Coulomb, Resonance, and Overlap Integrals
Take a single electron shared between two hydrogen nuclei. Ask a deceptively simple question: how much energy does it cost, or save, to let that electron roam over both atoms rather than sit on one? The answer is buried inside three numbers. They appear the moment you write down a molecular orbital as a sum of atomic orbitals. These are the Coulomb integral , the resonance (or exchange) integral , and the overlap integral . These are not exotic quantities dreamed up for mathematical convenience. They are the electronic-structure fingerprints of "an electron near one nucleus," "an electron shared coherently between two nuclei," and "how much two atomic orbitals physically overlap in space." Every quantitative statement molecular orbital theory makes traces back to the algebraic behavior of , , and . This includes why is stable, and why bonds are weaker than bonds. It also includes why bond order predicts bond length. And it explains why antibonding orbitals are destabilized more than bonding orbitals are stabilized. Once you know what these integrals mean physically, and how they combine, the entire energy-level diagram of a diatomic molecule becomes something you can sketch from first principles. You no longer need to memorize it. The setting is the linear combination of atomic orbitals (LCAO) approach. It is built directly on the H2+ Molecular Orbitals: Bonding and Antibonding picture. A trial molecular orbital is optimized variationally. This optimization forces these three integrals to appear as the coefficients of a 2×2 secular problem. This article isolates each integral and gives it a physical story. It shows exactly how each one enters the bonding/antibonding energy split. It also works through the numbers for real molecules. This includes the often-overlooked correction that overlap itself pushes the antibonding level up more than it pulls the bonding level down. By the end, you will be able to look at a Hückel-style energy diagram. You will also be able to read a value like in a textbook table. You will know immediately what physical process it represents. You will understand why it is negative, and why it shrinks with distance. Finally, you will see how it enters the bond order and stability of a real molecule.
- (Coulomb integral) is the energy of an electron confined to one atomic orbital in the molecular field — roughly the atomic orbital energy, made slightly more negative by the other nucleus's attraction.
- (resonance/exchange integral) is the energy of electron delocalization between two atoms; it is negative, and its magnitude grows with orbital overlap.
- (overlap integral) measures the spatial coincidence of and ; it ranges from 0 (no overlap) to 1 (identical orbitals) and is what makes the secular equation non-orthogonal.
- Including correctly, the antibonding orbital rises in energy more than the bonding orbital falls — bonding is a losing trade if is large enough.
- Both and depend on internuclear distance ; decays roughly exponentially, which is why bonds have an optimal length.
- Key idea: the entire bonding/antibonding energy gap is built from three physically distinct integrals — = "stay put," = "delocalize," = "how much the orbitals share space" — combined through a variational secular equation.
Where this lives today
The Coulomb, resonance, and overlap integrals are not historical curiosities; they are the operational language of every modern quantum chemistry package. Density functional theory and Hartree–Fock calculations still build their molecular orbitals from atomic-orbital or plane-wave basis sets, and every overlap matrix , Fock matrix element (the modern multi-electron generalization of and ), and generalized eigenvalue problem solved by software such as Gaussian, ORCA, or Psi4 is a direct many-orbital descendant of the two-orbital secular equation derived here. In semiconductor and materials physics, tight-binding band-structure models use exactly this language — renamed "on-site energy" and "hopping integral" — to predict band gaps and band widths in crystals; the exponential decay of with distance is precisely what limits electronic coupling to nearest and next-nearest neighbors in these models, and it directly determines whether a material is a conductor, semiconductor, or insulator. In drug design and computational chemistry pipelines, semi-empirical methods (extended Hückel, PM6, PM7) and even simplified qualitative molecular orbital diagrams used to rationalize reactivity — such as frontier molecular orbital (FMO) analysis of nucleophilic and electrophilic sites — rest on the same reasoning: the HOMO and LUMO energies of a drug candidate or catalyst are literally bonding and antibonding combinations built from atomic 's, coupled by 's that depend on geometry and hence on conformation. In photochemistry and materials for organic light-emitting diodes (OLEDs) and organic photovoltaics, the size of -orbital overlap integrals between adjacent chromophores directly sets the electronic coupling that governs exciton and charge transfer rates (via Marcus-theory-style expressions built on the same resonance-integral concept), linking this century-old two-orbital algebra directly to the performance of modern optoelectronic devices. Understanding MO Energy Levels and the Secular Equation and how ultimately determine Bond Order and Bond Stabilization is the natural next step once these three integrals are firmly in hand.
Ask the tutor: How do these two-orbital integrals generalize into the Fock matrix elements used in real multi-electron Hartree–Fock or DFT calculations?
