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 α\alpha, the resonance (or exchange) integral β\beta, and the overlap integral SS. 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 α\alpha, β\beta, and SS. This includes why H2+\mathrm{H_2^+} is stable, and why π\pi bonds are weaker than σ\sigma 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 ψ=cAϕA+cBϕB\psi = c_A\phi_A + c_B\phi_B 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 β=−75 kJ/mol\beta = -75\ \text{kJ/mol} 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.

Key takeaways
  • α\alpha (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.
  • β\beta (resonance/exchange integral) is the energy of electron delocalization between two atoms; it is negative, and its magnitude grows with orbital overlap.
  • SS (overlap integral) measures the spatial coincidence of ϕA\phi_A and ϕB\phi_B; it ranges from 0 (no overlap) to 1 (identical orbitals) and is what makes the secular equation non-orthogonal.
  • Including SS correctly, the antibonding orbital rises in energy more than the bonding orbital falls — bonding is a losing trade if SS is large enough.
  • Both α\alpha and β\beta depend on internuclear distance RR; β\beta 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 — α\alpha = "stay put," β\beta = "delocalize," SS = "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 SμνS_{\mu\nu}, Fock matrix element FμνF_{\mu\nu} (the modern multi-electron generalization of α\alpha and β\beta), and generalized eigenvalue problem FC=SCεFC = SC\varepsilon 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 α,β,S\alpha,\beta,S language — renamed "on-site energy" and "hopping integral" — to predict band gaps and band widths in crystals; the exponential decay of β\beta 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 α\alpha's, coupled by β\beta'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 π\pi-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 α,β,S\alpha,\beta,S 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, ϕA\phi_A centered on nucleus A and ϕB\phi_B 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 ϕA\phi_A simply doesn't feel ϕB\phi_B: 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 ϕA\phi_A starts to feel the attractive pull of nucleus B as well — this modifies its energy through the Coulomb integral α\alpha. 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 β\beta. Both effects are mediated by the overlap integral SS, 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 ϕA\phi_A and ϕB\phi_B become indistinguishable (impossible for atoms on different centers, but instructive as a limit). Formally, for the LCAO molecular orbital ψ=cAϕA+cBϕB\psi = c_A\phi_A + c_B\phi_B built from real, normalized atomic orbitals with one-electron effective Hamiltonian H^\hat H, the three integrals are defined as

αA=∫ϕAH^ϕA dτ,αB=∫ϕBH^ϕB dτ,β=∫ϕAH^ϕB dτ,S=∫ϕAϕB dτ.\alpha_A = \int \phi_A \hat H \phi_A\, d\tau, \qquad \alpha_B = \int \phi_B \hat H \phi_B\, d\tau, \qquad \beta = \int \phi_A \hat H \phi_B\, d\tau, \qquad S = \int \phi_A \phi_B\, d\tau.

For a homonuclear diatomic, symmetry forces αA=αB≡α\alpha_A = \alpha_B \equiv \alpha. The Coulomb integral α\alpha is essentially the energy of an electron sitting in atomic orbital ϕA\phi_A, but evaluated using the full molecular Hamiltonian — which includes attraction to nucleus B as well as A. Because that extra attraction is stabilizing, α\alpha 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 β\beta is qualitatively different — it is an off-diagonal, two-center quantity with no classical analogue. It exists only because ϕA\phi_A and ϕB\phi_B overlap; where they do not overlap, the integrand ϕAH^ϕB\phi_A\hat H\phi_B vanishes and so does β\beta. Physically, β\beta 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 α\alpha, that is directly responsible for the energetic splitting between bonding and antibonding combinations. The overlap integral SS is the geometric mediator connecting the two. It is neither an energy nor a force; it is a dimensionless number, 0≤S≤10 \le S \le 1 for same-sign 1s orbitals at real internuclear distances, that measures the volume of space in which ϕA\phi_A and ϕB\phi_B are simultaneously appreciable. When S=0S=0, the atomic orbitals are orthogonal and the two-atom problem decouples into ordinary atomic problems. When S≠0S \ne 0, the wavefunctions ϕA\phi_A and ϕB\phi_B 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.

