Quantum Well Energies

Consider a one-dimensional potential well containing a single particle. The particle has zero potential energy in the range ( 0 < x < 3 ) (0 < x < 3) , and infinite potential everywhere else (meaning that the particle is effectively trapped inside the well).

The behavior of the particle is governed by the time-independent Schrodinger equation:

α d 2 d x 2 Ψ ( x ) = E Ψ ( x ) \large{-\alpha \frac{d^2}{dx^2} \Psi(x) = E \, \Psi(x)}

In the above equation, Ψ ( x ) \Psi(x) is the particle's wave function, and E E is a constant representing the particle's total energy. The constant α \alpha contains Planck's constant as well as some other numbers.

Calculate the allowed values of E E using the following process:

1) Find a general solution for Ψ ( x ) \Psi(x)
2) Apply boundary conditions Ψ ( 0 ) = 0 \Psi(0) = 0 and Ψ ( 3 ) = 0 \Psi(3) = 0
3) Energy quantization is an implicit consequence of (1) and (2)

Let E 1 E_1 be the smallest non-zero energy the particle can have, and let E 2 E_2 be the second smallest value. These energies are related as follows:

E 2 E 1 = σ π 2 α \large{E_2 - E_1 = \sigma \, \pi^2 \, \alpha}

Determine the value of σ \sigma

Note: Thanks to Laszlo Mihaly for his illuminating commentary on my previous problem


The answer is 0.3333.

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2 solutions

Steven Chase
Jan 21, 2019

Writing the 1D SE:

α d 2 d x 2 Ψ = E Ψ d 2 d x 2 Ψ = E α Ψ \large{-\alpha \frac{d^2}{dx^2} \Psi = E \, \Psi \\ \frac{d^2}{dx^2} \Psi = -\frac{E}{\alpha} \, \Psi}

The general solution should be:

Ψ = A e j E / α x + B e j E / α x \large{\Psi = A \, e^{j \, \sqrt{E/\alpha} \, x} + B \, e^{-j \, \sqrt{E/\alpha} \, x}}

Assuming that the infinite potentials outside the well impose the conditions that Ψ ( 0 ) = 0 \Psi(0) = 0 and Ψ ( ) = 0 \Psi(\ell) = 0 , we have the following.

0 = A + B B = A 0 = e j E / α e j E / α e j E / α = e j E / α \large{0 = A + B \implies B = -A \\ 0 = e^{j \, \sqrt{E/\alpha} \, \ell} - \, e^{-j \, \sqrt{E/\alpha} \, \ell} \\ e^{j \, \sqrt{E/\alpha} \, \ell} = e^{-j \, \sqrt{E/\alpha} \, \ell} }

By inspection, the last equation is only satisfied when:

E α = ± n π \large{\sqrt{\frac{E}{\alpha}} \, \ell = \pm \, n \, \pi}

In the above equation, n n is an integer. The corresponding energy expression is:

E = n 2 π 2 2 α \large{E = \frac{n^2 \, \pi^2}{\ell^2} \alpha}

Thus, the boundary conditions on Ψ \Psi , combined with the Schrodinger equation, give rise to discrete energy levels in quantum mechanics.

In this case, = 3 \ell = 3 , so the difference between the two lowest energy levels is:

E 2 E 1 = π 2 9 ( 2 2 1 2 ) α = 1 3 π 2 α \large{E_2 - E_1 = \frac{\pi^2}{9} (2^2 - 1^2) \alpha = \frac{1}{3} \pi^2 \, \alpha}

Mark Hennings
Jan 18, 2019

Writing E = α k 2 E = \alpha k^2 we obtain the differential equation ψ ( x ) + k 2 ψ ( x ) = 0 \psi''(x) + k^2\psi(x) \; = \; 0 together with the boundary conditions ψ ( 0 ) = ψ ( 3 ) = 0 \psi(0) = \psi(3) =0 . Thus we deduce that ψ ( x ) = A sin k x \psi(x) =A\sin kx where sin 3 k = 0 \sin3k = 0 . Thus we deduce that k = 1 3 n π k = \tfrac13n\pi where n Z n \in \mathbf{Z} . We cannot have n = 0 n=0 , since that would make ψ 0 \psi \equiv 0 . Negative values of n n just return the same wave functions as positive ones. Thus we can assume that k = 1 3 π n k = \tfrac13\pi n for n N n \in \mathbb{N} , and we obtain energy levels E n = 1 9 n 2 π 2 α E_n \; = \; \tfrac19 n^2 \pi^2 \alpha for n N n \in \mathbb{N} , and so E 2 E 1 = 1 3 π 2 α E_2 - E_1 = \tfrac13\pi^2\alpha , making the answer 1 3 \boxed{\tfrac13} .

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