MO Energy Levels and the Secular Equation
Two hydrogen atoms drift together and something invisible happens first. Before any nucleus moves, before any bond "forms" in the classical sense, the electron's wavefunction reorganizes itself. It forms two new patterns, one lower in energy than either atom alone and one higher. Where do those two numbers come from? Not from Coulomb's law directly, not from a bond-strength lookup table. Instead, they come from a piece of linear algebra: a determinant set to zero. This article derives that determinant — the secular equation — from the Variational Principle applied to a linear combination of atomic orbitals. It shows exactly how the Coulomb integral , the resonance integral , and the overlap integral conspire to produce the bonding/antibonding energy gap. This matters because the secular equation is molecular orbital theory's computational engine. Every qualitative MO diagram chemists draw is a cartoon of eigenvalues. Those eigenvalues are extracted from exactly this kind of determinant. This includes the splitting of and , the ordering of levels in butadiene. It also includes the near-degenerate frontier orbitals that control a Diels–Alder transition state. Photoelectron spectroscopy measures these energies directly as ionization potentials. UV-Vis spectroscopy measures the gaps between them. Reactivity arguments built on HOMO–LUMO interactions are really statements. They describe which roots of the secular equation lie where. The big picture is a chain of three ideas fitting together. First, the variational principle guarantees something important. Any trial wavefunction built as a linear combination of basis functions has an energy. That energy is stationary — a true extremum. This holds only for specific combinations of coefficients. Those combinations are found by differentiating the energy expression. The result is then set to zero. Second, doing that differentiation for an LCAO trial function produces something specific. It produces a homogeneous linear system in the orbital coefficients. A homogeneous system has a nontrivial solution only when its determinant vanishes. Third, that vanishing-determinant condition — the secular equation — is a polynomial in the energy . Its roots are precisely the allowed MO energies. Its associated null-space vectors are the orbital coefficients. What follows builds this machinery from scratch for the simplest nontrivial case. This is a two-orbital, two-electron diatomic problem. The treatment then generalizes to basis functions. It works through three complete numerical examples. One is a symmetric homonuclear case worked asymmetrically in its parameters. Another is a heteronuclear case with genuinely unequal atomic energies. The third is a three-orbital linear system foreshadowing Hückel theory. It closes with the traps that catch nearly every student. These are the traps encountered first when meeting this determinant.
- The MO trial wavefunction has an energy that is stationary at the true MO energies — this is the variational principle in action.
- Minimizing with respect to each coefficient gives a homogeneous linear system, the secular equations, written compactly as .
- A nontrivial coefficient vector exists only if the secular determinant ; its roots are the allowed orbital energies.
- For two orbitals this determinant is a quadratic in , giving the familiar bonding/antibonding pair split around the average Coulomb energy .
- Overlap pushes the antibonding level up more than it pushes the bonding level down — bonding is always weaker than antibonding is strong, when .
- Unequal atomic energies (heteronuclear bonds) reduce the degree of mixing and polarize the MOs toward the lower-energy atom.
- Key idea: setting the secular determinant to zero converts "find the best LCAO wavefunction" into "solve a polynomial eigenvalue problem," and its roots are the MO energy levels.
Where this lives today
Every quantum chemistry software package — from a teaching-level extended Hückel calculation to a production-grade density functional theory code — ultimately solves a generalized matrix eigenvalue problem of the form , the direct linear-algebra descendant of the secular determinant derived here; the Roothaan–Hall equations of Hartree–Fock theory are exactly this equation dressed up with a self-consistent Fock matrix in place of a fixed Hamiltonian. Photoelectron spectroscopists interpret ionization energies as approximations to the negative of orbital energies (Koopmans' theorem), meaning every peak in a UV photoelectron spectrum of, say, formaldehyde or ethylene is effectively a measured root of some underlying secular equation. Materials scientists building tight-binding models of graphene, carbon nanotubes, and topological insulators use secular determinants of exactly this Hückel-style form, with the famous linear () dispersion of graphene's Dirac cones falling directly out of a secular determinant evaluated at each crystal momentum. Drug designers reasoning about the frontier molecular orbitals (HOMO/LUMO) of a candidate inhibitor — where nucleophilic or electrophilic attack will occur, whether a chromophore will absorb in the visible — are reading off the highest and lowest occupied roots of a secular equation computed (usually) at a semi-empirical or DFT level, but conceptually identical to the two-orbital and three-orbital determinants worked out above. Spectroscopic assignment of vibronic and electronic transitions in conjugated dyes, from indigo to cyanine laser dyes, still begins with a Hückel-style secular treatment of the system to get qualitatively correct orbital orderings before more expensive methods refine the numbers.