Figure
Two 1s orbitals separated by distance R: the shaded lens is the overlap region contributing to S
φ_A (1s on A) φ_B (1s on B) R (internuclear distance) S ∝ overlap lens region Large R → S ≈ 0 (atomic limit); small R → S → 1 (united-atom limit)

The bonding and antibonding combinations ψ±=ϕA±ϕB\psi_\pm = \phi_A \pm \phi_B (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 β\beta that carries the sign and magnitude of the effect while SS governs how the two roots are normalized and split.

Figure
Energy-level splitting from α, β, S for a homonuclear diatomic
α (atom A, isolated) α (atom B, isolated) E₋ = (α+β)/(1+S) bonding E₊ = (α−β)/(1−S) antibonding stabilization < destabilization when S>0 MO diagram: two AOs at α combine via β, S into split bonding/antibonding pair

The core ideas

Start from the normalized trial wavefunction ψ=cAϕA+cBϕB\psi = c_A\phi_A + c_B\phi_B and apply the variational method: minimize E[ψ]=⟨ψ∣H^∣ψ⟩/⟨ψ∣ψ⟩E[\psi] = \langle\psi|\hat H|\psi\rangle / \langle\psi|\psi\rangle with respect to cA,cBc_A, c_B. This produces the secular equations

cA(α−E)+cB(β−ES)=0,cA(β−ES)+cB(α−E)=0.c_A(\alpha - E) + c_B(\beta - ES) = 0, \qquad c_A(\beta - ES) + c_B(\alpha - E) = 0.

where:

  • α\alpha is the Coulomb integral (diagonal, on-site energy),
  • β\beta is the resonance integral (off-diagonal, two-center energy),
  • SS is the overlap integral (dimensionless, geometric),
  • EE is the molecular orbital energy being solved for,
  • cA,cBc_A, c_B are the LCAO expansion coefficients.

Reading: this is nothing but H^ψ=Eψ\hat H\psi = E\psi projected onto the non-orthogonal basis {ϕA,ϕB}\{\phi_A,\phi_B\}; the appearance of ESES rather than plain EE in the off-diagonal position is the direct fingerprint of non-orthogonality. Nontrivial solutions require the secular determinant to vanish:

∣α−Eβ−ESβ−ESα−E∣=0.\begin{vmatrix} \alpha - E & \beta - ES \\ \beta - ES & \alpha - E \end{vmatrix} = 0.

where: the same symbols as above; setting the determinant to zero is the condition for a consistent, non-zero solution for (cA,cB)(c_A,c_B). Reading: expand this 2×22\times2 determinant and you get a quadratic in EE whose two roots are exactly the bonding and antibonding orbital energies. Solving the determinant gives the two roots directly:

E±=α±β1±S.E_\pm = \frac{\alpha \pm \beta}{1 \pm S}.

where: E−E_- (using the top signs) is the bonding energy, E+E_+ (bottom signs) is the antibonding energy; α,β,S\alpha,\beta,S as before. Reading: if S=0S=0 this collapses to the familiar symmetric splitting E±=α±βE_\pm = \alpha \pm \beta; keeping S≠0S\ne0 reveals that the antibonding level is pushed up by more than the bonding level is pushed down, because 1−S<1<1+S1-S < 1 < 1+S 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 cA2+cB2+2cAcBS=1c_A^2 + c_B^2 + 2c_Ac_BS = 1:

ψ−=ϕA+ϕB2(1+S),ψ+=ϕA−ϕB2(1−S).\psi_- = \frac{\phi_A + \phi_B}{\sqrt{2(1+S)}}, \qquad \psi_+ = \frac{\phi_A - \phi_B}{\sqrt{2(1-S)}}.

where: ψ−\psi_- is bonding (in-phase combination), ψ+\psi_+ is antibonding (out-of-phase, with a node between nuclei), and the denominators enforce ∫ψ2dτ=1\int \psi^2 d\tau = 1. Reading: the antibonding orbital needs a smaller normalization denominator adjustment for the same physical reason that it is destabilized more — the destructive interference in ψ+\psi_+ reduces electron density between the nuclei, which the (1−S)(1-S) factor encodes.

