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intermediate · Physics · The Variational Method & WKB

Linear Variational Method

So far each trial state had a parameter that entered nonlinearly (a Gaussian width, an effective charge). The linear variational method instead writes the trial state as a linear combination of fixed basis functions and optimizes the coefficients. The magic is that minimizing over linear coefficients is exact and reduces to a matrix eigenvalue problem.

A basis-expansion trial state

Pick NN fixed, linearly independent functions { ∣χk⟩ }\{\,|\chi_k\rangle\,\} and write

∣ψ⟩=∑k=1Nck ∣χk⟩.|\psi\rangle = \sum_{k=1}^{N} c_k\, |\chi_k\rangle .

The coefficients ckc_k are the variational parameters. Define the Hamiltonian matrix and overlap matrix

Hjk=⟨χj∣H^∣χk⟩,Sjk=⟨χj∣χk⟩.H_{jk} = \langle \chi_j | \hat{H} | \chi_k \rangle, \qquad S_{jk} = \langle \chi_j | \chi_k \rangle .

If the basis is orthonormal, Sjk=δjkS_{jk} = \delta_{jk} and the overlap drops out.

The secular equation

Minimizing the Rayleigh quotient E=c†Hcc†ScE = \dfrac{\mathbf{c}^\dagger H \mathbf{c}}{\mathbf{c}^\dagger S \mathbf{c}} over the coefficients c\mathbf{c} leads to the generalized eigenvalue problem

H c=E S c,H\,\mathbf{c} = E\, S\, \mathbf{c},

with non-trivial solutions only when the secular determinant vanishes:

det⁡(H−ES)=0.\det(H - E S) = 0 .

For an orthonormal basis this is just det⁡(H−E 1)=0\det(H - E\,\mathbb{1}) = 0 — the ordinary eigenvalue equation. The NN roots E1≤E2≤⋯≤ENE_1 \leq E_2 \leq \dots \leq E_N are the linear variational energies. The smallest, E1E_1, is the best variational estimate of the ground state; remarkably, E2,…E_2, \dots are upper bounds on the excited states too (the Hylleraas–Undheim / MacDonald theorem).

The two-dimensional case

With two orthonormal basis states the Hamiltonian matrix is a real symmetric 2×22\times 2 matrix

H=(abbd),H = \begin{pmatrix} a & b \\ b & d \end{pmatrix},

and the secular equation det⁡(H−E 1)=0\det(H - E\,\mathbb{1}) = 0 gives the quadratic (a−E)(d−E)−b2=0(a-E)(d-E) - b^2 = 0, whose roots are

E±=a+d2±(a−d2)2+b2.E_\pm = \frac{a+d}{2} \pm \sqrt{\left(\frac{a-d}{2}\right)^2 + b^2}.

The off-diagonal coupling bb pushes the levels apart: the lower root E−E_- drops below the smaller diagonal entry. This level repulsion is the variational improvement over using a single basis state.

Try it

For H=(1113)H = \begin{pmatrix} 1 & 1 \\ 1 & 3 \end{pmatrix}, compute and return the lower eigenvalue — the best two-state variational estimate of the ground-state energy.

Run your code to see the quantum state.

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