
Separation of variables is a guess with a payoff. Assume Ψ(x, t) = ψ(x)φ(t), substitute, divide by the product, and the equation falls into a piece that depends on t alone and a piece that depends on x alone. Two functions of different variables can agree only by both being the same constant, and that single step is where the whole method lives — it goes through if and only if V carries no explicit time dependence. Comparing the resulting time factor with the plane wave, whose phase turns as e(−iωt) with E = ħω, names the constant: it is the energy. The time equation then integrates in one line to φ(t) = e(−iEt/ħ), a pure phase of unit modulus whenever E is real, and the spatial remainder is the eigenvalue problem Ĥψ = Eψ. What this costs is scope. You have not solved the time-dependent equation; you have found its stationary states, the special solutions whose probability density never moves. A general state is a superposition of them carrying different energies, and a superposition satisfies the time-dependent equation but not Ĥψ = Eψ, because there is no single E to put on the right. And if V itself depends on time — a driven atom, a wall that moves — the division that produced the constant never comes off, and the method is simply unavailable.
1The equation you have to solve, and why it resists
The time-dependent Schrödinger equation, iħ ∂Ψ/∂t = −(ħ²/2m) ∂²Ψ/∂x² + V(x, t)Ψ, is a partial differential equation: one unknown function of two variables, differentiated once in t and twice in x. For an arbitrary V there is no general closed form, and even where one exists you would not reach it by direct attack. Separation of variables sidesteps the problem rather than solving it. Ask a narrower question — are there any solutions of the special product form Ψ(x, t) = ψ(x)φ(t), in which the x-dependence and the t-dependence never mix? — and the answer comes in three lines. The narrower question is worth asking because the special solutions turn out to form a complete set: once you have all of them, every other solution is a superposition of them. But keep the logic straight. The ansatz is a guess about the form of a solution, justified only by substituting it and finding that it works. Nothing so far promises that such a solution exists, and nothing claims a general Ψ has this form.
2Substitute, divide, and watch the variables come apart
Put Ψ = ψφ into the equation. The time derivative touches only φ and the space derivative only ψ, so iħ ψ φ′ = −(ħ²/2m) ψ″ φ + V ψφ. Divide every term by the product ψφ — legitimate wherever it is non-zero — and you are left with iħ φ′/φ = −(ħ²/2m) ψ″/ψ + V. Now read the two sides. The left is a function of t and of nothing else. The right is a function of x and of nothing else, provided V = V(x). A function of t alone can equal a function of x alone only if neither actually varies: hold x fixed and the right side is a fixed number, so the left must equal that number for every t, and conversely. Both sides equal one constant. If instead V = V(x, t) — a laser field switched on, a well wall in motion — the right-hand side still contains t after the division, the argument collapses at this exact line, and the product ansatz buys nothing. That is the entire restriction on the method, and it is worth noticing that it shows up here, at the start, rather than at the end.
3Naming the constant: it has to be the energy
Call the constant E. Nothing in the algebra says what it is; the identification comes from outside. Two arguments agree. First, the time equation is iħφ′ = Eφ, so φ ∝ e(−iEt/ħ), and comparing this with the free-particle plane wave e(i(kx − ωt)) gives E = ħω — the Planck relation the whole equation was built on. Second, the spatial equation reads Ĥψ = Eψ with Ĥ = −(ħ²/2m)d²/dx² + V the operator for total energy, so for normalised ψ the mean energy is ⟨H⟩ = ∫ψ*Ĥψ dx = E∫|ψ|² dx = E. The variance goes the same way: ⟨H²⟩ = ∫ψ*Ĥ(Eψ) dx = E², so σH² = E² − E² = 0. A separable state has a sharp energy, not a spread of energies, and E is its value. That is the strongest justification for the name — not that the units work out, but that an energy measurement on such a state returns E every single time.