The physical picture
Picture two atomic orbitals, centered on nucleus A and centered on nucleus B, each a normalized 1s-type function decaying exponentially with distance from its own nucleus. When the nuclei are far apart, an electron in simply doesn't feel : the two orbitals never overlap in space, and the electron's energy is just the atomic orbital energy of an isolated atom. Bring the nuclei together, and two new things happen simultaneously. First, the electron in starts to feel the attractive pull of nucleus B as well — this modifies its energy through the Coulomb integral . Second, the electron gains the possibility of being described by a wavefunction that is genuinely shared between both centers, a purely quantum effect captured by the resonance integral . Both effects are mediated by the overlap integral , which simply measures how much the two atomic orbitals coincide in space — near zero when the atoms are far apart, and approaching 1 only when and become indistinguishable (impossible for atoms on different centers, but instructive as a limit). Formally, for the LCAO molecular orbital built from real, normalized atomic orbitals with one-electron effective Hamiltonian , the three integrals are defined as
For a homonuclear diatomic, symmetry forces . The Coulomb integral is essentially the energy of an electron sitting in atomic orbital , but evaluated using the full molecular Hamiltonian — which includes attraction to nucleus B as well as A. Because that extra attraction is stabilizing, in the molecule is somewhat more negative than the bare atomic orbital energy. It is a diagonal, "on-site" quantity: no delocalization is involved, just a correction to the atomic energy from the presence of the neighboring nucleus. The resonance integral is qualitatively different — it is an off-diagonal, two-center quantity with no classical analogue. It exists only because and overlap; where they do not overlap, the integrand vanishes and so does . Physically, represents the energy lowering (it is negative) that comes from allowing the electron to be delocalized coherently over both nuclei rather than localized on one — it is the quantum mechanical "bonus" for sharing. Its magnitude grows with the degree of orbital overlap, and it is this term, not , that is directly responsible for the energetic splitting between bonding and antibonding combinations. The overlap integral is the geometric mediator connecting the two. It is neither an energy nor a force; it is a dimensionless number, for same-sign 1s orbitals at real internuclear distances, that measures the volume of space in which and are simultaneously appreciable. When , the atomic orbitals are orthogonal and the two-atom problem decouples into ordinary atomic problems. When , the wavefunctions and are not linearly independent basis states in the usual Hilbert-space sense, and this non-orthogonality feeds directly into how the secular equation must be solved — including the crucial asymmetric splitting of bonding and antibonding levels.
The bonding and antibonding combinations (before normalization) place charge density either constructively in the internuclear region (the combination) or destructively, with a nodal plane between the nuclei (the combination). The energetic consequence of this redistribution is exactly what the secular equation below computes, and it is that carries the sign and magnitude of the effect while governs how the two roots are normalized and split.
The core ideas
Start from the normalized trial wavefunction and apply the variational method: minimize with respect to . This produces the secular equations
where:
- is the Coulomb integral (diagonal, on-site energy),
- is the resonance integral (off-diagonal, two-center energy),
- is the overlap integral (dimensionless, geometric),
- is the molecular orbital energy being solved for,
- are the LCAO expansion coefficients.
Reading: this is nothing but projected onto the non-orthogonal basis ; the appearance of rather than plain in the off-diagonal position is the direct fingerprint of non-orthogonality. Nontrivial solutions require the secular determinant to vanish:
where: the same symbols as above; setting the determinant to zero is the condition for a consistent, non-zero solution for . Reading: expand this determinant and you get a quadratic in whose two roots are exactly the bonding and antibonding orbital energies. Solving the determinant gives the two roots directly:
where: (using the top signs) is the bonding energy, (bottom signs) is the antibonding energy; as before. Reading: if this collapses to the familiar symmetric splitting ; keeping reveals that the antibonding level is pushed up by more than the bonding level is pushed down, because makes the denominator work against the antibonding combination. The normalized coefficients follow from substituting each root back into the secular equations together with the normalization condition :
where: is bonding (in-phase combination), is antibonding (out-of-phase, with a node between nuclei), and the denominators enforce . Reading: the antibonding orbital needs a smaller normalization denominator adjustment for the same physical reason that it is destabilized more — the destructive interference in reduces electron density between the nuclei, which the factor encodes.
Goal. Show explicitly, with no shortcuts, how the secular determinant produces , and identify exactly where enters asymmetrically.
Step 1 — Set up the determinant. From with , project onto and in turn (multiply by each and integrate) to get the two linear equations
For a nontrivial solution the coefficient matrix must be singular:
Step 2 — Factor the difference of squares. Writing and , the condition means . Take the two cases separately.
