Physic Labs

Quantum mechanics

The particle in a box and quantum tunneling

An infinite well has discrete energy levels; for a finite barrier the wavefunction decays but remains nonzero beyond it, giving a tunneling probability.

Potential energy determines where classical motion is allowed, but the Schrödinger equation permits a wavefunction to extend into classically forbidden regions. Two basic models are the infinite well, which illustrates quantization, and the finite barrier, which illustrates tunneling.

En=n2π2ℏ22mL2,ψn(x)=2Lsin⁡nπxL;T≈e−2κa,κ=2m(V0−E)ℏE_n=\frac{n^2\pi^2\hbar^2}{2mL^2},\quad\psi_n(x)=\sqrt{\frac2L}\sin\frac{n\pi x}{L};\qquad T\approx e^{-2\kappa a},\quad\kappa=\frac{\sqrt{2m(V_0-E)}}{\hbar}

Definition: One-dimensional infinite well

For V=0V=0 on 0<x<L0<x<L and V=∞V=\infty outside, boundary conditions ψ(0)=ψ(L)=0\psi(0)=\psi(L)=0 allow only wave numbers kn=nπ/Lk_n=n\pi/L (n=1,2,...n=1,2,...). The ground-state energy is nonzero: a confined particle cannot have both zero position spread and zero momentum.

Change level nn to see standing-wave nodes and En∝n2E_n∝n²; switch to a finite barrier to observe a wave packet transmitted with reduced amplitude.

Penetrating a finite barrier

For a rectangular barrier of height V0V_0 and width aa, with E<V0E<V_0, the solution decays in the barrier as e−κxe^{-\kappa x}. Exact transmission also depends on matching at both boundaries; T≈e−2κaT\approx e^{-2\kappa a} is a WKB approximation for a sufficiently thick/high barrier, not an exact formula in every case.

Example: Ground-state energy in a box

An electron is confined in a 1D box of length L=1.00L=1.00 nm. Find E1E_1 in eV.

Solution

E1=h2/(8meL2)=6.02×10−20E_1=h^2/(8m_eL^2)=6.02\times10^{-20} J =0.376=0.376 eV.

For a particle with E<V0E<V_0 incident on a barrier of height V0V_0, the Schrödinger equation gives an evanescent solution in the forbidden region. For a rectangular barrier of width aa, transmission decreases approximately as T∝e−2κaT\propto e^{-2\kappa a}, where κ=2m(V0−E)/ℏ\kappa=\sqrt{2m(V_0-E)}/\hbar. A wider barrier or heavier particle therefore makes tunneling less likely. For a light particle and a thin barrier, the probability remains finite. This underlies scanning tunneling microscopes and alpha decay; the ideal one-dimensional model must be distinguished from a real material's structure.

Quick check

In a 1D infinite well, how does level nn energy scale?

For E<V0E<V_0, what is the qualitative form of the wavefunction inside a rectangular barrier?

References

  1. David J. Griffiths, Darrell F. Schroeter (2018). Introduction to Quantum Mechanics