Ask the tutor: Can you walk through how the secular determinant changes shape once we build in the zero-overlap approximation used in Hückel theory, and why chemists accept that trade-off?
The physical picture
Picture two atomic orbitals, centered on atom A and centered on atom B, each a perfectly good one-electron wavefunction on its own atom. When the atoms approach, an electron near this diatomic framework should be described by some wavefunction that is not exactly or but has to smoothly interpolate and superpose both. The LCAO Approximation proposes the simplest possible ansatz:
The coefficients and are not known in advance — they are the very things we are solving for. The strategy is to treat them as variational parameters: compute the energy expectation value of as a function of , then find the values of that minimize (or, more precisely, make stationary) that energy. Quantum mechanics guarantees, via the Variational Principle, that any such stationary energy is an upper bound to a true eigenvalue of the Hamiltonian, and that the best two-parameter trial function of this form gives the two energies closest to the true bonding and antibonding orbital energies achievable within this basis. The physical content hiding inside the resulting algebra is this: the atomic orbitals are not orthogonal in general (they overlap in space, quantified by ), and the Hamiltonian couples them through the resonance integral , a negative number for bonding interactions between orbitals of the same phase. The diagonal Hamiltonian element (equal for homonuclear cases) is the Coulomb integral, essentially the energy an electron would have sitting in that atomic orbital in the molecular environment. All three integrals — , , — were characterized on their own terms elsewhere; here they become the raw material fed into a determinant.
Reading the diagram: the two atomic levels, degenerate at energy , are pulled apart into a lower bonding combination and a higher antibonding combination. The magnitude of splitting and its asymmetry — the antibonding level rises more than the bonding level falls — is a direct, unavoidable consequence of nonzero overlap , derived rigorously below. The secular determinant is the formal device that finds exactly these two roots and no others, for any number of basis orbitals, not only two.
This second figure is the actual algebraic pipeline: differentiate the variational energy expression, obtain a pair of linear homogeneous equations in , and recognize that these equations have a nonzero solution only when their coefficient determinant vanishes. That last step is not a physical assumption — it is a theorem of linear algebra, and it is the entire content of "the secular equation."
The core ideas
For a general -orbital LCAO basis , define the Hamiltonian and overlap matrix elements
where: is the resonance integral (or Coulomb integral when ) between basis orbitals ; is their overlap integral, with for normalized orbitals. Both matrices are real and symmetric here because is Hermitian and the basis is chosen real, as is standard for atomic , orbitals in simple MO treatments. The condition that the variationally optimized LCAO coefficients exist and are nontrivial is the secular equation:
where: is the matrix of ; is the overlap matrix; is the unknown MO energy, playing the role of the generalized eigenvalue. This is a polynomial equation of degree in ; it has real roots (counting multiplicity) because and are real symmetric with positive definite — these are exactly the MO energy levels built from this basis. For each root , the coefficient vector solving
where: is the (unnormalized) column of LCAO coefficients for the -th molecular orbital; this equation is solved after is known, one root at a time — gives the shape of that particular molecular orbital once normalized against . Specializing to the two-orbital homonuclear case (, , , ), the determinant reads
where: is the atomic Coulomb integral (energy of an electron confined to one atomic orbital in the molecular field); is the resonance integral coupling the two orbitals; is their mutual overlap; is the sought MO energy. Expanding this determinant and solving the resulting quadratic gives the two roots
where: (using top signs, since conventionally) is the lower, bonding orbital energy ; is the higher, antibonding orbital energy . Reading this equation: because typically and , the denominator on the antibonding root is smaller than on the bonding root, which is precisely why the antibonding level rises further above than the bonding level falls below it — an asymmetry with real consequences for whether a four-electron interaction (both orbitals doubly filled, as in He) is net bonding or antibonding.
Goal. Starting only from the trial wavefunction and the variational principle, derive the secular determinant and its two roots , without assuming the answer in advance.