4A pure phase is what makes a state stationary
Integrating iħφ′ = Eφ gives φ(t) = e(−iEt/ħ), any constant of integration being absorbed into ψ. For real E this has modulus exactly one: e(−iEt/ħ) × e(+iEt/ħ) = 1. So |Ψ(x, t)|² = |ψ(x)|² |φ(t)|² = |ψ(x)|², frozen for all time. The same cancellation runs through every expectation value, since in ∫Ψ*ÂΨ dx the two phases meet as e(+iEt/ħ)e(−iEt/ħ) = 1, so ⟨x⟩, ⟨p⟩ and the mean of any operator carrying no explicit time dependence are constants as well. This is why the separable solutions are called stationary states, and it is a strong physical claim: an electron in the n = 2 level of an atom is not orbiting, and its probability cloud is not sloshing. The phase, meanwhile, is very much alive. It turns through 2π in a time h/E — ten femtoseconds or so for an electron confined to a nanometre — and no measurement on this state can see that rotation, because a global phase cancels out of every expectation value. Only the relative phase between two terms of a superposition is observable, which is exactly what makes superpositions the interesting case.
5Boundary conditions, not the ODE, quantise E
What remains is −(ħ²/2m)ψ″ + Vψ = Eψ, an ordinary differential equation in x, second order and linear. As an ODE it is unfussy: choose any real E and any V and solutions exist. Quantisation therefore does not come from the equation. It comes from insisting that ψ be an admissible wavefunction — normalisable, continuous, with ψ′ continuous wherever V is finite, and satisfying whatever the boundaries demand. In an infinite well of width L those conditions force ψ(0) = ψ(L) = 0, which kills every solution except sin(nπx/L) and leaves Eₙ = n²π²ħ²/2mL² = n²h²/8mL². For an electron in L = 1.00 nm the ladder is 0.376 eV, 1.504 eV, 3.384 eV — discrete because the box refuses everything else, not because the differential equation did. Ask for E = 0.5 eV and a mathematical solution still exists; it simply fails to vanish at both walls. Reading the spatial part as an eigenvalue problem is what makes the finite well, the harmonic oscillator and the hydrogen atom one technique instead of three.
6A superposition solves one equation and not the other
Because Ĥ is linear, any sum Ψ(x, t) = Σ cₙ ψₙ(x) e(−iEₙt/ħ) also solves the time-dependent equation, with the coefficients fixed once and for all by the initial state through cₙ = ∫ψₙ*(x)Ψ(x,0) dx. That sum is the general solution, and it is the reason separating was worth the trouble. But it is not an eigenstate. Feed it to Ĥψ = Eψ and the left side returns Σ cₙ Eₙ ψₙ e(−iEₙt/ħ), which is not E times the state for any single E unless exactly one cₙ is non-zero. Two occupied levels leave a cross term in |Ψ|² that beats at (Eₘ − Eₙ)/h — in the hundreds of terahertz for the lowest pairs of that 1.00 nm well — so the density genuinely moves and no time-independent equation can describe it. The rule to carry away is to write Ĥψ = Eψ only for a state you have already committed to being an energy eigenstate. Everything else evolves.
Key equations
Read the units, assumptions and limits before substituting.
The separable ansatz
Ψ(x, t) = ψ(x) φ(t)
It selects the stationary states out of all the solutions; it is not the general solution.
ψ in m(−1/2) for a 1-D state, φ dimensionless; the split is a guess, tested by substituting it.Where the separation constant appears
iħ φ′/φ = −(ħ²/2m) ψ″/ψ + V(x) = E
Only a time-independent V lets the x-side be free of t. This single line is the whole method — and its whole restriction.
Left side a function of t only, right side of x only, so both equal one constant E, in joules.The time factor
φ(t) = e(−iEt/ħ), |φ| = 1 for real E
Unit modulus is why an eigenstate's density is frozen; a complex E would drain the norm instead.
