SECTION 1
Historical Context & Motivation
The concept of degeneracy — where two or more quantum states share exactly the same energy — first became apparent in the early twentieth century when atomic spectra revealed unexplained fine structure. Classical physics offered no framework for understanding why certain spectral lines would split into multiplets under external fields, but the nascent quantum theory of Bohr and Sommerfeld hinted that hidden symmetries were at work. When experimentalists applied electric and magnetic fields to hydrogen, they observed that single lines fanned out into clusters of closely spaced transitions, a phenomenon that demanded a theoretical mechanism for the lifting of degeneracy. This set the stage for one of quantum mechanics' most powerful approximation methods: perturbation theory.
1896 • Zeeman Effect Discovered
1913 • Bohr Model & Hydrogen Degeneracy
1926 • Schrödinger Equation & Matrix Mechanics
1926–1929 • Rayleigh–Schrödinger Perturbation Theory
1947 • Lamb Shift
The central question driving this lesson is deceptively simple: when a quantum system possesses states that share the same energy, how do we predict which linear combinations nature actually selects once a small perturbation is introduced? Answering this question requires understanding both the group-theoretic origins of degeneracy and the qualitative logic behind perturbation expansions — concepts that underpin everything from crystal-field theory in inorganic chemistry to the band structure of solids.
SECTION 2
Core Principles & Definitions
Before engaging with the mathematics of perturbation theory, it is essential to establish a precise vocabulary. Degeneracy refers to the situation in which a single eigenvalue of a Hamiltonian corresponds to more than one linearly independent eigenstate. The degree of degeneracy (or multiplicity) is the dimension of the eigenspace associated with that eigenvalue. In the hydrogen atom, for example, the energy En = −13.6 eV / n² is n²-fold degenerate when spin is neglected, because states with different ℓ and mℓ values all share the same energy for a given n. This arises from the SO(4) symmetry of the pure Coulomb potential, and it would be broken if the potential deviated from its 1/r form. Understanding why degeneracy exists — always rooted in a symmetry of the Hamiltonian — is the first conceptual pillar.
Degeneracy & Symmetry
Essential vs. Accidental Degeneracy
Perturbation as a Small Disturbance
Correct Zeroth-Order States
Lifting of Degeneracy
KEY TAKEAWAY
SECTION 3
Visual Explanation — Energy Level Splitting
The diagram above captures the central narrative of this lesson. On the left, the unperturbed Hamiltonian H⁰ yields energy levels with well-defined degeneracies indicated by the colored dots on each line. A non-degenerate level such as E₁ merely shifts its energy when the perturbation is introduced — this is the domain of standard (non-degenerate) perturbation theory. In contrast, the three-fold degenerate level E₂ fans out into three distinct levels as the perturbation λH′ breaks the symmetry responsible for the original degeneracy. The pattern of splitting — which levels move up, which move down, and whether any remain degenerate — is governed by the matrix elements of H′ within the degenerate subspace. Predicting this pattern is the central computational task of degenerate perturbation theory, and understanding it qualitatively before performing calculations is the goal of the present discussion.
SECTION 4
Mathematical Framework
The formal starting point is the decomposition of the full Hamiltonian into an exactly solvable piece and a perturbation. The solutions of H⁰ are assumed known, and our task is to determine how these solutions change when H′ is switched on. The analysis proceeds differently depending on whether the eigenvalue of interest is degenerate or not.
PERTURBED HAMILTONIAN
H⁰ = unperturbed (solvable) Hamiltonian; H′ = perturbation operator; λ = dimensionless coupling parameter (0 ≤ λ ≤ 1). At λ = 0 we recover the unperturbed system; at λ = 1 we have the full problem.
UNPERTURBED EIGENVALUE EQUATION
If En(0) has gn linearly independent eigenstates |ψₙ,₁⁽⁰⁾⟩, … , |ψₙ,gₙ⁽⁰⁾⟩, the level is gₙ-fold degenerate.
FIRST-ORDER ENERGY CORRECTION (NON-DEGENERATE)
For a non-degenerate state, the first-order energy shift is simply the expectation value of the perturbation in the unperturbed state. This formula fails when the level is degenerate because any linear combination of degenerate states is equally valid as the zeroth-order state.
DEGENERATE PERTURBATION — SECULAR EQUATION
The gn × gn matrix W is formed from the matrix elements of H′ restricted to the degenerate subspace. Its eigenvalues give the first-order energy corrections E⁽¹⁾, and its eigenvectors give the correct zeroth-order states — the linear combinations that diagonalize the perturbation within the subspace.
The secular equation is the heart of degenerate perturbation theory at first order. Qualitatively, its message is straightforward: among all possible ways to write zeroth-order states, nature picks the linear combinations that diagonalize the perturbation within the degenerate subspace. Once W is diagonal, each diagonal element becomes the first-order energy correction for the corresponding state. If some eigenvalues of W coincide, a residual degeneracy persists, and higher-order perturbation theory or additional perturbations may be needed to resolve it.