Step 1 — Write the variational energy functional. The energy expectation value of the normalized-in-form trial function is
Expanding both inner products using linearity and real,
Here , and since the two cross terms combine into ; the same logic gives the overlap denominator with .
Step 2 — Clear the denominator and treat as a function of . Write (using , ) so that
This is an implicit definition of ; the variational principle demands we find the stationary points of this function over .
Step 3 — Differentiate with respect to holding fixed, and set to zero. Differentiating both sides of the Step 2 equation with respect to , using the product rule on the left since itself depends on :
At a stationary point, by definition of "stationary," so this collapses to
Dividing by 2 and rearranging into homogeneous form,
Step 4 — Repeat for . By the identical steps, differentiating with respect to and setting the stationary condition gives the second linear equation:
Together, Steps 3–4 form a homogeneous linear system for — the secular equations.
Step 5 — Demand a nontrivial solution. The trivial solution always satisfies the system but describes no electron anywhere, which is unphysical. A homogeneous linear system has a nonzero solution vector if and only if its coefficient matrix is singular, i.e., its determinant vanishes:
This is the secular determinant, and it is now a direct consequence of the variational stationarity condition, not an extra postulate.
Step 6 — Specialize to the homonuclear case and expand. Set , . Expanding the determinant:
This factors as a difference of squares:
Step 7 — Solve each linear factor for . From the first bracket, . From the second bracket, . Since is negative (a stabilizing resonance integral by convention), the root with in the numerator is the lower energy — the bonding MO — and is the antibonding MO, confirming the result quoted above.
Go deeper · Derivation B · 1 minWhy the antibonding level rises more than the bonding level falls
Goal. Quantify the asymmetry of the splitting directly from , showing algebraically (not just qualitatively) why makes bonding weaker than antibonding is destabilizing — a fact essential for understanding why filling both levels (as in He) gives net repulsion.
Step 1 — Write both energies relative to . Define the shifts (stabilization of bonding MO) and (destabilization of antibonding MO):
Step 2 — Compare the two shifts. Both shifts share the identical numerator ; since , this numerator is positive (as and are both positive contributions when or when is small — in the standard convention is also negative, and the sign bookkeeping is confirmed numerically in the worked examples below). They differ only in denominator: for versus for .
Step 3 — Take the ratio.
For any physically realistic overlap , this ratio is strictly greater than 1, proving algebraically, with no numerical example needed to see the sign of the effect — though the size is worked out below.
Step 4 — Physical reading. Because , a hypothetical molecule with both the bonding and antibonding MOs doubly occupied (four electrons total in this two-orbital space) has a net energy change of
more precisely the total electronic energy relative to two separated atoms shifts by , an energy increase. This is the quantitative root of the textbook statement that He is unbound (or only van-der-Waals bound): filling both and MOs formed from 1s orbitals leaves the system higher in energy than two separate He atoms, purely because of the -driven asymmetry derived here.
Worked examples
Example 1 — Foundational: homonuclear diatomic with explicit, non-round numbers. Take a model diatomic (parameters chosen to be numerically distinct and realistic in magnitude, not tuned to round out prettily) with
Compute the bonding and antibonding energies using . Bonding root:
Antibonding root:
So the bonding MO sits eV below the atomic level, while the antibonding MO sits eV above it. Checking the algebraic prediction from the second derivation, should equal ; numerically , matching (small rounding only). This single calculation demonstrates every qualitative feature of MO splitting: the average of is not (it is pulled slightly, because of the asymmetric denominators, though for small it is close), and the antibonding destabilization visibly exceeds the bonding stabilization. Limiting case check: as , both denominators collapse to 1, giving symmetric about — this is exactly the zero-overlap approximation used in elementary MO cartoons and is recovered correctly from the general formula, confirming internal consistency.
Example 2 — Applied: heteronuclear bond (unequal Coulomb integrals), e.g. an HF-like system. Now the two atomic orbitals are not equivalent: eV (a hydrogen-like 1s), eV (a more electronegative fluorine-like 2p), with resonance integral eV and overlap . The secular determinant is now
Expanding (careful: the two diagonal terms are no longer equal, so no simple difference-of-squares factoring applies):
Expand each piece. First, . Numerically, , and , so this piece is . Second, . Subtracting,
Applying the quadratic formula, . Compute the discriminant: , and , so the discriminant is , whose square root is .
