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beginner · Physics · Quantum Tunneling & Barriers

Finite Potential Step

Classical physics says that a particle with enough energy clears a step and a particle without it bounces back. Quantum mechanics says something richer: even when the particle has more energy than the step, there is a non-zero probability of reflection. Setting up the problem carefully is the first step toward understanding this, and toward the far stranger phenomenon of tunneling through a barrier.

The potential

Place a step potential along the xx-axis:

V(x)={0x<0(region I),V0x0(region II),V(x) = \begin{cases} 0 & x < 0 \quad \text{(region I)}, \\ V_0 & x \geq 0 \quad \text{(region II)}, \end{cases}

where V0>0V_0 \gt 0 is the height of the step. A particle of mass mm and total energy EE travels from left to right. We focus on the over-barrier case E>V0E \gt V_0 first.

The stationary-state approach

Because the potential is piecewise constant, the time-independent Schrödinger equation

22md2ψdx2+V(x)ψ(x)=Eψ(x)-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2} + V(x)\,\psi(x) = E\,\psi(x)

reduces to a simple second-order ODE with constant coefficients in each region. Define two wave-numbers:

k1=2mE,k2=2m(EV0).k_1 = \frac{\sqrt{2mE}}{\hbar}, \qquad k_2 = \frac{\sqrt{2m(E - V_0)}}{\hbar}.

Both k1k_1 and k2k_2 are real and positive when E>V0E \gt V_0. In region I the general solution is a superposition of a right-moving incident wave and a left-moving reflected wave:

ψI(x)=Aeik1x+Beik1x.\psi_\text{I}(x) = A\,e^{ik_1 x} + B\,e^{-ik_1 x}.

In region II, which extends to x+x \to +\infty, there is no surface to reflect from, so only a transmitted wave propagates to the right:

ψII(x)=Ceik2x.\psi_\text{II}(x) = C\,e^{ik_2 x}.

The amplitudes AA, BB, and CC are complex numbers. By convention AA is treated as known (the incoming beam is prepared with amplitude AA), and we solve for BB and CC.

Matching conditions at the boundary

The wave function and its first derivative must both be continuous everywhere, including at the step at x=0x = 0. Continuity of ψ\psi:

A+B=C.A + B = C.

Continuity of dψ/dxd\psi/dx:

ik1(AB)=ik2C.ik_1(A - B) = ik_2\,C.

These two equations in two unknowns (BB and CC) are the entire algebra of the problem. Solving them gives

B=k1k2k1+k2A,C=2k1k1+k2A.B = \frac{k_1 - k_2}{k_1 + k_2}\,A, \qquad C = \frac{2k_1}{k_1 + k_2}\,A.

Why reflection occurs at all

Classically, a particle with E>V0E \gt V_0 always passes the step; reflection is impossible. Quantum mechanically, B0B \neq 0 whenever k1k2k_1 \neq k_2, i.e., whenever V00V_0 \neq 0. The physical reason is that the wave-number changes abruptly at x=0x = 0: the wave is propagating at wavelength λ1=2π/k1\lambda_1 = 2\pi/k_1 on the left and λ2=2π/k2\lambda_2 = 2\pi/k_2 on the right. Whenever two media with different propagation speeds meet at a sharp boundary, partial reflection is inevitable — this is the same physics that partially reflects light at a glass surface, expressed in wave mechanics.

Sub-barrier case and the approach to tunneling

When E<V0E \lt V_0 the quantity EV0E - V_0 is negative, so k2k_2 would be imaginary. Write κ=2m(V0E)/\kappa = \sqrt{2m(V_0 - E)}/\hbar (real, positive). The solution in region II becomes an evanescent (exponentially decaying) wave:

ψII(x)=Ceκx,x0.\psi_\text{II}(x) = C\,e^{-\kappa x}, \quad x \geq 0.

The matching conditions still hold, and the algebra shows B=A|B| = |A|: the step reflects the particle with probability 1, matching the classical prediction. However, ψII\psi_\text{II} is not zero — the wave function penetrates into the classically forbidden region with a characteristic length 1/κ1/\kappa.

This penetration depth is the seed of tunneling: if region II has finite width rather than extending to infinity, the wave function can reach the far side before decaying to zero, and transmission becomes possible. That scenario — the rectangular barrier — is the subject of the next lesson.

Summary of the setup

The finite potential step is solved in three moves:

  1. Write down k1k_1 and k2k_2 (or κ\kappa in the sub-barrier case) from the kinetic energy in each region.
  2. Write the most general wave function in each region consistent with the boundary conditions at infinity (no incoming wave from the right).
  3. Match ψ\psi and ψ\psi' at x=0x = 0 to find the reflection and transmission amplitudes.

The reflection coefficient R=B/A2R = |B/A|^2 and the transmission coefficient T=(k2/k1)C/A2T = (k_2/k_1)|C/A|^2 will be derived in the next lesson; they satisfy R+T=1R + T = 1 as required by probability conservation.

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