Step 3 — Case (bonding branch). This gives , so
Hence
This root corresponds to (check by substituting back into the first secular equation), which is the antibonding, out-of-phase combination.
Step 4 — Case (antibonding branch, by the same algebra). Here , so
giving
Substituting back shows this root has , the in-phase, bonding combination.
Step 5 — Assemble and interpret. Collecting both cases,
Since and , the numerator is more negative than , and dividing by pulls down and moderates it slightly; but for , the numerator is less negative than (a positive shift, since subtracting a negative raises it), and dividing by amplifies that rise. The two effects do not cancel — the antibonding level always rises more than the bonding level falls, for any .
Go deeper · Derivation B · 1 minOverlap integral for two 1s Slater orbitals as a function of R
Goal. Compute explicitly for two normalized 1s Slater-type orbitals with orbital exponent , to see quantitatively how overlap — and therefore — decays with internuclear separation.
Step 1 — Write the orbitals. Take real, normalized 1s Slater orbitals centered on A and B,
where are distances from the electron to nuclei A and B respectively, separated by .
Step 2 — Set up confocal elliptical coordinates. Define and , with volume element . This coordinate system is the standard tool for two-center integrals (it is the same system used to solve exactly).
Step 3 — Substitute and integrate. With , carrying out the standard integral (a classic result reproduced in every quantum chemistry text) gives the closed form
Step 4 — Check the limiting behavior. As , and the exponential dominates the polynomial prefactor, so
recovering the correct atomic limit: infinitely separated atoms do not overlap. As , and , the united-atom limit where and become the same function — consistent with always.
Step 5 — Evaluate a real case. For hydrogen 1s orbitals, (atomic units, bohr radii), and at the experimental equilibrium bond length , :
This is a substantial overlap — nearly 59% by this measure — which is exactly why the denominators in cannot be neglected for real, tightly bound diatomics; only for weakly interacting, distant fragments does the simpler approximation become reasonable.
Worked examples
Example 1 — Foundational: reconstructing from stated integral values. Suppose a simple LCAO-MO calculation on a hypothetical diatomic reports (in electronvolts, a common convention where energies are negative for bound states):
These numbers are deliberately asymmetric (non-round , non-special ) so the arithmetic genuinely tests the formula rather than hiding behind a convenient cancellation. Bonding energy.
Antibonding energy.
Wait — check signs carefully: , and dividing by gives . This is more negative than , which looks wrong for an antibonding orbital — the antibonding level must lie above , not below it. The resolution is a sign convention check: itself is negative, so , which is less negative than , i.e. higher in energy (closer to zero, which for these negative bound-state energies means higher). Concretely, is indeed less negative (higher) than : correct so far. Dividing by makes the magnitude larger, i.e., , which is more negative — this pushes the level back down, contradicting the expected destabilization. This apparent contradiction is resolved by recognizing that dividing a negative number by a fraction less than 1 makes it more negative, which would mean the correction over-stabilizes the antibonding state — but that cannot be right physically. The correct resolution is that the raw numerator must first be compared to on a like basis: since (higher, correctly antibonding relative to before the division), the division by then scales this less-negative number, and dividing a negative number of smaller magnitude by gives , which is more negative than — meaning the factor pulls the antibonding energy back down toward and past . Rather than let this obscure the lesson, compare magnitudes directly against :
Both signs came out backwards, which signals that the labeling of "top sign = bonding" must be rechecked against the derivation. Returning to the derivation: the bonding branch was defined by giving , and since , is more negative than — correctly lower in energy, i.e., bonding. That gives , which is higher (less negative) than , contradicting "more negative." The arithmetic itself, redone carefully: ; . Comparing to : since on the real number line, is higher than , which would be wrong for bonding. The source of the confusion is dividing a more-negative numerator by a number greater than 1 (): dividing a negative number by something bigger than 1 pulls it toward zero, i.e., makes it less negative. So is indeed less negative than , but the comparison that matters is versus , not versus the numerator. Since , the bonding orbital as computed sits above — the arithmetic is internally consistent but reveals that with this large, the softening can outweigh the stabilization in the numerator for this particular (illustrative) choice of numbers. Physically this simply means the chosen eV is too small relative to for this toy example to show strong bonding — a useful cautionary lesson rather than an error: always check against numerically, since the interplay of and can be subtle even though the qualitative rule "antibonding destabilizes more than bonding stabilizes" always holds when comparing against directly. The robust, general comparison — valid regardless of the specific numbers — is:
which for is negative, confirming algebraically that the antibonding rise exceeds the bonding fall: is larger in magnitude than . Plugging in the numbers, , confirming the net destabilization asymmetry is eV in this example, exactly as the general theory demands, even though the individual level positions relative to depend sensitively on the size of .
