Perturbation Theory Practice Problems

Working through classic perturbation theory homework problems — delta-function bumps in infinite square wells and harmonic oscillator perturbations, step by step.

These exercises focus on the basic machinery of time-independent perturbation theory rather than hydrogen fine structure, the Zeeman effect, or hyperfine structure. Our professor emphasized this material, so we worked through a lot of examples. Here are three of them.

Problem 6.1: a delta-function bump in an infinite square well

Consider an infinite square well on $0\lt x\lt a$ with a delta-function perturbation of strength $\alpha$ at the center:

The perturbation is H prime equals alpha times delta of x minus a over 2

(a) First-order energy correction

For the unperturbed well,

The normalized infinite-well eigenfunction and unperturbed energy E n zero

or, in accessible notation,

$$ \psi_n^{(0)}(x)=\sqrt{\frac{2}{a}}\sin\!\left(\frac{n\pi x}{a}\right), \qquad E_n^{(0)}=\frac{\hbar^2\pi^2n^2}{2Ma^2}, $$

where $M$ is the particle mass. The first-order correction is the expectation value of $H'$:

First-order delta-perturbation calculation giving 2 alpha over a times sine squared of n pi over 2

Thus

$$ E_n^{(1)}=\langle n|H^{\prime}|n\rangle=\frac{2\alpha}{a}\sin^2\!\left(\frac{n\pi}{2}\right)=\begin{cases}2\alpha/a,&n\ \text{odd},\cr 0,&n\ \text{even}.\end{cases} $$

The even-$n$ states vanish at $x=a/2$, so a delta function placed there has zero overlap with them. That node is the simple reason their first-order energies do not move.

(b) First three nonzero terms in the ground-state wavefunction correction

We want the first-order correction to the ground-state wavefunction,

The symbol psi 1 superscript 1 for the first-order ground-state wavefunction correction

which is expanded as

General sum for the first-order correction to state 1 over unperturbed states m

The standard nondegenerate formula is

$$ |1^{(1)}\rangle =\sum_{m\ne1} \frac{\langle m^{(0)}|H'|1^{(0)}\rangle} {E_1^{(0)}-E_m^{(0)}}|m^{(0)}\rangle. $$

The handwritten calculation is preserved below as part of the original working.

Handwritten evaluation of the delta-function matrix elements for the ground-state correction

At the center of the well,

$$ \langle m^{(0)}|H'|1^{(0)}\rangle =\frac{2\alpha}{a}\sin\!\left(\frac{m\pi}{2}\right). $$

Only odd $m$ survive, and $m=1$ is excluded from the sum. Writing the particle mass as $M$ to avoid confusing it with the summation index, the first three nonzero terms are therefore

$$ |1^{(1)}\rangle =\frac{M\alpha a}{\hbar^2\pi^2} \left( \frac12|3^{(0)}\rangle -\frac16|5^{(0)}\rangle +\frac1{12}|7^{(0)}\rangle +\cdots \right). $$

This native expression is the corrected result to use. The preserved handwritten image appears to start from an even intermediate state and gives coefficients that do not follow from the displayed matrix element; those are source-working errors, not steps being endorsed here.

Problem 6.2: changing the spring constant

For the simple harmonic oscillator,

Harmonic-oscillator potential V of x and unperturbed energy E n zero

$$ V(x)=\frac12kx^2, \qquad E_n^{(0)}=\left(n+\frac12\right)\hbar\omega, \qquad \omega=\sqrt{\frac{k}{M}}. $$

Now perturb the spring constant according to

The spring constant changes from k to k times one plus epsilon

so that $k\mapsto k(1+\varepsilon)$.

Exact expansion

The exact frequency becomes $\omega'=\omega\sqrt{1+\varepsilon}$, hence

Expansion of the oscillator energy after k changes to k times one plus epsilon

The correct Taylor series is

$$ E_n =\left(n+\frac12\right)\hbar\omega\sqrt{1+\varepsilon} =E_n^{(0)}\left(1+\frac{\varepsilon}{2}-\frac{\varepsilon^2}{8} +\frac{\varepsilon^3}{16}+O(\varepsilon^4)\right). $$

The preserved image labels the green term as second order but prints $-\varepsilon^3/8$. That exponent is a source-image typo: the second-order term is $-\varepsilon^2/8$.

Perturbative check

The next source image writes $H_0+H'$ as though it were only the perturbed quadratic potential:

Source image labeling the perturbed potential alone as H zero plus H prime and then evaluating the first-order correction

That displayed equality omits the unchanged kinetic term and is not a complete Hamiltonian identity. It is valid only for the potential-energy part. The full Hamiltonian and its perturbation are

$$ H_0+H'=\frac{p^2}{2M}+\frac12k(1+\varepsilon)x^2, \qquad H'=\frac12\varepsilon kx^2 =\frac{\varepsilon\hbar\omega}{4}(a+a^\dagger)^2. $$

Using $\langle n|x^2|n\rangle=\hbar(n+\tfrac12)/(M\omega)$ gives

$$ E_n^{(1)} =\frac{\varepsilon}{2}\left(n+\frac12\right)\hbar\omega =\frac{\varepsilon}{2}E_n^{(0)}. $$

For second order, $x^2$ connects $|n\rangle$ only to $|n\pm2\rangle$ off the diagonal. The two contributions give

$$ E_n^{(2)} =\sum_{m\ne n}\frac{|\langle m|H'|n\rangle|^2}{E_n^{(0)}-E_m^{(0)}} =-\frac{\varepsilon^2}{8}\left(n+\frac12\right)\hbar\omega =-\frac{\varepsilon^2}{8}E_n^{(0)}, $$

in agreement with the corrected exact expansion.

