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Numerical Methods in Quantum Mechanics - Dipartimento di Fisica

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This demonstrates Eq.(4.19), s<strong>in</strong>ce the second term is either positive or zero,<br />

as E n ≥ E 0 by def<strong>in</strong>ition of ground state,<br />

This simple result is extremely important: it tells us that any function ψ,<br />

yields for the expectation energy an upper estimate of the energy of the ground<br />

state. If the ground state is unknown, an approximation to the ground state<br />

can be found by vary<strong>in</strong>g ψ <strong>in</strong>side a given set of functions and look<strong>in</strong>g for the<br />

function that m<strong>in</strong>imizes 〈H〉. This is the essence of the variational method.<br />

4.1.4 Variational method <strong>in</strong> practice<br />

One identifies a set of trial wave functions ψ(v; α 1 , . . . , α r ), where v are the<br />

variables of the problem (coord<strong>in</strong>ates etc), α i , i = 1, . . . , r are parameters. The<br />

energy eigenvalue will be a function of the parameters:<br />

∫<br />

E(α 1 , . . . , α r ) = ψ ∗ Hψ dv (4.22)<br />

The variational method consists <strong>in</strong> look<strong>in</strong>g for the m<strong>in</strong>imum of E with respect<br />

to a variation of the parameters, that is, by impos<strong>in</strong>g<br />

∂E<br />

∂α 1<br />

= . . . = ∂E<br />

∂α r<br />

= 0 (4.23)<br />

The function ψ satisfy<strong>in</strong>g these con<strong>di</strong>tions with the lowest E is the function<br />

that better approximates the ground state, among the considered set of trial<br />

functions.<br />

It is clear that a suitable choice of the trial functions plays a crucial role<br />

and must be carefully done.<br />

4.2 Secular problem<br />

The variational method can be reduced to an algebraic problem by expand<strong>in</strong>g<br />

the wave function <strong>in</strong>to a f<strong>in</strong>ite basis of functions, and apply<strong>in</strong>g the variational<br />

pr<strong>in</strong>ciple to f<strong>in</strong>d the optimal coefficients of the expansion. Based on Eq. (4.10),<br />

this means calculat<strong>in</strong>g the functional (i.e. a “function” of a function):<br />

G[ψ] = 〈ψ|H|ψ〉 − ɛ〈ψ|ψ〉<br />

∫<br />

∫<br />

= ψ ∗ Hψ dv − ɛ ψ ∗ ψ dv (4.24)<br />

and impos<strong>in</strong>g the stationary con<strong>di</strong>tion on G[ψ]. Such procedure produces an<br />

equation for the expansion coefficients that we are go<strong>in</strong>g to determ<strong>in</strong>e.<br />

It is important to notice that our basis is formed by a f<strong>in</strong>ite number N of<br />

functions, and thus cannot be a complete system: <strong>in</strong> general, it is not possible<br />

to write any function ψ (<strong>in</strong>clud<strong>in</strong>g exact solutions of the Schröd<strong>in</strong>ger equation)<br />

as a l<strong>in</strong>ear comb<strong>in</strong>ation of the functions <strong>in</strong> this basis set. What we are go<strong>in</strong>g to<br />

do is to f<strong>in</strong>d the ψ function that better approaches the true ground state, among<br />

all functions that can be expressed as l<strong>in</strong>ear comb<strong>in</strong>ations of the N chosen basis<br />

functions.<br />

35

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