A Particle in a Well of Finite Height

Key idea: H3 Quantum Mechanics: the finite square well — exponential decay outside the well, boundary matching, and why tunnelling is possible.

  • Advanced Physics
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Learning objectives

  • Use state functions, boundary conditions, stationary states, and measurement to analyse introductory quantum systems.

In an infinite well, the wavefunction is strictly zero outside the well. Real wells are finite: if the particle’s energy is below the wall height, the wavefunction decays outside the well but is not zero. This is evanescent penetration; if the forbidden region has finite width and another allowed region lies beyond it, the same mathematics permits tunnelling transmission.

Prerequisites + Path

1. Finite-square-well model

We use the common “finite square well” model:

  • V(x) = 0 for 0 < x < L
  • V(x) = V₀ for x ≤ 0 and x ≥ L

For a bound state, the particle has:

E < V₀

The finite-well schematic below shows the key bound-state signature: oscillatory ψ(x) inside the well with exponential tails outside.

Finite square well with exponential tailsPotential-energy profile and bound-state wavefunction showing oscillatory interior behaviour and evanescent tails outside.xVV₀V = 0E0Lψ ∝ e^(-κx)ψ ∝ e^(+κx)oscillatory inside well
Scroll diagram horizontally to read all labels.
For E < V₀, ψ(x) oscillates inside 0 < x < L and decays exponentially into the classically forbidden regions on both sides.

2. Solutions in each region

Start from the time-independent Schrödinger equation:

-(ħ²/2m)d²ψ/dx² + Vψ = Eψ

Region II (inside the well, 0 < x < L)

Here V = 0, so:

d²ψ/dx² = -k²ψ where k² = 2mE/ħ²

General solution:

ψ_II(x) = A sin(kx) + B cos(kx)

Regions I and III (outside the well)

Here V = V₀ and for a bound state E < V₀, so:

d²ψ/dx² = κ²ψ where κ² = (2m(V₀-E))/ħ²

General solution:

ψ(x) = Ce^(κ x) + De^(-κ x)

Physical acceptability requires ψ → 0 far from the well:

  • Region I (x < 0): discard e^(-κ x) (it blows up as x → -∞), so ψ_I(x) = F e^(κ x)
  • Region III (x > L): discard e^(+κ x) (it blows up as x → + ∞), so ψ_III(x) = G e^(-κ x)

So the wavefunction is non-zero outside the well but decays exponentially.

3. Boundary conditions and quantisation

At a finite potential step, both ψ and its first derivative must be continuous:

  • at x = 0: ψ_I = ψ_II and dψ_I/dx = dψ_II/dx
  • at x = L: ψ_II = ψ_III and dψ_II/dx = dψ_III/dx

These conditions do not force ψ to be zero at the walls. Instead, they select only certain values of E that make the three-region solution “fit” smoothly, so the bound-state energies are still discrete.

What changes compared to the infinite well?
  • Infinite well: boundary conditions are ψ(0) = ψ(L) = 0 and ψ = 0 outside. - Finite well: ψ is continuous at the walls and “leaks” outside with an exponential tail.

4. Penetration depth and tunnelling

Outside the well, ψ ∝ e^(-κ x), so the probability density falls like:

|ψ|² ∝ e^(-2κ x)

A common way to describe how far the wavefunction penetrates is the penetration depth:

δ = 1/κ

Larger V₀ (or smaller E) makes κ larger, so the tail decays faster and the finite well approaches the infinite-well limit.

Tail versus transmission

A non-zero tail outside a bound well does not by itself describe a particle escaping to infinity. Tunnelling transmission refers to a finite barrier with a classically allowed region on its far side.

5. Common traps

  1. Saying “the particle cannot be outside because E < V₀” (quantum mechanically it can, with small probability).
  2. Using sinusoidal solutions outside the well for E < V₀ (they should be exponential).
  3. Forgetting the continuity of both ψ and dψ/dx at boundaries.
  4. Confusing ψ with |ψ|².

6. Quick check

A. For a bound state (E < V₀), what is the qualitative form of the wavefunction outside the well?

Answer

Exponential decay, e.g. ψ ∝ e^(-κ x).

B. If V₀ increases while E stays the same, what happens to the tunnelling tail?

Answer

κ = square root of (2m(V₀-E))/ħ increases, so the wavefunction decays faster and the tail becomes shorter.

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Course and syllabus information
Course
Advanced Physics
Edition
Advanced Physics