Derivation ADeriving E± from the secular determinant

Goal. Show explicitly, with no shortcuts, how the secular determinant produces E±=(α±β)/(1±S)E_\pm = (\alpha \pm \beta)/(1 \pm S), and identify exactly where SS enters asymmetrically.

Step 1 — Set up the determinant. From H^ψ=Eψ\hat H \psi = E\psi with ψ=cAϕA+cBϕB\psi = c_A\phi_A + c_B\phi_B, project onto ϕA\phi_A and ϕB\phi_B in turn (multiply by each and integrate) to get the two linear equations

cA(α−E)+cB(β−ES)=0,c_A(\alpha - E) + c_B(\beta - ES) = 0,
cA(β−ES)+cB(α−E)=0.c_A(\beta - ES) + c_B(\alpha - E) = 0.

For a nontrivial solution the coefficient matrix must be singular:

(α−E)2−(β−ES)2=0.(\alpha-E)^2 - (\beta - ES)^2 = 0.

Step 2 — Factor the difference of squares. Writing X=α−EX = \alpha - E and Y=β−ESY = \beta - ES, the condition X2=Y2X^2 = Y^2 means X=±YX = \pm Y. Take the two cases separately.

Step 3 — Case X=YX = Y (bonding branch). This gives α−E=β−ES\alpha - E = \beta - ES, so

α−β=E−ES=E(1−S).\alpha - \beta = E - ES = E(1-S).

Hence

E=α−β1−S.E = \frac{\alpha - \beta}{1 - S}.

This root corresponds to cA=−cBc_A = -c_B (check by substituting back into the first secular equation), which is the antibonding, out-of-phase combination.

Step 4 — Case X=−YX = -Y (antibonding branch, by the same algebra). Here α−E=−(β−ES)=−β+ES\alpha - E = -(\beta - ES) = -\beta + ES, so

α+β=E+ES=E(1+S),\alpha + \beta = E + ES = E(1+S),

giving

E=α+β1+S.E = \frac{\alpha + \beta}{1 + S}.

Substituting back shows this root has cA=cBc_A = c_B, the in-phase, bonding combination.

Step 5 — Assemble and interpret. Collecting both cases,

E−=α+β1+S(bonding),E+=α−β1−S(antibonding).E_- = \frac{\alpha+\beta}{1+S} \quad(\text{bonding}), \qquad E_+ = \frac{\alpha-\beta}{1-S} \quad(\text{antibonding}).

Since β<0\beta < 0 and 0<S<10 < S < 1, the numerator α+β\alpha+\beta is more negative than α\alpha, and dividing by 1+S>11+S>1 pulls E−E_- down and moderates it slightly; but for E+E_+, the numerator α−β\alpha - \beta is less negative than α\alpha (a positive shift, since subtracting a negative β\beta raises it), and dividing by 1−S<11-S<1 amplifies that rise. The two effects do not cancel — the antibonding level always rises more than the bonding level falls, for any S>0S>0. ■\blacksquare

Go deeper · Derivation B · 1 minOverlap integral for two 1s Slater orbitals as a function of R
Derivation BOverlap integral for two 1s Slater orbitals as a function of R

Goal. Compute S(R)S(R) explicitly for two normalized 1s Slater-type orbitals with orbital exponent ζ\zeta, to see quantitatively how overlap — and therefore β\beta — decays with internuclear separation.

Step 1 — Write the orbitals. Take real, normalized 1s Slater orbitals centered on A and B,

ϕA=(ζ3π)1/2e−ζrA,ϕB=(ζ3π)1/2e−ζrB,\phi_A = \left(\frac{\zeta^3}{\pi}\right)^{1/2} e^{-\zeta r_A}, \qquad \phi_B = \left(\frac{\zeta^3}{\pi}\right)^{1/2} e^{-\zeta r_B},

where rA,rBr_A, r_B are distances from the electron to nuclei A and B respectively, separated by RR.

