Time Independent Perturbation Theory

Consider the time independent Schrödinger equation,R2(453)

$\displaystyle \hat{H} \phi_n(x) = E_n \phi_n(x),$ (10)

for a system described by the Hamiltonian $ \hat{H}=\hat{p}^2/2m +\hat{V}$, and assume that all the eigenfunctions $ \phi_n(x)$ are known. The goal of this section is to show that these eigenfunctions $ \phi_n(x)$ can be used to solve the time independent Schrödinger equation of a slightly different problem: a problem described by the Hamiltonian $ \hat{H'}=\hat{H}+\lambda \hat{\omega}$. This is accomplished by implementing the equations of Perturbation Theory derived in this section.

Consider the equation

$\displaystyle (\hat{H} + \lambda \hat{\omega}) \tilde{\Phi}_n(\lambda ,x) = \tilde{E}_n(\lambda) \tilde{\Phi}_n(\lambda , x),$ (11)

where $ \lambda$ is a small parameter, so that both $ \tilde{\Phi}_n(\lambda)$ and $ \tilde{E}_n(\lambda)$ are well approximated by rapidly convergent expansions in powers of $ \lambda$ (i.e., expansions where only the first few terms are important).

Expanding $ \tilde{\Phi}_n(\lambda)$ we obtain,

$\displaystyle \tilde{\Phi}_n(\lambda , x) = \sum_j {C_{jn}(\lambda) \phi_j(x)}.$

Substituting this expression in the time independent Schrödinger equation we obtain,

$\displaystyle \sum_j {C_{jn}(\lambda) [\hat{H} \phi_j(x) + \lambda \hat{\omega} \phi_j (x)]} = \tilde{E_n}(\lambda) \sum_k {C_{kn}{(\lambda)} \phi_k(x)}.,$

therefore,

$\displaystyle C_{ln}(\lambda) E_l + \lambda \sum_j C_{jn}(\lambda)<\phi_l\vert\hat{\omega}\vert\phi_j> = \tilde{E_n}(\lambda) C_{ln}(\lambda).$ (12)

Expanding $ C_{kj}$ and $ E_n$ in powers of $ \lambda$ we obtain,

$ C_{kj}(\lambda)= C_{kj}^{(0)} + C_{kj}^{(1)}\lambda + C_{kj}^{(2)} \lambda^2 + ...,$

and

$ \tilde{E}_n(\lambda) = E_n^{(0)} + E_n^{(1)}\lambda + E_n^{(2)} \lambda^2 + ...$

Substituting these expansions into Eq. (12) we obtain,

$ (C_{ln}^{(0)}E_l^{(0)} -E_n C_{ln}^{(0)}) + \lambda(C_{ln}^{(1)}E_l + \sum_j C...
... - E_n^{(2)} C_{ln}^{(0)} -E_n C_{ln}^{(2)} -E_n^{(1)}C_{ln}^{(1)} ) + ... = 0.$

This equation must be valid for any $ \lambda$. Therefore, each of the terms in between parenthesis must be equal to zero.

Zeroth order in $ \lambda$ \begin{displaymath}
\begin{cases}
C_{ln}^{(0)} (E_l^{(0)} -E_n) =0, \\ \text{if...
...C_{nn}^{(0)} =1, \ \text{and} \ E_l^{(0)} =E_n. \\
\end{cases}\end{displaymath}

First order in $ \lambda$ \begin{displaymath}
\begin{cases}
C_{ln}^{(1)}(E_l -E_n) = E_n^{(1)}C_{ln}^{(0)...
..._{nn}^{(0)}<\phi_n\vert\hat{\omega}\vert\phi_n>.\\
\end{cases}\end{displaymath}

Note that $ C_{nn}^{(1)}$ is not specified by the equations listed above. $ C_{nn}^{(1)}$ is obtained by normalizing the wave function written to first order in $ \lambda$.

2nd order in $ \lambda$ \begin{displaymath}
\begin{cases}
C_{ln}^{(2)}(E_l -En) + \sum_j C_{jn}^{(1)}<\p...
...phi_l\vert\hat{\omega}\vert\phi_n>}{(E_l -E_n)}.\\
\end{cases}\end{displaymath}

Exercise 9: Calculate the energy shifts to first order in $ \lambda$ for all excited states of the perturbed particle in the box described by the following potential:


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Assume that the potential is described by perturbation $ W(x)=$Sin$ (\frac{\pi x}{a})$ to the particle in the box.