E in J, ħ = 1.055 × 10⁻³⁴ J s; the phase turns through 2π in a time h/E.Time-independent Schrödinger equation
−(ħ²/2m) d²ψ/dx² + V(x)ψ = Eψ ⇔ Ĥψ = Eψ
An eigenvalue problem: the boundary conditions, not the differential equation, decide which E survive.
Ĥ = p̂²/2m + V(x); with ψ in m(−1/2), every term carries J m(−1/2).Why the density is stationary
|Ψ(x, t)|² = |ψ(x)|²
Every expectation value of a time-independent operator is then a constant — hence the name stationary.
True for a single eigenstate only, and only because e(−iEt/ħ) cancels its own conjugate.The general state is a sum, not an eigenstate
Ψ(x, t) = Σₙ cₙ ψₙ(x) e(−iEₙt/ħ)
Solves the time-dependent equation; obeys Ĥψ = Eψ only when exactly one cₙ is non-zero.
cₙ = ∫ψₙ*(x) Ψ(x, 0) dx, dimensionless, with Σ|cₙ|² = 1.Interactive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Sweep θ with n held fixed: Re Ψ and Im Ψ trade places and the dial turns, while the lower curve does not shift by a pixel — that is |φ| = 1 doing its work. Then change n, and everything reshapes at once, because the level is what the boundary conditions fixed and the phase is not.
Live results
- ENERGY Eₙ
- 4 E₁
- PHASE PERIOD h/Eₙ
- 2.75 fs
- REAL PART Re φ
- 0.50
- MODULUS |φ|
- 1.00
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. Level n in ψₙ: 2; Phase θ = Eₙt/ħ: 60 °
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 treat Ĥψ = Eψ as the Schrödinger equation and then hang the factor e(−iEt/ħ) on whatever state is in front of you. It fits a single eigenstate and nothing else. A superposition of n = 1 and n = 2 evolves as c₁ψ₁e(−iE₁t/ħ) + c₂ψ₂e(−iE₂t/ħ), two phases turning at two different rates; there is no one E to put in a single exponential, and the mismatch you would be discarding is exactly the beat that makes the density move. The mirror error is to read stationary as nothing happens. The phase never stops turning, and it is unobservable only because it is global — put two such states together and the relative phase becomes a measurable oscillation.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
A particle is in the separable state Ψ(x, t) = ψ(x) e(−iEt/ħ) with real E = 3.00 eV. Show that its probability density carries no time dependence, and find how long the phase factor takes to complete one full turn.
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.
- Form the density: |Ψ|² = Ψ*Ψ = ψ*(x)e(+iEt/ħ) · ψ(x)e(−iEt/ħ). For real E the two exponentials multiply to e⁰ = 1.
- So |Ψ(x, t)|² = |ψ(x)|², independent of t — and with it every expectation value of an operator carrying no explicit t. That is exactly what stationary means.
- The phase returns to its starting value when Et/ħ = 2π, so t = 2πħ/E = h/E.
- E = 3.00 eV = 3.00 × 1.602 × 10⁻¹⁹ = 4.807 × 10⁻¹⁹ J, giving t = 6.626 × 10⁻³⁴ ÷ 4.807 × 10⁻¹⁹ = 1.38 × 10⁻¹⁵ s.
Answer. |Ψ|² = |ψ|² for every t, so the state is stationary; the phase completes one turn in h/E = 1.38 × 10⁻¹⁵ s, a rotation no measurement on this state alone can detect.
MediumExample 2
Substitute Ψ(x, t) = ψ(x)φ(t) into iħ ∂Ψ/∂t = −(ħ²/2m) ∂²Ψ/∂x² + V Ψ and carry the separation through to the two ordinary equations. Then state precisely what changes if the potential is instead V(x, t) = V₀(x) + F₀ x cos(Ωt), the potential of an oscillating uniform force of amplitude F₀ and drive frequency Ω.
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.