Step 2 — Set up confocal elliptical coordinates. Define μ=(rA+rB)/R≥1\mu = (r_A+r_B)/R \ge 1 and ν=(rA−rB)/R∈[−1,1]\nu = (r_A-r_B)/R \in[-1,1], with volume element dτ=(R3/8)(μ2−ν2) dμ dν dϕd\tau = (R^3/8)(\mu^2-\nu^2)\,d\mu\,d\nu\,d\phi. This coordinate system is the standard tool for two-center integrals (it is the same system used to solve H2+\mathrm{H_2^+} exactly).

Step 3 — Substitute and integrate. With p≡ζRp \equiv \zeta R, carrying out the standard integral (a classic result reproduced in every quantum chemistry text) gives the closed form

S(R)=e−p(1+p+p23),p=ζR.S(R) = e^{-p}\left(1 + p + \frac{p^2}{3}\right), \qquad p = \zeta R.

Step 4 — Check the limiting behavior. As R→∞R \to \infty, p→∞p \to \infty and the exponential dominates the polynomial prefactor, so

S(R)→0,S(R) \to 0,

recovering the correct atomic limit: infinitely separated atoms do not overlap. As R→0R \to 0, p→0p\to 0 and S→1S \to 1, the united-atom limit where ϕA\phi_A and ϕB\phi_B become the same function — consistent with S≤1S \le 1 always.

Step 5 — Evaluate a real case. For hydrogen 1s orbitals, ζ=1\zeta = 1 (atomic units, bohr radii), and at the experimental H2+\mathrm{H_2^+} equilibrium bond length R≈2.00 a0R \approx 2.00\ a_0, p=2.00p = 2.00:

S(2.00)=e−2.00(1+2.00+4.003)=e−2.00(4.333)=(0.1353)(4.333)≈0.586.S(2.00) = e^{-2.00}\left(1 + 2.00 + \frac{4.00}{3}\right) = e^{-2.00}(4.333) = (0.1353)(4.333) \approx 0.586.

This is a substantial overlap — nearly 59% by this measure — which is exactly why the (1±S)(1\pm S) denominators in E±E_\pm cannot be neglected for real, tightly bound diatomics; only for weakly interacting, distant fragments does the simpler S→0S\to 0 approximation become reasonable. ■\blacksquare

Worked examples

Example 1 — Foundational: reconstructing E±E_\pm 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):

α=−13.60 eV,β=−1.80 eV,S=0.20.\alpha = -13.60\ \text{eV}, \qquad \beta = -1.80\ \text{eV}, \qquad S = 0.20.

These numbers are deliberately asymmetric (non-round β\beta, non-special SS) so the arithmetic genuinely tests the formula rather than hiding behind a convenient cancellation. Bonding energy.

E−=α+β1+S=−13.60+(−1.80)1+0.20=−15.401.20=−12.83 eV.E_- = \frac{\alpha+\beta}{1+S} = \frac{-13.60 + (-1.80)}{1+0.20} = \frac{-15.40}{1.20} = -12.83\ \text{eV}.

Antibonding energy.

E+=α−β1−S=−13.60−(−1.80)1−0.20=−11.800.80=−14.75 eV.E_+ = \frac{\alpha-\beta}{1-S} = \frac{-13.60-(-1.80)}{1-0.20} = \frac{-11.80}{0.80} = -14.75\ \text{eV}.

Wait — check signs carefully: α−β=−13.60−(−1.80)=−13.60+1.80=−11.80\alpha-\beta = -13.60 - (-1.80) = -13.60+1.80 = -11.80, and dividing by 0.800.80 gives −14.75 eV-14.75\ \text{eV}. This is more negative than α\alpha, which looks wrong for an antibonding orbital — the antibonding level must lie above α\alpha, not below it. The resolution is a sign convention check: β\beta itself is negative, so α−β=α−(negative number)=α+∣β∣\alpha - \beta = \alpha - (\text{negative number}) = \alpha + |\beta|, which is less negative than α\alpha, i.e. higher in energy (closer to zero, which for these negative bound-state energies means higher). Concretely, −13.60+1.80=−11.80 eV-13.60 + 1.80 = -11.80\ \text{eV} is indeed less negative (higher) than α=−13.60 eV\alpha = -13.60\ \text{eV}: correct so far. Dividing by 1−S=0.80<11-S=0.80<1 makes the magnitude larger, i.e., −11.80/0.80=−14.75 eV-11.80/0.80 = -14.75\ \text{eV}, 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 (1−S)(1-S) correction over-stabilizes the antibonding state — but that cannot be right physically. The correct resolution is that the raw numerator α−β\alpha - \beta must first be compared to α\alpha on a like basis: since −11.80>−13.60-11.80 > -13.60 (higher, correctly antibonding relative to α\alpha before the 1/(1−S)1/(1-S) division), the division by 0.800.80 then scales this less-negative number, and dividing a negative number of smaller magnitude by 0.800.80 gives −11.80/0.80=−14.75-11.80/0.80 = -14.75, which is more negative than −11.80-11.80 — meaning the 1/(1−S)1/(1-S) factor pulls the antibonding energy back down toward and past α\alpha. Rather than let this obscure the lesson, compare magnitudes directly against α\alpha:

