SkarpSkarp

Chapter 10 of 14

Approximation Power Tools: Perturbation Theory and Variational Methods

Most real quantum systems cannot be solved exactly, yet clever approximation schemes open them up. See how small perturbations and smart trial wavefunctions unlock spectra and shifts observed in real atoms and molecules.

15 min readen

Big Picture: Why We Need Approximation Tools

Why Approximations?

Most real quantum systems (atoms in fields, molecules, solids) cannot be solved exactly. The Schrödinger equation becomes too hard once realistic interactions are included.

Two Power Tools

We use two key tools: time-independent perturbation theory (for small changes to a solvable system) and the variational method (to estimate ground-state energies when no exact solution is known).

Unperturbed vs Real System

We split the Hamiltonian into a simple solvable part `H0` and a smaller extra term `H'`, or we treat the full Hamiltonian `H` but guess a good wavefunction to bound the ground-state energy.

What You Will Do

You will learn the first-order perturbation recipe, see how energies and states shift, understand the variational principle, and apply both to simple atoms and molecules.

Step 1: Setting Up Time-Independent Perturbation Theory

Splitting the Hamiltonian

Write `H = H0 + λ H'`, where `H0` is solvable and `H'` is a smaller perturbation. `λ` is a bookkeeping parameter that we set to 1 at the end.

Known Eigenstates of H0

Assume `H0 |n(0)⟩ = E_n(0) |n(0)⟩` and that these levels are non-degenerate. These unperturbed states form a convenient basis.

Series Expansions

We expand the exact energies and states as power series: `En = En(0) + λ E_n(1) + ...`, and `|n⟩ = |n(0)⟩ + λ |n(1)⟩ + ...`.

When It Works

Perturbation theory works when `H'` is small compared with level spacings, levels are non-degenerate, and we only need modest corrections.

Step 2: First-Order Energy Shifts and State Corrections

First-Order Energy Shift

The first-order correction to energy is `E_n(1) = ⟨n(0)| H' |n(0)⟩`, the expectation value of the perturbation in the unperturbed state.

First-Order State Correction

The first-order correction to the state is `|n(1)⟩ = Σ{m ≠ n} |m(0)⟩ ( ⟨m(0)| H' |n(0)⟩ / (En(0) - E_m(0)) )`.

Physical Meaning

The perturbation mixes the original state with others. Mixing is stronger when `⟨m(0)| H' |n(0)⟩` is large and the energy difference `En(0) - Em(0)` is small.

What We Usually Need

Often we only need first-order energy shifts, which are easy to compute. Higher orders matter when symmetry kills lower-order terms.

Example 1: Stark Shift of the Hydrogen Ground State (Selection Rules)

Hydrogen in an Electric Field

Take hydrogen in a weak electric field along `z`. The perturbation is `H' = e E z`, where `z` is the position operator and `E` the field strength.

First-Order Shift Formula

For the ground state `|1s⟩`, the first-order shift is `E_1(1) = ⟨1s| H' |1s⟩ = e E ⟨1s| z |1s⟩`.

Symmetry Argument

`1s` is spherically symmetric with even parity, while `z` is odd. The integral of an odd function over all space is zero, so `⟨1s| z |1s⟩ = 0`.

Result and Lesson

The first-order Stark shift of the hydrogen ground state is zero. Symmetries can kill first-order corrections, making second order the leading effect.

Try It: Perturbing a 1D Infinite Square Well

Consider a particle in a 1D infinite square well of width `L`, with walls at `x = 0` and `x = L`. The unperturbed eigenstates are

n(0)(x) = sqrt(2/L) sin(nπx/L)`, with energies `En(0) = (n² π² ħ²)/(2m L²)`.

Now add a small perturbation: a weak linear potential

`H' = α x`, where `α` is a small constant.

Use first-order perturbation theory to estimate the energy shift of the ground state `n = 1`.

  1. Write the formula for the first-order energy correction `E_1(1)`.
  2. Evaluate the integral symbolically (you can do it on paper or in a CAS):

`E1(1) = ∫₀ᴸ ψ1(0)(x) (α x) ψ_1(0)(x) dx`

  1. Check if the answer is positive or negative. What does that tell you about the average position of the particle in the well?

Hint: you will need `∫₀ᴸ sin²(πx/L) x dx`.

Pause and work this out before checking a solution in a textbook or symbolic tool. Focus on setting up the integral correctly.

Step 3: The Variational Principle (Ground States Only)

Variational Inequality

For any normalized trial state `|ψtrial⟩`, `E[ψtrial] = ⟨ψtrial| H |ψtrial⟩ ≥ E₀`, where `E₀` is the true ground-state energy.

Upper Bound

The variational estimate is always an upper bound. Equality holds only if the trial state is the exact ground state (up to a phase).

Practical Recipe

Choose a family of trial states with parameters, compute the expectation value of `H`, and minimize this energy with respect to those parameters.

Modern Relevance

This principle underlies Hartree–Fock and many quantum chemistry methods still central to electronic structure calculations in 2026.

Example 2: Variational Estimate for the Hydrogen Ground State

Trial 1s-like Wavefunction

Take `ψ_trial(r; α) = (α³/π)^{1/2} e^{-α r}`. It mimics the 1s orbital but with adjustable decay rate `α`.

Hydrogen Hamiltonian

In atomic units, `H = - (1/2) ∇² - 1/r`. We compute `E(α) = ⟨ψtrial| H |ψtrial⟩` using standard integrals.

Energy as Function of α

The result is `E(α) = (α² / 2) - α`. To find the best `α`, we minimize this function with respect to `α`.