- Differentiate the product: ∂Ψ/∂t = ψ φ′ and ∂²Ψ/∂x² = ψ″ φ, so the equation becomes iħ ψ φ′ = −(ħ²/2m) ψ″ φ + V ψ φ.
- Divide every term by ψφ wherever it is non-zero: iħ φ′/φ = −(ħ²/2m) ψ″/ψ + V(x).
- The left side depends only on t, the right only on x. Fix x and the right side is a number, so the left equals that same number for every t. Both sides equal one constant; call it E.
- Time equation: iħ φ′ = Eφ, so φ(t) = e(−iEt/ħ). Space equation: −(ħ²/2m) ψ″ + Vψ = Eψ, which is Ĥψ = Eψ.
- With V = V₀(x) + F₀ x cos(Ωt), the same division leaves iħ φ′/φ = −(ħ²/2m) ψ″/ψ + V₀(x) + F₀ x cos(Ωt). The right-hand side still contains t, so the argument that both sides must be constant never starts. A driven system has no stationary states, and the separation is unavailable, not merely harder.
Answer. iħ φ′/φ = E = −(ħ²/2m) ψ″/ψ + V, giving φ = e(−iEt/ħ) and Ĥψ = Eψ. With the driving term, t survives on the x-side, both sides cannot be one constant, and no product solution exists.
HardExample 3
An electron sits in a 1.00 nm infinite square well, so Eₙ = n²h²/8mL². It is prepared as Ψ(x, 0) = (√3 ψ₁ + ψ₃)/2. Check the normalisation, write Ψ(x, t), find ⟨E⟩, find the frequency at which |Ψ|² oscillates, and say whether this state satisfies Ĥψ = Eψ.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- The ladder: E₁ = h²/8mL² = (6.626 × 10⁻³⁴)² ÷ (8 × 9.109 × 10⁻³¹ × (1.00 × 10⁻⁹)²) = 4.390 × 10⁻⁶⁷ ÷ 7.288 × 10⁻⁴⁸ = 6.02 × 10⁻²⁰ J = 0.376 eV, so E₃ = 9E₁ = 3.384 eV.
- Normalisation: the ψₙ are orthonormal, so |c₁|² + |c₃|² = 3/4 + 1/4 = 1. The state is already normalised.
- Each term carries its own phase, never a shared one: Ψ(x, t) = (√3/2) ψ₁ e(−iE₁t/ħ) + (1/2) ψ₃ e(−iE₃t/ħ).
- Mean energy: ⟨E⟩ = Σ |cₙ|² Eₙ = 0.75 × 0.376 + 0.25 × 3.384 = 0.282 + 0.846 = 1.128 eV, which is 3E₁.
- The cross term in |Ψ|² carries the relative phase e(−i(E₃−E₁)t/ħ), so the density oscillates at f = (E₃ − E₁)/h = 8E₁/h = 8 × 6.02 × 10⁻²⁰ ÷ 6.626 × 10⁻³⁴ = 7.27 × 10¹⁴ Hz, a period of 1.37 fs.
- Test the eigenvalue equation: Ĥ acting on the state gives (√3/2)E₁ψ₁e(−iE₁t/ħ) + (1/2)E₃ψ₃e(−iE₃t/ħ). Since E₁ ≠ E₃ this is not any constant times Ψ.
Answer. ⟨E⟩ = 3E₁ = 1.13 eV; |Ψ|² oscillates at 7.27 × 10¹⁴ Hz, a period of 1.37 fs; and no — Ĥψ = Eψ fails because E₁ ≠ E₃. Only the time-dependent equation holds.
Quick check
Select an answer and explain it before checking.
Review & continue
Separation of variables writes a solution as a function of position alone multiplied by a function of time alone, which reduces the time-dependent Schrödinger equation to the eigenvalue equation Ĥψ = Eψ — but only when the potential has no explicit time dependence.
- 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.