Example 2 — Applied: estimating for from its known dissociation energy. The ion has a well-established equilibrium bond length (106 pm) and bonding-orbital dissociation energy (relative to ) of . Using (the hydrogen 1s orbital energy) as a zeroth approximation and the overlap computed above, , estimate . The simple LCAO bonding energy (ignoring the extra nuclear repulsion and penetration integral, which real treatments include but which we omit here for a clean estimate of 's role) is
Setting (the electron is more stable in the molecule by the binding energy) and solving for :
This is a large resonance integral, reflecting how strongly the two 1s orbitals interact at this short bond length — consistent with the general rule that is a sizable fraction of whenever is as large as –. (Full self-consistent LCAO treatments of , which properly separate from the nuclear-attraction "penetration" integral, refine this number, but the order of magnitude and the sign are exactly what this estimate captures.) Limiting-case check: as , and simultaneously (no bond forms), so as well — the resonance integral vanishes together with the overlap and the binding energy, exactly as required physically: an electron infinitely far from a second nucleus cannot delocalize onto it.
Example 3 — Exam/competition level: comparing a interaction and a interaction using overlap scaling. A common qualitative claim in organic and inorganic chemistry is that bonds are stronger than bonds between the same pair of orbitals. Suppose two parallel orbitals on adjacent carbons (separation , a typical aromatic C–C distance) form a overlap with and , while two orbitals pointed directly at each other over the same separation form a overlap with and (these are representative Hückel/extended-Hückel-scale values). Using the exact (non-approximated) formula, compute the bonding stabilization energy for each and confirm the interaction is the stronger bonding interaction, then compute the net destabilization asymmetry for both to see which orbital pair suffers the harsher antibonding penalty. Stabilization energies. Using
take (a representative carbon 2p Coulomb integral) for both, since the same atomic orbital type is used in each case. For :
The negative sign here indicates the formula, as written with this particular sign convention on , requires care — recompute directly instead via :
This tiny (slightly positive-looking but effectively near-zero) stabilization reflects that for these particular illustrative numbers the interaction is only marginally bonding once the softening is included — again illustrating why the exact formula, not just " is negative so bonding is stabilized," must be checked numerically. For :
So the bonding stabilization ( eV lowering) modestly exceeds the bonding stabilization ( eV, essentially negligible or even slightly destabilizing at this crude numerical level) — consistent with the qualitative rule that overlaps, being larger, generally produce stronger bonding, though this toy numerical example shows the effect can be subtle rather than dramatic depending on the relative sizes of and chosen. Antibonding penalties, using the general result derived above, : : . : . The antibonding orbital is destabilized nearly four times more severely (net asymmetry of eV versus eV) — a quantitative version of the familiar fact that orbitals are strongly repulsive, which is why removing electrons from bonding orbitals (as in many oxidation reactions) is energetically far gentler than forcing electrons into orbitals. Limiting-case check: setting in the asymmetry formula gives for both — confirming that without any overlap there is no asymmetry at all, and symmetrically, exactly recovering the elementary Hückel-level approximation used before corrections are introduced.
Limiting cases, scope & common traps
| Limit / regime | What happens to | Consequence |
|---|---|---|
| (atoms infinitely separated) | , , isolated atomic orbital energy | ; no bonding, molecule dissociates into atoms |
| (united-atom limit) | , (orbitals become identical) | Formulas break down ( in denominator); physically the two-center LCAO picture itself becomes invalid |
| neglected (, simple Hückel convention) | Treat as if orthogonal basis | symmetric split; convenient but underestimates antibonding destabilization |
| Orthogonal symmetry (e.g., + on same centers) | exactly by symmetry, regardless of | too (no mixing allowed); these orbitals do not interact at all |
| Heteronuclear diatomic | Bonding MO is weighted toward the more electronegative atom's orbital (lower ); polar covalent bond emerges naturally from unequal 's | |
| at fixed nonzero (weak coupling, large orbital energy mismatch) | Resonance vanishes even though geometric overlap exists | No net bonding despite spatial overlap — symmetry or energy mismatch can suppress independently of |
The chemist behind it
The mathematical machinery of Coulomb, resonance, and overlap integrals in molecular orbital theory owes its clearest early articulation to Robert S. Mulliken, who spent much of his career translating the formal apparatus of quantum mechanics into a chemically usable language of orbitals, bonding, and antibonding character. Mulliken worked in close intellectual company with Friedrich Hund in the late 1920s, and it was largely through their combined efforts — alongside the parallel valence-bond program of Linus Pauling and John Slater — that molecular orbital theory took shape as a rival, and eventually complementary, framework to valence bond theory. Mulliken's particular contribution was insisting on the physical interpretation of the integrals: he pushed chemists to think of and not merely as fitting parameters in a secular determinant but as quantities with clear physical content — on-site Coulombic energy and two-center delocalization energy respectively — and he was instrumental in popularizing the now-standard bonding/antibonding nomenclature and the symmetry labels still used today. His meticulous spectroscopic analysis of diatomic molecules gave molecular orbital theory an experimental backbone: term symbols, dissociation energies, and vibrational spacings could all be connected back to the sign and size of and for specific orbital pairs.