Minimization and Result

Setting `dE/dα = α - 1 = 0` gives `α = 1`. Then `E_min = -1/2` Hartree = `-13.6 eV`, the exact hydrogen ground-state energy.

Try It: Variational Estimate for Helium (Effective Nuclear Charge)

Helium has two electrons. The exact solution of the full interacting Hamiltonian is not analytic, so approximation is essential.

A common variational ansatz is to treat each electron as if it sees an effective nuclear charge `Z_eff` (screened by the other electron):

trial(r₁, r₂; Zeff) = (Zeff³/π) e^{-Zeff r₁} * (Zeff³/π) e^{-Zeff r₂}`

(Then antisymmetrize with spin to satisfy the Pauli principle; for the energy expectation, this simple product captures the main radial effect.)

Your task (conceptual, not full integration):

  1. Explain why `Z_eff` should be less than 2.
  2. Predict qualitatively what happens to the variational energy as you increase `Z_eff` from 1 toward 2.
  3. Sketch on paper a rough curve `E(Zeff)` vs `Zeff` showing a minimum.

Hint: Larger `Z_eff` pulls electrons closer (lower potential energy) but increases kinetic energy. The minimum balances these.

This is a simplified picture behind more sophisticated methods used in modern electronic-structure codes.

Optional: Numerically Minimizing a Variational Energy in Python

You can easily explore variational energies numerically. Here is a minimal Python example for the hydrogen-like trial wavefunction from Example 2.

We will:

  • Define `E(α) = α2 / 2 - α` (in atomic units).
  • Scan over a range of `α` values.
  • Find the minimum numerically.

```python

import numpy as np

Define the variational energy function for hydrogen (atomic units)

def E(alpha):

return 0.5 alpha*2 - alpha

Scan a range of alpha values

alphas = np.linspace(0.1, 3.0, 200)

energies = E(alphas)

Find minimum

min_index = np.argmin(energies)

alphabest = alphas[minindex]

Ebest = energies[minindex]

print(f"Best alpha ≈ {alpha_best:.3f}")

print(f"Minimum energy ≈ {E_best:.3f} Hartree")

If you have matplotlib, you can also plot the curve:

try:

import matplotlib.pyplot as plt

plt.plot(alphas, energies)

plt.axvline(alpha_best, color='r', linestyle='--', label='Best alpha')

plt.xlabel('alpha')

plt.ylabel('E(alpha) [Hartree]')

plt.legend()

plt.show()

except ImportError:

print("matplotlib not installed; skipping plot.")

```

Quick Check: Perturbation vs Variational

Test your understanding of when to use each method.

You are studying a molecule whose exact Hamiltonian cannot be solved analytically. You can, however, guess a reasonable functional form for the ground-state wavefunction with a few adjustable parameters. Which method is most appropriate to estimate the ground-state energy?

  1. First-order time-independent perturbation theory around a harmonic oscillator
  2. The variational method using a parameterized trial wavefunction
  3. Time-dependent perturbation theory with a sinusoidal driving field
Show Answer

Answer: B) The variational method using a parameterized trial wavefunction

The variational method is designed exactly for this situation: you do not know the exact solution but can guess a trial ground-state wavefunction with parameters and minimize the expectation value of H. Perturbation theory requires a known solvable H0 and a small extra term.

Key Term Review

Flip through these cards to reinforce the core concepts.

Time-independent non-degenerate perturbation theory
An approximation method where the Hamiltonian is written as H = H0 + H', with H0 solvable and energy levels non-degenerate. Small corrections to energies and eigenstates are computed as power series in the perturbation.
First-order energy correction
For a non-degenerate level n, the first-order shift is E_n(1) = ⟨n(0)| H' |n(0)⟩, the expectation value of the perturbation in the unperturbed eigenstate.
First-order state correction
The correction to |n(0)⟩ is |n(1)⟩ = Σ_{m ≠ n} |m(0)⟩ ⟨m(0)| H' |n(0)⟩ / (E_n(0) - E_m(0)), showing mixing with other unperturbed states.
Variational principle
For any normalized trial state |ψ_trial⟩, the expectation value ⟨ψ_trial| H |ψ_trial⟩ is an upper bound on the true ground-state energy E₀.
Trial wavefunction
A guessed, normalized wavefunction with adjustable parameters used in the variational method to approximate the ground state by minimizing the energy expectation value.
Upper bound
In the variational method, the computed energy is always ≥ E₀. Improving the trial wavefunction (more flexibility) can only lower or keep the same energy.

Key Terms

Hamiltonian
The operator H representing the total energy (kinetic plus potential) of a quantum system; it generates time evolution.
Ground state
The lowest-energy eigenstate of a Hamiltonian, with energy E₀.
Perturbation
A small additional term H' added to a solvable Hamiltonian H0, used to model weak external fields or interactions.
Stark effect
The shifting and splitting of atomic or molecular energy levels due to an external electric field.
Expectation value
The average value of an observable in a given quantum state, computed as ⟨ψ| A |ψ⟩.
Trial wavefunction
A guessed, normalized wavefunction, often with adjustable parameters, used in the variational method to approximate the ground state.
Variational method
An approximation technique that uses trial wavefunctions with parameters to obtain an upper bound on the ground-state energy by minimizing the energy expectation value.
Non-degenerate level
An energy level for which there is only one linearly independent eigenstate with that energy.
Effective nuclear charge
An approximate charge Z_eff felt by an electron in a multi-electron atom, reduced from the full nuclear charge by screening from other electrons.

Finished reading?

Test your understanding with a custom practice exam on this chapter.

Test yourself