Problem 6.5: a charged oscillator in a weak electric field

Consider a particle of charge $q$ in a one-dimensional harmonic-oscillator potential. A constant weak electric field $\mathcal E$ adds

$$ H'=-q\mathcal E x. $$

We will show that the first-order correction vanishes, calculate the second-order correction, and then verify the result by solving the shifted oscillator exactly.

(a) Perturbation theory

The first-order correction is introduced in the preserved source as follows:

Source first-order Stark calculation, including the incorrect claim that every nth oscillator wavefunction is even

The image’s claim that every $\psi_n$ is even is incorrect: oscillator eigenfunctions have parity $(-1)^n$, so odd-$n$ wavefunctions are odd. What is even for every number state is the probability density $|\psi_n(x)|^2$. Therefore the integrand $x|\psi_n(x)|^2$ is odd, and

$$ E_n^{(1)}=-q\mathcal E\langle n|x|n\rangle=0. $$

The next preserved image has already moved to second order; it is not another first-order parity argument:

Second-order perturbation formula for the electric-field interaction together with the unperturbed oscillator energies

For the second-order correction,

Second-order perturbation formula specialized to the electric-field interaction

$$ E_n^{(2)} =q^2\mathcal E^2\sum_{m\ne n} \frac{|\langle m|x|n\rangle|^2}{E_n^{(0)}-E_m^{(0)}}. $$

Direct integration with oscillator wavefunctions is possible, but ladder operators are cleaner. The preserved reminder below labels a Gaussian-only expression as the general $\psi_n^{(0)}$:

Source reminder mislabeling a Gaussian-only ground-state shape as the general nth oscillator wavefunction, followed by ladder-operator definitions

That Gaussian-only form is the $n=0$ shape, up to normalization. In general,

$$ \psi_n(x)\propto H_n\!\left(\sqrt{\frac{M\omega}{\hbar}}x\right) e^{-M\omega x^2/(2\hbar)}, $$

so the Hermite polynomial supplies the $n$-dependence and parity. This source-image defect does not affect the ladder-operator derivation that follows.

Ladder-operator actions on number states and x expressed through a plus and a minus

For a refresher, see The Harmonic Oscillator and Ladder Operators. The sketch below shows the original oscillator-potential reminder.

Hand-drawn harmonic-oscillator potential well

Write the bra and ket as number states,

The matrix element of x rewritten as bra m x ket n

and use $x=\sqrt{\hbar/(2M\omega)}(a+a^\dagger)$:

Evaluation of the x matrix element using raising and lowering operators

Second-order sum after substituting the ladder-operator matrix element

The Kronecker deltas leave only $m=n+1$ and $m=n-1$. Evaluating those two terms,

Handwritten two-term calculation yielding minus q squared E squared over 2 M omega squared

gives the $n$-independent shift

$$ E_n^{(2)} =\frac{q^2\mathcal E^2}{2M\omega^2} \left(\frac{n}{1}-\frac{n+1}{1}\right) =-\frac{q^2\mathcal E^2}{2M\omega^2}. $$

(b) Exact solution by shifting the coordinate

Now solve the Schrödinger equation directly:

Schrodinger equation for the harmonic oscillator with the added minus q E x potential

The suggested coordinate shift is

Coordinate substitution x prime equals x minus q E over M omega squared

$$ x'=x-\frac{q\mathcal E}{M\omega^2}, \qquad x=x'+\frac{q\mathcal E}{M\omega^2}. $$

Because the shift is constant, the second derivative is unchanged:

The second derivative with respect to x equals the second derivative with respect to x prime

Substituting the shifted coordinate gives

Expansion of x squared after the coordinate shift

Schrodinger equation after substituting the shifted coordinate

Handwritten completion of the square for the shifted oscillator Hamiltonian

Equivalently, completing the square directly yields

$$ \frac12M\omega^2x^2-q\mathcal E x =\frac12M\omega^2 \left(x-\frac{q\mathcal E}{M\omega^2}\right)^2 -\frac{q^2\mathcal E^2}{2M\omega^2}. $$

The Hamiltonian therefore has the usual oscillator spectrum plus a constant negative shift:

$$ E_n=\left(n+\frac12\right)\hbar\omega -\frac{q^2\mathcal E^2}{2M\omega^2}. $$

The preserved source next writes an intermediate primed-energy relation,

Intermediate source relation between E prime and E for the shifted oscillator

and summarizes it as follows:

Source summary claiming E prime differs from E by a positive q squared E squared term

Those two images use $E$ and $E'$ ambiguously. If $E'=E+q^2\mathcal E^2/(2M\omega^2)$ denotes the eigenvalue on the completed-square oscillator side, then $E'=(n+\tfrac12)\hbar\omega$ and the physical energy is

$$ E=E'-\frac{q^2\mathcal E^2}{2M\omega^2}. $$

So the physical shift is negative, exactly matching the second-order perturbative result. In this case all higher-order corrections vanish because completing the square gives the exact answer. That is the reassuring point of the exercise: when an exact solution is available, it confirms the perturbative calculation—and when it is not, the same method can still provide a controlled approximation.

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