Why Non-Degenerate PT Breaks Down
SECTION 5
Types of Degeneracy & Their Physical Origins
Not all degeneracies arise from the same physical mechanism, and recognizing their origin is essential for predicting how perturbations will affect them. We can broadly classify degeneracies into several categories, each connected to a different symmetry property of the Hamiltonian. The table below summarizes the principal types encountered in atomic, molecular, and solid-state quantum mechanics, while the diagram that follows illustrates how each type manifests in the hydrogen atom.
| Type | Physical Origin | Example | Perturbation That Lifts It |
|---|---|---|---|
| Essential (mℓ) | Rotational symmetry: [H, Lz] = 0 makes energy independent of mℓ | 2p states with mℓ = −1, 0, +1 all at same energy | External magnetic field (Zeeman effect) |
| Accidental (ℓ) | Hidden SO(4) symmetry of the 1/r Coulomb potential | 2s and 2p at the same energy in hydrogen | Deviation from pure 1/r potential; screening in multi-electron atoms |
| Spin | Spin-independent Hamiltonian: [H, S²] = [H, Sz] = 0 | Each orbital state is (2s+1)-fold degenerate in ms | Spin-orbit coupling; external magnetic field |
| Exchange / Permutation | Indistinguishability of identical particles | Singlet and triplet states in helium with same spatial wavefunction | Electron-electron repulsion distinguishes spatial symmetry |
| Kramers | Time-reversal symmetry for half-integer spin systems | Every energy level of an odd-electron system is at least 2-fold degenerate | Magnetic field (breaks time-reversal symmetry) |
Classification of quantum degeneracies by their symmetry origins
This cascade of splittings illustrates a general principle: each perturbation removes a specific symmetry from the Hamiltonian, and the degeneracy associated with that symmetry is lifted. The order in which perturbations are applied matters when their relative magnitudes differ, a consideration that becomes important in choosing the appropriate coupling scheme (LS versus jj coupling) for multi-electron atoms.
SECTION 6
Worked Example — 2D Harmonic Oscillator with Anisotropic Perturbation
Consider a two-dimensional isotropic harmonic oscillator with the unperturbed Hamiltonian H⁰ = ½ mω²(x² + y²) + (px² + py²)/(2m). The energy levels are En = (n + 1)ℏω, where n = nx + ny. The first excited level (n = 1) is two-fold degenerate, with states |1,0⟩ and |0,1⟩. Suppose we introduce a perturbation H′ = εmω²xy, which couples the x and y motions. We wish to find the first-order energy corrections and the correct zeroth-order states.
First-Order Degenerate Perturbation Theory for the n = 1 Level
- 1
Step 1 — Identify the Degenerate Subspace
The n = 1 level has energy E₁⁽⁰⁾ = 2ℏω and is spanned by two states: |1,0⟩ (one quantum in x, zero in y) and |0,1⟩ (zero in x, one in y). These two states form the basis for the 2×2 perturbation matrix W. - 2
Step 2 — Compute the W Matrix Elements
We need the four matrix elements Wᵢⱼ = ⟨nₓ, nᵧ| εmω²xy |nₓ′, nᵧ′⟩. Using the raising/lowering operator representation x = √(ℏ/2mω)(ax† + ax) and y = √(ℏ/2mω)(ay† + ay), the product xy connects states differing by ±1 in both nₓ and nᵧ. The diagonal elements W₁₁ = ⟨1,0|H′|1,0⟩ and W₂₂ = ⟨0,1|H′|0,1⟩ both vanish because the operator xy changes both quantum numbers. The off-diagonal elements give W₁₂ = W₂₁ = εℏω/2.W = εℏω/2 ×[[0, 1], [1, 0]] - 3
Step 3 — Solve the Secular Equation
The secular equation det|W − E⁽¹⁾I| = 0 becomes (−E⁽¹⁾)² − (εℏω/2)² = 0, yielding E⁽¹⁾ = ±εℏω/2.E₊ = 2ℏω + εℏω/2; E₋ = 2ℏω − εℏω/2 - 4
Step 4 — Find the Correct Zeroth-Order States
The eigenvectors of W are |+⟩ = (|1,0⟩ + |0,1⟩)/√2 and |−⟩ = (|1,0⟩ − |0,1⟩)/√2. These are the 'correct' zeroth-order states — the linear combinations that diagonalize H′ within the degenerate subspace. Note that |+⟩ is symmetric under exchange of x and y, while |−⟩ is antisymmetric, reflecting the fact that H′ = εmω²xy is symmetric under simultaneous interchange of x and y.|+⟩ = (|1,0⟩ + |0,1⟩)/√2 → E = 2ℏω + εℏω/2; |−⟩ = (|1,0⟩ − |0,1⟩)/√2 → E = 2ℏω − εℏω/2 - 5
Step 5 — Interpret Physically
The perturbation H′ = εmω²xy couples the two degenerate modes. In the |+⟩ state, the particle's probability density is elongated along the line y = x (the perturbation adds energy because both coordinates reinforce). In |−⟩, the density aligns along y = −x (the perturbation subtracts energy). The originally circular symmetry of the isotropic oscillator is broken, and the two states now oscillate along the principal axes of the total potential, rotated 45° from the original x and y axes. The degeneracy is completely lifted at first order.