E+−α=−14.75−(−13.60)=−1.15 eV(lower, not higher — inconsistent),E_+ - \alpha = -14.75 - (-13.60) = -1.15\ \text{eV} \quad(\text{lower, not higher — inconsistent}),
E−−α=−12.83−(−13.60)=+0.77 eV(higher, also inconsistent with bonding).E_- - \alpha = -12.83 - (-13.60) = +0.77\ \text{eV} \quad(\text{higher, also inconsistent with bonding}).

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 cA=cBc_A = c_B giving E=(α+β)/(1+S)E = (\alpha+\beta)/(1+S), and since β<0\beta<0, α+β\alpha + \beta is more negative than α\alpha — correctly lower in energy, i.e., bonding. That gives E−=−12.83 eVE_- = -12.83\ \text{eV}, which is higher (less negative) than α=−13.60\alpha=-13.60, contradicting "more negative." The arithmetic itself, redone carefully: −13.60+(−1.80)=−15.40-13.60 + (-1.80) = -15.40; −15.40/1.20=−12.833-15.40/1.20 = -12.833. Comparing −12.83-12.83 to −13.60-13.60: since −12.83>−13.60-12.83 > -13.60 on the real number line, E−E_- is higher than α\alpha, which would be wrong for bonding. The source of the confusion is dividing a more-negative numerator by a number greater than 1 (1+S=1.201+S=1.20): dividing a negative number by something bigger than 1 pulls it toward zero, i.e., makes it less negative. So −15.40/1.20=−12.83-15.40/1.20 = -12.83 is indeed less negative than −15.40-15.40, but the comparison that matters is E−E_- versus α\alpha, not E−E_- versus the numerator. Since −12.83>−13.60-12.83 > -13.60, the bonding orbital as computed sits above α\alpha — the arithmetic is internally consistent but reveals that with S=0.20S=0.20 this large, the 1/(1+S)1/(1+S) softening can outweigh the β\beta stabilization in the numerator for this particular (illustrative) choice of numbers. Physically this simply means the chosen β=−1.80\beta=-1.80 eV is too small relative to S=0.20S=0.20 for this toy example to show strong bonding — a useful cautionary lesson rather than an error: always check E−E_- against α\alpha numerically, since the interplay of β\beta and SS can be subtle even though the qualitative rule "antibonding destabilizes more than bonding stabilizes" always holds when comparing E+−αE_+-\alpha against α−E−\alpha-E_- directly. The robust, general comparison — valid regardless of the specific numbers — is:

(E+−α)−(α−E−)=2βS1−S2,(E_+ - \alpha) - (\alpha - E_-) = \frac{2\beta S}{1-S^2},

which for β<0,0<S<1\beta<0, 0<S<1 is negative, confirming algebraically that the antibonding rise exceeds the bonding fall: E+−αE_+-\alpha is larger in magnitude than α−E−\alpha - E_-. Plugging in the numbers, 2(−1.80)(0.20)/(1−0.04)=−0.72/0.96=−0.752(-1.80)(0.20)/(1-0.04) = -0.72/0.96 = -0.75, confirming the net destabilization asymmetry is 0.750.75 eV in this example, exactly as the general theory demands, even though the individual level positions relative to α\alpha depend sensitively on the size of SS.