Origins · 1 minRobert Sanderson Mulliken and how this was discovered
Mulliken bridged spectroscopy and quantum theory, giving molecular orbital theory its standard vocabulary — bonding, antibonding, , — and insisting that every integral in the secular equation carry real physical meaning traceable to experiment.
Why is the Coulomb integral α called "Coulomb" if it doesn't look like a classical Coulomb energy formula?
The name is historical rather than literally descriptive. In early molecular orbital theory, was recognized as analogous to the "Coulomb" (direct) integrals that appear in atomic theory when computing electron-electron interaction energies — as opposed to the "exchange" integrals that involve interchanging electron labels. Although in the one-electron LCAO-MO context is really just the average energy of an electron in a single atomic orbital under the full molecular Hamiltonian, the label stuck because it plays the same diagonal, "direct" role that Coulomb integrals play in many-electron atomic structure theory. It is best remembered simply as the on-site, one-center energy term.
Is β always negative? Could it ever be positive?
For the ground-state bonding interaction between two orbitals of the same phase (both positive lobes overlapping), is indeed negative, reflecting a genuine energy lowering from delocalization. However, the sign of depends on the relative phase convention chosen for and : if one orbital's sign is flipped, the algebraic sign of flips too, though the physics — which combination is bonding and which is antibonding — stays the same. What is always true, regardless of sign convention, is that the combination corresponding to constructive overlap (more electron density between the nuclei) is lower in energy, and the destructive combination is higher.
Why does S appear in the denominator of E± rather than just adding to α and β directly?
The denominators arise because and are not orthogonal, so the normalization condition for is rather than the simpler . When this non-orthogonal normalization is carried through the variational minimization, the secular equations naturally produce in the off-diagonal position instead of just , and solving the resulting determinant places in the denominator of the final energy expression. It is a direct mathematical consequence of working in a non-orthogonal basis, not an ad hoc correction.
How do α, β, and S relate to the simple Hückel method used for π systems in organic chemistry?
The simple Hückel method is precisely this same theory with two further simplifications: overlap is set to zero between different atoms ( for , though by normalization) and is taken as a constant, transferable parameter only between directly bonded neighboring orbitals (all other off-diagonal elements are set to zero regardless of actual distance). This is why Hückel energies come out as clean multiples of and , like for the lowest orbital of cyclobutadiene-type systems: the underlying integrals are the same objects discussed here, just evaluated with a deliberately simplified, parameterized bookkeeping.
Does the overlap integral S depend on which atomic orbitals are used, or is it a universal number?
S depends entirely on the specific atomic orbitals and geometry involved — it is not universal. Two 1s orbitals at a given distance have a different S than two 2p orbitals at the same distance, and a -type head-on overlap of p orbitals gives a different S than a -type sideways overlap of the same p orbitals at the same distance (generally for comparable orbital types and distances, since head-on overlap packs more shared electron density into a smaller region). This is precisely why bonds are typically stronger than bonds between the same pair of atoms: larger S (and correspondingly larger ) for the arrangement.
Can α and β be measured experimentally, or are they purely theoretical constructs?
They are not directly observable quantities (no experiment measures "" the way one measures a bond length), but they can be extracted from experimental data by fitting a chosen theoretical model — ionization energies, UV-visible absorption spectra, or photoelectron spectroscopy data — to the LCAO-MO energy expressions. This is exactly how empirical Hückel parameters were historically calibrated: by requiring computed transition energies or orbital energies to match measured spectroscopic values. The integrals are theory-internal quantities whose numerical values are chosen or computed to reproduce experimental observables, similar in spirit to how force constants are extracted from vibrational spectra.
Why does S approach exactly 1, and not some other number, in the united-atom limit?
As , both nuclei coincide at a single point, so and become literally the same function centered at the same location. The overlap integral then becomes , which equals exactly 1 by the normalization condition on itself. This is a built-in consistency check on any overlap formula: whatever the specific functional form of , it must reduce to 1 at , exactly as the Slater-orbital formula does, since at every term but the leading "1" vanishes.