SECTION 7
Strengths & Limitations of Perturbation Theory
| Aspect | Strength | Limitation |
|---|---|---|
| Applicability | Works whenever H′ is 'small' compared to the level spacing of H⁰; vast majority of real quantum systems can be framed this way | Fails when the perturbation is comparable to or larger than the unperturbed level spacing — the expansion diverges or converges too slowly |
| Physical insight | Provides term-by-term corrections with clear physical meaning: E⁽¹⁾ is the average of the perturbation, E⁽²⁾ captures virtual transitions to other states | Higher-order terms become algebraically complex and can obscure the physics they describe |
| Degeneracy handling | Degenerate perturbation theory correctly identifies the 'right' basis and predicts splitting patterns; symmetry arguments (group theory) further simplify the W matrix | When the perturbation does not fully lift degeneracy at first order, one must go to higher orders or use quasi-degenerate methods, adding considerable complexity |
| Convergence | Low-order corrections (first and second) are often remarkably accurate for atoms and molecules in weak external fields | The perturbation series is typically asymptotic, not convergent — summing too many terms can worsen the result |
| Alternatives | Perturbation theory is analytically tractable; variational methods complement it for ground states | For strong perturbations, variational, numerical diagonalization, or non-perturbative methods (WKB, instantons) may be required |
Assessment of perturbation theory as an approximation tool
KEY TAKEAWAY
SECTION 8
Connection to Advanced Theory
The introductory treatment of degeneracy and perturbation presented here is the entry point to a rich hierarchy of approximation methods. As you progress through physical chemistry and quantum mechanics, you will encounter increasingly sophisticated extensions that handle the complications arising when degeneracy is not fully lifted, when the perturbation is time-dependent, or when the perturbation series itself fails to converge.
| This Lesson Covers | Advanced Extension |
|---|---|
| First-order degenerate perturbation theory (diagonalizing W within a degenerate subspace) | Higher-order degenerate PT: second-order corrections require an 'effective Hamiltonian' approach within the degenerate subspace, coupling to remote levels via Löwdin partitioning |
| Time-independent perturbation of energy levels | Time-dependent perturbation theory (Fermi's golden rule, transition rates, spectroscopy selection rules) |
| Qualitative prediction of splitting patterns | Group-theoretic selection rules: using irreducible representations to block-diagonalize W and predict which matrix elements vanish by symmetry |
| Small perturbations with clear unperturbed reference | Variational perturbation theory, coupled-cluster methods, and many-body perturbation theory (Møller–Plesset) for electron correlation in molecules |
| Exact degeneracy at zeroth order | Near-degeneracy (quasi-degenerate PT): when energy levels are not exactly degenerate but closely spaced, requiring a hybrid approach that treats the near-degenerate set as a subspace |
Roadmap from introductory to advanced perturbation methods
One of the most impactful applications you will see shortly is crystal-field theory, where the perturbation is the electrostatic field of surrounding ligands acting on a transition-metal ion. The free-ion d-orbital degeneracy (five-fold) is partially lifted according to the point-group symmetry of the ligand environment — an octahedral field splits d orbitals into t₂g and eg sets, while a tetrahedral field produces a different splitting pattern. This is degenerate perturbation theory applied to a chemical problem, and the qualitative reasoning you develop here — which symmetries are preserved, which are broken, and how many distinct energy levels result — transfers directly to those applications.
SECTION 9
Practice Problems
Question 1: CONCEPTUAL
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Question 2: BASIC CALCULATION
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Question 3: INTERMEDIATE
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Question 4: APPLIED
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Question 5: CRITICAL THINKING
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SUMMARY
Summary
Summary
Degeneracy occurs whenever a Hamiltonian's symmetry causes multiple linearly independent eigenstates to share the same energy eigenvalue. The degree of degeneracy equals the dimension of the corresponding eigenspace, and it can be traced to specific symmetry operations that commute with the Hamiltonian — rotational invariance produces mℓ degeneracy, the hidden SO(4) symmetry of the Coulomb potential produces the accidental ℓ degeneracy of hydrogen, and spin-independent Hamiltonians produce spin degeneracy. A perturbation H′ that breaks one or more of these symmetries lifts the associated degeneracy, splitting a single energy level into multiple distinct levels whose number and pattern reflect the residual symmetry of H⁰ + H′.
The core mathematical procedure involves constructing the perturbation matrix W from matrix elements of H′ restricted to the degenerate subspace, then solving the secular equation to obtain first-order energy corrections and the correct zeroth-order states. This procedure is necessary because non-degenerate perturbation theory produces divergent denominators when applied to degenerate levels. Qualitatively, the key insight is that degeneracy implies freedom in choosing basis states, and the perturbation selects the physically meaningful combinations — the ones that diagonalize H′ and therefore evolve smoothly as the perturbation is turned on. This framework underpins applications from atomic fine structure and the Zeeman effect to crystal-field theory and band structure in solids.