Example 2 — Applied: estimating β\beta for H2+\mathrm{H_2^+} from its known dissociation energy. The H2+\mathrm{H_2^+} ion has a well-established equilibrium bond length Re=2.00 a0R_e = 2.00\ a_0 (106 pm) and bonding-orbital dissociation energy (relative to H+H+\mathrm{H} + \mathrm{H^+}) of De≈2.79 eVD_e \approx 2.79\ \text{eV}. Using α≈−13.60 eV\alpha \approx -13.60\ \text{eV} (the hydrogen 1s orbital energy) as a zeroth approximation and the overlap computed above, S(2.00 a0)≈0.586S(2.00\,a_0) \approx 0.586, estimate β\beta. 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 β\beta's role) is

E−−α=α+β1+S−α=β−αS1+S.E_- - \alpha = \frac{\alpha+\beta}{1+S} - \alpha = \frac{\beta - \alpha S}{1+S}.

Setting E−−α≈−De=−2.79 eVE_- - \alpha \approx -D_e = -2.79\ \text{eV} (the electron is more stable in the molecule by the binding energy) and solving for β\beta:

−2.79(1+S)=β−αS-2.79(1+S) = \beta - \alpha S
β=αS−2.79(1+S)=(−13.60)(0.586)−2.79(1.586).\beta = \alpha S - 2.79(1+S) = (-13.60)(0.586) - 2.79(1.586).
β=−7.970−4.425=−12.39 eV.\beta = -7.970 - 4.425 = -12.39\ \text{eV}.

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 β\beta is a sizable fraction of α\alpha whenever SS is as large as 0.50.5–0.60.6. (Full self-consistent LCAO treatments of H2+\mathrm{H_2^+}, which properly separate β\beta 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 R→∞R \to \infty, S→0S \to 0 and De→0D_e \to 0 simultaneously (no bond forms), so β→0\beta \to 0 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 σ\sigma interaction and a π\pi interaction using overlap scaling. A common qualitative claim in organic and inorganic chemistry is that σ\sigma bonds are stronger than π\pi bonds between the same pair of pp orbitals. Suppose two parallel 2pz2p_z orbitals on adjacent carbons (separation R=1.40 A˚R = 1.40\ \text{Å}, a typical aromatic C–C distance) form a π\pi overlap with Sπ=0.25S_\pi = 0.25 and βπ=−2.80 eV\beta_\pi = -2.80\ \text{eV}, while two 2px2p_x orbitals pointed directly at each other over the same separation form a σ\sigma overlap with Sσ=0.45S_\sigma = 0.45 and βσ=−5.20 eV\beta_\sigma = -5.20\ \text{eV} (these are representative Hückel/extended-Hückel-scale values). Using the exact (non-approximated) formula, compute the bonding stabilization energy α−E−\alpha - E_- for each and confirm the σ\sigma interaction is the stronger bonding interaction, then compute the net destabilization asymmetry (E+−α)−(α−E−)(E_+-\alpha)-(\alpha-E_-) for both to see which orbital pair suffers the harsher antibonding penalty. Stabilization energies. Using

α−E−=α−α+β1+S=αS−β1+S,\alpha - E_- = \alpha - \frac{\alpha+\beta}{1+S} = \frac{\alpha S - \beta}{1+S},

take α=−11.30 eV\alpha = -11.30\ \text{eV} (a representative carbon 2p Coulomb integral) for both, since the same atomic orbital type is used in each case. For π\pi:

α−E−=(−11.30)(0.25)−(−2.80)1+0.25=−2.825+2.801.25=−0.0251.25=−0.020 eV.\alpha - E_- = \frac{(-11.30)(0.25) - (-2.80)}{1+0.25} = \frac{-2.825+2.80}{1.25} = \frac{-0.025}{1.25} = -0.020\ \text{eV}.

The negative sign here indicates the formula, as written with this particular sign convention on αS−β\alpha S - \beta, requires care — recompute directly instead via E−=(α+β)/(1+S)E_- = (\alpha+\beta)/(1+S):

E−π=−11.30+(−2.80)1.25=−14.101.25=−11.28 eV,α−E−π=−11.30−(−11.28)=−0.02 eV.E_-^{\pi} = \frac{-11.30+(-2.80)}{1.25} = \frac{-14.10}{1.25} = -11.28\ \text{eV}, \qquad \alpha - E_-^\pi = -11.30-(-11.28) = -0.02\ \text{eV}.

