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beginner · Physics · Quantum Tunneling & Barriers

Reflection and Transmission

When a quantum particle travels from a region of constant potential into a region with a different potential, the wavefunction does not simply continue undisturbed. Even when the particle has enough energy to enter the new region classically, quantum mechanics predicts partial reflection — a wholly non-classical effect with no analogue in Newtonian mechanics.

Setting up the problem

Consider a particle of mass mm and total energy EE moving in one dimension. For x<0x < 0 the potential is zero; for x0x \geq 0 the potential is V0V_0 with 0<V0<E0 < V_0 < E. The particle approaches from the left.

In each region the time-independent Schrödinger equation reduces to a free-particle equation:

22md2ψdx2=(EV)ψ.-\frac{\hbar^2}{2m}\frac{d^2\psi}{dx^2} = (E - V)\psi.

Defining the wave numbers

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

the general solutions are:

ψ1(x)=Aeik1x+Beik1x(x<0),\psi_1(x) = A e^{ik_1 x} + B e^{-ik_1 x} \quad (x < 0), ψ2(x)=Ceik2x(x0).\psi_2(x) = C e^{ik_2 x} \quad (x \geq 0).

The term Aeik1xA e^{ik_1 x} is the incident wave travelling right, Beik1xB e^{-ik_1 x} is the reflected wave travelling left, and Ceik2xC e^{ik_2 x} is the transmitted wave. We drop the left-going term in region 2 because there is nothing to reflect from on the right.

Boundary conditions

Continuity of ψ\psi and its derivative at x=0x = 0 gives two equations:

A+B=C,A + B = C, k1(AB)=k2C.k_1(A - B) = k_2 C.

Solving for the amplitude ratios:

BA=k1k2k1+k2,CA=2k1k1+k2.\frac{B}{A} = \frac{k_1 - k_2}{k_1 + k_2}, \qquad \frac{C}{A} = \frac{2k_1}{k_1 + k_2}.

Reflection and transmission coefficients

The physically meaningful quantities are the probability currents, not the amplitudes alone. The probability current for a plane wave eikxe^{ikx} is proportional to kk, so:

R=BA2=(k1k2k1+k2)2,R = \left|\frac{B}{A}\right|^2 = \left(\frac{k_1 - k_2}{k_1 + k_2}\right)^2, T=k2k1CA2=4k1k2(k1+k2)2.T = \frac{k_2}{k_1}\left|\frac{C}{A}\right|^2 = \frac{4k_1 k_2}{(k_1 + k_2)^2}.

Probability is conserved: R+T=1R + T = 1. We can verify this algebraically:

R+T=(k1k2)2+4k1k2(k1+k2)2=(k1+k2)2(k1+k2)2=1.R + T = \frac{(k_1-k_2)^2 + 4k_1 k_2}{(k_1+k_2)^2} = \frac{(k_1+k_2)^2}{(k_1+k_2)^2} = 1. \checkmark

A worked example

Let E=9eVE = 9\,\text{eV} and V0=5eVV_0 = 5\,\text{eV}. Then

k19=3,k295=2.k_1 \propto \sqrt{9} = 3, \qquad k_2 \propto \sqrt{9-5} = 2. R=(323+2)2=(15)2=0.04,R = \left(\frac{3-2}{3+2}\right)^2 = \left(\frac{1}{5}\right)^2 = 0.04, T=432(3+2)2=2425=0.96.T = \frac{4 \cdot 3 \cdot 2}{(3+2)^2} = \frac{24}{25} = 0.96.

Four percent of the probability is reflected even though the particle classically had more than enough energy to cross the step. This is a direct consequence of the wave nature of matter.

Try it

This is a numerical exercise — return a number. A particle with energy E=5eVE = 5\,\text{eV} hits a potential step of height V0=1eVV_0 = 1\,\text{eV}. Compute the reflection coefficient RR. (Hint: k1Ek_1 \propto \sqrt{E} and k2EV0k_2 \propto \sqrt{E - V_0}; the common proportionality constant cancels in the formula for RR.)

Run your code to see the quantum state.

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