Paper 2, Section II, C

Applications of Quantum Mechanics
Part II, 2017

Give an account of the variational method for establishing an upper bound on the ground-state energy of a Hamiltonian HH with a discrete spectrum Hn=EnnH|n\rangle=E_{n}|n\rangle, where EnEn+1,n=0,1,2E_{n} \leqslant E_{n+1}, n=0,1,2 \ldots

A particle of mass mm moves in the three-dimensional potential

V(r)=AeμrrV(r)=-\frac{A e^{-\mu r}}{r}

where A,μ>0A, \mu>0 are constants and rr is the distance to the origin. Using the normalised variational wavefunction

ψ(r)=α3πeαr\psi(r)=\sqrt{\frac{\alpha^{3}}{\pi}} e^{-\alpha r}

show that the expected energy is given by

E(α)=2α22m4Aα3(μ+2α)2E(\alpha)=\frac{\hbar^{2} \alpha^{2}}{2 m}-\frac{4 A \alpha^{3}}{(\mu+2 \alpha)^{2}}

Explain why there is necessarily a bound state when μ<Am/2\mu<A m / \hbar^{2}. What can you say about the existence of a bound state when μAm/2\mu \geqslant A m / \hbar^{2} ?

[Hint: The Laplacian in spherical polar coordinates is

2=1r2r(r2r)+1r2sinθθ(sinθθ)+1r2sin2θ2ϕ2]\left.\nabla^{2}=\frac{1}{r^{2}} \frac{\partial}{\partial r}\left(r^{2} \frac{\partial}{\partial r}\right)+\frac{1}{r^{2} \sin \theta} \frac{\partial}{\partial \theta}\left(\sin \theta \frac{\partial}{\partial \theta}\right)+\frac{1}{r^{2} \sin ^{2} \theta} \frac{\partial^{2}}{\partial \phi^{2}}\right]