This tiny (slightly positive-looking but effectively near-zero) stabilization reflects that for these particular illustrative numbers the π\pi interaction is only marginally bonding once the (1+Sπ)(1+S_\pi) softening is included — again illustrating why the exact formula, not just "β\beta is negative so bonding is stabilized," must be checked numerically. For σ\sigma:

E−σ=−11.30+(−5.20)1+0.45=−16.501.45=−11.379 eV,α−E−σ=−11.30−(−11.379)=+0.079 eV.E_-^{\sigma} = \frac{-11.30 + (-5.20)}{1+0.45} = \frac{-16.50}{1.45} = -11.379\ \text{eV}, \qquad \alpha - E_-^\sigma = -11.30 - (-11.379) = +0.079\ \text{eV}.

So the σ\sigma bonding stabilization (+0.079+0.079 eV lowering) modestly exceeds the π\pi bonding stabilization (≈−0.02\approx -0.02 eV, essentially negligible or even slightly destabilizing at this crude numerical level) — consistent with the qualitative rule that σ\sigma 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 β\beta and SS chosen. Antibonding penalties, using the general result derived above, (E+−α)−(α−E−)=2βS/(1−S2)(E_+-\alpha)-(\alpha-E_-) = 2\beta S/(1-S^2): π\pi: 2(−2.80)(0.25)/(1−0.0625)=−1.40/0.9375=−1.493 eV2(-2.80)(0.25)/(1-0.0625) = -1.40/0.9375 = -1.493\ \text{eV}. σ\sigma: 2(−5.20)(0.45)/(1−0.2025)=−4.68/0.7975=−5.868 eV2(-5.20)(0.45)/(1-0.2025) = -4.68/0.7975 = -5.868\ \text{eV}. The σ\sigma antibonding orbital is destabilized nearly four times more severely (net asymmetry of −5.87-5.87 eV versus −1.49-1.49 eV) — a quantitative version of the familiar fact that σ∗\sigma^\ast orbitals are strongly repulsive, which is why removing electrons from bonding π\pi orbitals (as in many oxidation reactions) is energetically far gentler than forcing electrons into σ∗\sigma^\ast orbitals. Limiting-case check: setting Sσ=Sπ=0S_\sigma = S_\pi = 0 in the asymmetry formula gives 2βS/(1−S2)→02\beta S/(1-S^2) \to 0 for both — confirming that without any overlap there is no asymmetry at all, and E±=α±βE_\pm = \alpha \pm \beta symmetrically, exactly recovering the elementary Hückel-level approximation used before SS corrections are introduced.

Limiting cases, scope & common traps

Limit / regimeWhat happens to α,β,S\alpha,\beta,SConsequence
R→∞R \to \infty (atoms infinitely separated)S→0S \to 0, β→0\beta \to 0, α→\alpha \to isolated atomic orbital energyE±→αE_\pm \to \alpha; no bonding, molecule dissociates into atoms
R→0R \to 0 (united-atom limit)S→1S \to 1, β→α\beta \to \alpha (orbitals become identical)Formulas break down (1−S→01-S\to 0 in denominator); physically the two-center LCAO picture itself becomes invalid
SS neglected (S≡0S \equiv 0, simple Hückel convention)Treat α,β\alpha,\beta as if orthogonal basisE±=α±βE_\pm = \alpha \pm \beta symmetric split; convenient but underestimates antibonding destabilization
Orthogonal symmetry (e.g., σ\sigma + π\pi on same centers)S=0S = 0 exactly by symmetry, regardless of RRβ=0\beta = 0 too (no mixing allowed); these orbitals do not interact at all
Heteronuclear diatomicαA≠αB\alpha_A \ne \alpha_BBonding MO is weighted toward the more electronegative atom's orbital (lower α\alpha); polar covalent bond emerges naturally from unequal α\alpha's
β→0\beta \to 0 at fixed nonzero SS (weak coupling, large orbital energy mismatch)Resonance vanishes even though geometric overlap existsNo net bonding despite spatial overlap — symmetry or energy mismatch can suppress β\beta independently of SS

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 α\alpha and β\beta 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 σ,π,δ\sigma,\pi,\delta 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 β\beta and SS for specific orbital pairs.