Bonding root: eV. Wait — check ordering: the more negative root is the lower (bonding) energy, so take the branch giving the more negative value. Antibonding root: eV. Re-examine: eV is lower than eV, so in fact eV (bonding, lower) and eV (antibonding, higher). This makes physical sense: since eV is already lower than eV, the bonding MO — built mostly from the lower-energy fluorine-like orbital — sits close to but below , while the antibonding MO sits close to but above . The bonding MO is stabilized by only eV relative to , much less than the homonuclear Example 1's stabilization, because unequal atomic energies reduce mixing efficiency — a general and important trend: the more electronegativity difference between two atoms, the less the bonding MO is stabilized relative to the lower atomic level, even though the bond may still be strong in absolute terms because that level was already low. Limiting case check: if this heteronuclear formula must reduce to the homonuclear result; setting in the quadratic reproduces exactly the Example 1 factoring, confirming the general heteronuclear treatment correctly contains the homonuclear case as a special instance.
Example 3 — Competition level: three-orbital linear chain (a minimal Hückel-style secular determinant). Consider three orbitals in a linear (non-cyclic) chain — a toy allyl-radical-like system — with all Coulomb integrals equal to , nearest-neighbor resonance integral between orbitals 1–2 and 2–3 (but not 1–3, since they are not adjacent), and — to make the example a genuine test of the general determinant rather than the familiar zero-overlap Hückel shortcut — retain a small nearest-neighbor overlap while setting overlap between non-adjacent orbitals 1 and 3 to exactly zero (a reasonable approximation, since they are far apart). The secular determinant is
Let and for brevity. The determinant expands (along the first row) as
This factors immediately into or , i.e. .
Root 1: . This is the nonbonding molecular orbital, exactly at the atomic energy — the middle rung of the allyl-type ladder, independent of both and , a structurally important and testable prediction.
Root 2:
Root 3: Now insert numbers: eV, eV, , so eV and . Root 2 (using in numerator): eV. This is the antibonding MO (highest energy of the three, since it's the least negative). Root 3: eV. This is the bonding MO (most negative, lowest energy). Root 1 remains eV, the nonbonding MO, sitting numerically between the other two (), exactly as the qualitative allyl MO diagram requires: one bonding level below , one nonbonding level at , one antibonding level above . Limiting case check: setting recovers the standard zero-overlap Hückel allyl result directly, since both denominators collapse to 1 — this is precisely the simplification that Hückel theory adopts as a standing approximation, and this worked example shows explicitly what is being neglected when that approximation is made.
Limiting cases, scope & common traps
| Limit / regime | What happens to | Why |
|---|---|---|
| (zero differential overlap) | , symmetric about | Denominators ; this is the Hückel-theory standing approximation |
| (no interaction) | Orbitals don't couple; no splitting at all | |
| , large mismatch | Splitting shrinks; MOs become nearly pure atomic orbitals | Mixing efficiency drops as the energy denominator in perturbative language grows |
| Recovers the symmetric homonuclear formula exactly | Confirms heteronuclear result contains homonuclear as special case | |
| (orbitals nearly identical/coincident) | formally; treatment breaks down | Basis becomes linearly dependent; must reorthogonalize basis first |
| orbitals | Determinant becomes degree- polynomial; up to distinct roots | Same derivation, larger matrix — no new physics, more algebra |
The chemist behind it
The secular determinant as a chemical tool is inseparable from Erich Hückel, who in 1931 applied exactly this variational-plus-determinant machinery to electrons in unsaturated and aromatic hydrocarbons, reducing the electronic structure problem to a small, hand-solvable polynomial equation — a breakthrough precisely because it made quantum mechanical reasoning about aromaticity and reactivity tractable without a computer. Hückel trained originally as a physicist under Peter Debye, working on dipole moments and electrolyte theory (the Debye–Hückel theory of ionic solutions bears his name for entirely separate reasons), before turning his attention in the late 1920s to the puzzle of why benzene's six electrons behave so differently from three isolated double bonds. His molecular orbital treatment, built from a secular determinant with all diagonal Coulomb integrals equal and only nearest-neighbor resonance integrals nonzero, gave the now-iconic result that a closed shell of electrons in a cyclic conjugated system is unusually stable — a rule chemists still apply by name today. The mathematical core of that theory is exactly the vanishing-determinant condition developed in this article, specialized to cyclic and acyclic conjugated systems with the zero-overlap simplification.
