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8.1: Approximate Solution of the Schrödinger Equation

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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|ΦΦ|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]=ijϕ|ii|ˆH|jj|ϕ=i|ϕ|i|2Ei=E0+i|ϕ|i|2(EiE0)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 (EiE0) 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.


This page titled 8.1: Approximate Solution of the Schrödinger Equation is shared under a CC BY 4.0 license and was authored, remixed, and/or curated by Graeme Ackland via source content that was edited to the style and standards of the LibreTexts platform.

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