Step potential

Step potential

The Schrödinger equation for a one dimensional step potential is a model system in quantum mechanics and scattering theory. The problem consists of solving the time-independent Schrödinger equation for a particle with a step-like potential in one dimension. Typically, the potential is modeled as a Heaviside step function.

Calculation

The time-independent Schrödinger equation for the wave function psi(x) reads

:Hpsi(x)= [-frac{hbar^2}{2m}frac{d^2}{dx^2}+V(x)] psi(x)=Epsi(x),

where H is the Hamiltonian, hbar is the (reduced)
Planck constant, m is the mass, E the energy of the particle and

:V(x)=V_0Theta(x)

is the potential step with height V_0 >0. Theta(x)=0,; x<0;; Theta(x)=1,; x>0 is the Heaviside step-function. The barrier is positioned at x=0. Withoutchanging the results, any other shifted position was possible.The first term in the Hamiltonian, -frac{hbar^2}{2m}frac{d^2}{dx^2}psi is the kinetic energy.

The step divides the space in two parts (x<0, x>0). In any of these parts the potential is constant meaning the particle is quasi-free, and the solution of the Schrödinger equation can be written as a superposition of left and right moving waves (see free particle)

:psi_L(x)= frac{1}{sqrt{k_0 left(A_r e^{i k_0 x} + A_l e^{-ik_0x} ight)quad x<0 , :psi_R(x)= frac{1}{sqrt{k_1 left(B_r e^{ k_1 x} + B_l e^{-k_1x} ight)quad x>0

where the wave vectors are related to the energy via

:k_0=sqrt{2m E/hbar^2}, and:k_1=sqrt{2m (V_0-E)/hbar^2}.

The index r/l on the coefficients A and B denotes the direction of the velocity vector. Note that for energies E, the wave function to the right of the step is exponentially decaying over a distance 1/(ik_1). Nevertheless we keep the notation r/l even though the waves are not propagating anymore in this case. The prefactor frac{1}{sqrt{k ensures a correct normalization of the probability flux.clarifyme

The coefficients A, B have to be found from the boundary conditions of the wave function at x=0. The wave function and its derivative have to be continuous everywhere, so.

:psi_L(0)=psi_R(0),:frac{d}{dx}psi_L(0) = frac{d}{dx}psi_R(0).

Inserting the wave functions, the boundary conditions give the following restrictions on the coefficients

:sqrt{k_1}(A_r+A_l)=sqrt{k_0}(B_r+B_l):sqrt{k_0}(A_r-A_l)=sqrt{k_1}(B_r-B_l),

Transmission and reflection

At this point, it is instructive to compare the situation to the classical case. In both cases, the particle behaves as a free particle outside of the barrier region. A classical particle with energy E larger than the barrier height V_0 does not feel the barrier at all, while a classical particle with E incident on the barrier from the left would always get reflected.

To study the quantum case, let us consider the following situation: a particle incident on the barrier from the left side (A_r). It may be reflected (A_l) or transmitted (B_r). Here and in the following assume E>V_0

To find the amplitudes for reflection and transmission for incidence from the left, we put in the above equations A_r=1 (incoming particle), A_l=r (reflection), B_l=0 (no incoming particle from the right) and B_r=t (transmission). We then solve the set of two linear equations for r, t.

The result is:

:t=frac{2sqrt{k_0k_1{k_0+k_1}:r=frac{k_0-k_1}{k_0+k_1}.

The model is symmetric with respect to a mirror transformation and at the same time exchange k_0leftrightarrow k_1. For incidence from the right we have therefore the amplitudes for transmission and reflection

:t'=t=frac{2sqrt{k_0k_1{k_0+k_1}:r'=-r=frac{k_1-k_0}{k_0+k_1}.

Analysis of the obtained expressions.

E

E>V_0

In this energy range the transmission and reflection coefficient differ from the classical case. They are the same for incidence from the left and right and read

:T=|t|^2=|t'|^2=frac{4k_0k_1}{(k_0+k_1)^2}:R=|r|^2=|r'|^2=1-T=frac{(k_0-k_1)^2}{(k_0+k_1)^2}

respectively. In the limit of large energies, Egg V_0, the classical result ("T=1", "R=0") is recovered.Thus there is a finite probability for a particle with an energy larger than the step height to be reflected.

Remarks, application

The Heaviside-step potential mainly serves as an exercise in quantum mechanics classes as the solution requires the understanding of a variety of concepts of quantum physics like normalization, matching of wave functions, reflection/transmission amplitudes, and probabilities.

A similar problem to the one considered appears in the physics of normal-metal superconductor interfaces. Quasiparticles are scattered at the pair potential which in the simplest model may be assumed to have a step-like shape. The solution of the Bogoliubov-de Gennes equation resembles that of the discussed Heaviside-step potential. In the superconductor normal-metal case this gives rise to Andreev reflection.

Step potential is the potential between any two equipotential rings. In the event electrical energy is impressed at a point such as a point on the earth’s surface, a current passes outward through materials including soil and concrete surrounding the point. The electrical resistance of the materials results in a diminishing potential as a function of the distance from the point receiving the electrical energy. In other words, a plurality of equipotential surfaces or rings of decreasing potential surrounds the point. Lightning is an example of impressing electrical energy at a point. A person standing near the point of the lightning strike and oriented between any two equipotential rings or across the potential gradient can likely incur an unsafe step potential between the feet or points of contact to the ground.

See also

*Finite potential well
*Infinite potential well
*Delta potential barrier (QM)
*Finite potential barrier (QM)


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