8.1: Approximate Solution of the Schrödinger Equation
( \newcommand{\kernel}{\mathrm{null}\,}\)
If we can’t find an analytic solution to the Schrödinger equation, a trick known as the variational principle allows us to estimate the energy of the ground state of a system. We choose an unnormalized trial function Φ(an) which depends on some variational parameters, an and minimise
E[an]=⟨Φ|ˆH|Φ⟩⟨Φ|Φ⟩
with respect to those parameters. This gives an approximation to the wavefunction whose accuracy depends on the number of parameters and the clever choice of Φ(an). For more rigorous treatments, a set of basis functions with expansion coefficients an may be used.
The proof is as follows, if we expand the normalised wavefunction
|ϕ(an)⟩=Φ(an)/⟨Φ(an)|Φ(an)⟩1/2
in terms of the true (unknown) eigenbasis |i⟩ of the Hamiltonian, then its energy is
E[an]=∑ij⟨ϕ|i⟩⟨i|ˆH|j⟩⟨j|ϕ⟩=∑i|⟨ϕ|i⟩|2Ei=E0+∑i|⟨ϕ|i⟩|2(Ei−E0)≥E0
where the true (unknown) ground state of the system is defined by ˆH|i0⟩=E0|i0⟩. The inequality arises because both |⟨ϕ|i⟩|2 and (Ei−E0) must be positive.
Thus the lower we can make the energy E[ai], the closer it will be to the actual ground state energy, and the closer |ϕ⟩ will be to |i0⟩.
If the trial wavefunction consists of a complete basis set of orthonormal functions |χi⟩, each multiplied by ai:|ϕ⟩=∑iai|χi⟩ then the solution is exact and we just have the usual trick of expanding a wavefunction in a basis set. Alternately, we might just use an incomplete set with a few low-energy basis functions to get a |Φ⟩ close to the ground state |i0⟩. In practice, this is how most quantum mechanics problems are solved.