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 H∣n⟩=En∣n⟩H|n\rangle=E_{n}|n\rangle, where En⩽En+1,n=0,1,2…E_{n} \leqslant E_{n+1}, n=0,1,2 \ldots

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

V(r)=−Ae−μrrV(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)=α3πe−αr\psi(r)=\sqrt{\frac{\alpha^{3}}{\pi}} e^{-\alpha r}

show that the expected energy is given by

E(α)=ℏ2α22m−4Aα3(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/ℏ2\mu<A m / \hbar^{2}. What can you say about the existence of a bound state when μ⩾Am/ℏ2\mu \geqslant A m / \hbar^{2} ?

[Hint: The Laplacian in spherical polar coordinates is

∇2=1r2∂∂r(r2∂∂r)+1r2sin⁡θ∂∂θ(sin⁡θ∂∂θ)+1r2sin⁡2θ∂2∂ϕ2]\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]

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