Origins · 1 minErich Hückel and how this was discovered
Hückel bridged mathematical physics and organic chemistry at a moment when the two communities rarely spoke the same language. Trained in the Debye school of rigorous statistical and electrostatic theory, he brought a physicist's comfort with matrices, secular equations, and perturbation theory into a discipline still dominated by structural and synthetic reasoning. His 1931 papers on the electronic structure of ethylene, benzene, and related unsaturated systems established that a drastically simplified Hamiltonian — retaining only nearest-neighbor coupling and treating and electrons separately — could reproduce the qualitative energetic ordering of real molecules using nothing more than the determinant machinery every chemistry student now works through by hand.
What is the difference between the secular equation and the secular determinant?
They refer to the same underlying condition viewed two ways. The "secular equations" are the set of homogeneous linear equations obtained from differentiating the variational energy with respect to each LCAO coefficient — one equation per orbital in the basis. The "secular determinant" is the single scalar equation, , that must hold for that homogeneous system to have a nonzero solution. In practice chemists use the two terms almost interchangeably, but strictly the determinant is the condition under which the equations admit a physically meaningful (nonzero) solution.
Why must the trial wavefunction coefficients not both be zero?
If , the trial wavefunction vanishes identically everywhere in space. A wavefunction that is zero everywhere describes no electron and cannot be normalized (its norm is zero, not one), so it has no physical meaning. The entire point of the secular determinant is to find the special energies for which the homogeneous coefficient system permits a genuinely nonzero, normalizable coefficient vector — that is the mathematical signature of an actual allowed molecular orbital.
Does the secular determinant approach work for more than two atomic orbitals?
Yes, and the derivation generalizes directly: for basis orbitals, the variational energy is differentiated with respect to all coefficients, producing homogeneous linear equations, whose coefficient matrix is . Setting that determinant to zero gives a degree- polynomial in with up to real roots — this is exactly the structure used in Hückel theory for benzene (a 6×6 determinant) and in modern computational chemistry, where basis sets often contain hundreds of functions and the determinant is diagonalized numerically rather than expanded symbolically.
Why is the overlap matrix S sometimes just replaced by the identity matrix?
Some simplified treatments (most famously the standard zero-overlap Hückel approximation) assume for and , making the identity matrix. This turns the generalized eigenvalue problem into an ordinary eigenvalue problem , which is algebraically much simpler to solve by hand. It is a genuine approximation — real atomic orbitals on adjacent atoms do overlap — but for qualitative orbital-ordering purposes it captures the correct physics at much lower computational cost, as demonstrated by the limiting case worked through explicitly above.
How does this connect to bond order and bond strength?
Once the secular determinant gives the MO energies and coefficients, the pattern of which MOs are filled with electrons (bonding versus antibonding) determines whether a bond forms and how strong it is — this is the subject explored under Bond Order and Bond Stabilization. Broadly, electrons in bonding MOs (energy below α) stabilize the molecule relative to separated atoms, electrons in antibonding MOs (energy above α) destabilize it, and the net stabilization, weighted appropriately, correlates with measured bond dissociation energies and bond lengths.
What physically is the Coulomb integral α doing in this determinant, separate from resonance β?
The Coulomb integral represents the energy an electron would have if it were confined entirely to atomic orbital within the full molecular Hamiltonian — essentially the atomic orbital energy, perturbed slightly by the presence of the other nucleus. It sets the baseline reference level from which bonding and antibonding orbitals split; , by contrast, is entirely responsible for how much splitting occurs. Without there is no mixing and no chemical bond at all, regardless of what is, which is why (and the overlap that scales its effect) is the true "bonding" integral.
Can the secular determinant give complex or negative-only energy roots?
No — for a real, symmetric Hamiltonian matrix and a real, symmetric, positive-definite overlap matrix (which is always the case for a basis of genuinely linearly independent real atomic orbitals), the generalized eigenvalue problem is guaranteed by linear algebra to produce exactly real roots for an system. Whether those roots are numerically negative or positive depends entirely on the energy convention chosen (e.g., ionization energies are often quoted as positive numbers while orbital energies relative to the vacuum are negative), not on any mathematical restriction of the determinant itself.