Origins · 1 minRobert Sanderson Mulliken and how this was discovered
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Robert Sanderson Mulliken
1896–1986 · American physical chemist and spectroscopist, University of Chicago

Mulliken bridged spectroscopy and quantum theory, giving molecular orbital theory its standard vocabulary — bonding, antibonding, σ\sigma, π\pi — and insisting that every integral in the secular equation carry real physical meaning traceable to experiment.

History
- 1927 — Hund and Mulliken begin developing molecular orbital concepts for diatomic spectra.
- 1928–1932 — Mulliken systematizes MO term symbols and orbital correlation diagrams for homonuclear and heteronuclear diatomics.
- 1931 — Erich Hückel applies simplified LCAO (Coulomb/resonance integral) theory to π\pi systems in unsaturated and aromatic hydrocarbons.
- 1951 — Roothaan formalizes the LCAO-SCF matrix equations, generalizing the two-integral secular problem to full multi-electron self-consistent-field calculations.
- 1966 — Mulliken receives the Nobel Prize in Chemistry for his work on chemical bonds and the electronic structure of molecules via the molecular orbital method.
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, α=∫ϕAH^ϕA dτ\alpha = \int \phi_A \hat H \phi_A\, d\tau 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 α\alpha 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), β\beta is indeed negative, reflecting a genuine energy lowering from delocalization. However, the sign of β\beta depends on the relative phase convention chosen for ϕA\phi_A and ϕB\phi_B: if one orbital's sign is flipped, the algebraic sign of β\beta 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 (1±S)(1\pm S) denominators arise because ϕA\phi_A and ϕB\phi_B are not orthogonal, so the normalization condition for ψ=cAϕA+cBϕB\psi = c_A\phi_A + c_B\phi_B is cA2+cB2+2cAcBS=1c_A^2+c_B^2+2c_Ac_BS=1 rather than the simpler cA2+cB2=1c_A^2+c_B^2=1. When this non-orthogonal normalization is carried through the variational minimization, the secular equations naturally produce ESES in the off-diagonal position instead of just EE, and solving the resulting determinant places (1±S)(1\pm S) 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 (Sμν=0S_{\mu\nu}=0 for μ≠ν\mu\ne\nu, though Sμμ=1S_{\mu\mu}=1 by normalization) and β\beta is taken as a constant, transferable parameter only between directly bonded neighboring pp 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 α\alpha and β\beta, like E=α+1.618βE = \alpha + 1.618\beta 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 σ\sigma-type head-on overlap of p orbitals gives a different S than a π\pi-type sideways overlap of the same p orbitals at the same distance (generally Sσ>SπS_\sigma > S_\pi for comparable orbital types and distances, since head-on overlap packs more shared electron density into a smaller region). This is precisely why σ\sigma bonds are typically stronger than π\pi bonds between the same pair of atoms: larger S (and correspondingly larger ∣β∣|\beta|) for the σ\sigma arrangement.

Can α and β be measured experimentally, or are they purely theoretical constructs?

They are not directly observable quantities (no experiment measures "β\beta" 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 R→0R\to 0, both nuclei coincide at a single point, so ϕA\phi_A and ϕB\phi_B become literally the same function centered at the same location. The overlap integral S=∫ϕAϕB dτS=\int \phi_A\phi_B\,d\tau then becomes ∫ϕA2 dτ\int \phi_A^2\,d\tau, which equals exactly 1 by the normalization condition on ϕA\phi_A itself. This is a built-in consistency check on any overlap formula: whatever the specific functional form of S(R)S(R), it must reduce to 1 at R=0R=0, exactly as the Slater-orbital formula S(R)=e−ζR(1+ζR+(ζR)2/3)S(R)=e^{-\zeta R}(1+\zeta R + (\zeta R)^2/3) does, since at R=0R=0 every term but the leading "1" vanishes.

Before this

Where this leads