Skip to article frontmatterSkip to article content

Problem Sheet: Week 10

School of Physics, University of Bristol

Infinite Square Well

  1. In this question we will find the momentum wavefunctions associated to the energy eigenstates of the infinite square well. Recall that the spatial wavefunctions of the energy eigenstates are given by

    un(x)=2asin(nπxa),u_n(x) = \sqrt{\frac{2}{a}} \sin \left(\frac{n \pi x}{a}\right),

    for 0xa0 \leq x \leq a, and un(x)=0u_n(x) = 0 otherwise.

    1. Show that the momentum wavefunction u~n(p)\tilde{u}_n(p) associated to un(x)u_n(x) is given by

      u~n(p)=πann2π2a2p2/2(1(1)neiap/).\tilde{u}_n(p) = \sqrt{\frac{\pi a}{\hbar}}\frac{n}{n^2 \pi^2 - a^2p^2/\hbar^2}(1-(-1)^ne^{-iap/\hbar}).
    2. For n=1n = 1 and n=2n = 2, i.e. for the ground state and first excited state, sketch the real and imaginary parts of the momentum wavefunctions, and also the momentum probability density.

  2. Consider a particle confined inside an infinite square well of width aa. The wavefunction of the particle is

    Ψ(x)={3a3xif 0x<a,0otherwise. \Psi(x) = \begin{cases} \sqrt{\frac{3}{a^3}}x& \text{if } 0 \leq x < a, \\ 0 &\text{otherwise. } \end{cases}
    1. Sketch the wavefunction Ψ(x)\Psi(x) and confirm that it is normalised.

    In this Problem we would like to write this wavefunction as a superposition of the energy eigenstates of the infinite square well. That is, we would like to write Ψ(x)\Psi(x) as

    Ψ(x)=n=1cnun(x), \Psi(x) = \sum_{n=1}^{\infty} c_n u_n(x),

    where un(x)=2asin(nπxa) u_n(x) = \sqrt{\frac{2}{a}}\sin \left(\frac{n\pi x}{a}\right) for 0xa0 \leq x \leq a, and un(x)=0u_n(x) = 0 otherwise.

    1. Show that the amplitude cnc_n is given by

      cn=6(1)nnπ. c_n = - \frac{\sqrt{6} (-1)^n}{n\pi}.
    2. What are the probabilities for the particle to have the energies E1E_1, E2E_2 and E3E_3, where En=2π2n2/2ma2E_n = \hbar^2\pi^2n^2/2ma^2 are the energy levels of the infinite square well?

    3. What is the probability for the particle to have energy at least E4E_4?

  3. In this question we will consider an approximation to the wavefunction from Problem 10.2, and study its evolution. One way to approximate a wavefunction is to consider only the amplitudes which have largest modulus. Therefore, consider the following initial wavefunction for a particle,

    Ψ(x,0)=A6π(u1(x)12u2(x)+13u3(x)),\Psi(x,0) = A \frac{\sqrt{6}}{\pi}\left(u_1(x) - \frac{1}{2}u_2(x) + \frac{1}{3}u_3(x) \right),

    where AA is a normalisation constant.

    1. Find the normalisation constant AA.
    1. Make a sketch of the wavefunction Ψ(x,0)\Psi(x,0).
    2. Write down Ψ(x,t)\Psi(x,t), the wavefunction of the particle at time tt.
    3. Show that the wavefunction of the particle returns to the form it has at t=0t = 0 whenever the time is a multiple of the period T=2π/ωT = 2\pi/\omega, where
      ω=π22Ma2. \omega = \frac{\hbar \pi^2}{2 M a^2}.
      That is, show that Ψ(x,mT)=Ψ(x,0)\Psi(x,mT) = \Psi(x,0), where mm is an integer.