Valence Bond versus Molecular Orbital Theory

Take one hydrogen molecule. Stretch its bond from equilibrium out to twenty angstroms. Ask two theories to predict the energy along the way. Simple molecular orbital theory says the electrons stay pleasantly delocalized right up to that absurd separation. It reports a spurious, finite binding energy for two atoms that are, by any chemical instinct, no longer bonded at all. Simple valence bond theory, restricted from the start to purely covalent pairing, gets the dissociation limit qualitatively right. But it pays for this at short range, where it neglects an ionic contribution that the true wavefunction badly wants. Neither simple picture is the full story. The tension between them is one of the most instructive contrasts in the whole of quantum chemistry. This comparison matters because VB and MO theory are not two competing final answers. They are two different bookkeeping schemes for the same underlying Schrödinger equation. Each encodes a different chemical intuition. MO theory builds delocalized orbitals first and fills them with electrons. This is the natural language of bands, aromaticity, and spectroscopy. VB theory builds bonds from overlapping atomic orbitals and superposes covalent and ionic structures. This is the natural language of curly arrows, resonance, and directed bonding discussed under Directed Bonding and Molecular Geometry from VB Theory. Both start from the same two-electron, two-nucleus Hamiltonian. Both are approximations built from a restricted set of configurations. Both converge, when pushed far enough with configuration interaction, to the same exact answer. The big picture is that simple MO theory over-delocalizes. It shows too much ionic character at all distances, including infinity. Simple VB theory under-delocalizes instead. It shows no ionic character at any distance, even at equilibrium where some is needed. The cure in each case is the same: mix in the configurations the simple theory left out. For MO theory this means configuration interaction between the ground and doubly-excited determinants. For VB theory it means adding ionic structures to the covalent one. This is exactly the weighting scheme introduced in Covalent and Ionic Contributions to the Bond. Done properly, both routes reconstruct the same multi-configurational wavefunction. The historical "VB versus MO" rivalry dissolves into a single variational problem viewed from two coordinate systems. This article works through the H₂ molecule in full. It covers the explicit forms of the simple MO and simple VB wavefunctions. It shows their expansion in the same atomic-orbital basis, to reveal exactly what each one is missing. It examines the dissociation-limit pathology of MO theory and the equilibrium-bond pathology of VB theory. It traces the convergence of both toward the exact two-electron wavefunction. This convergence happens once ionic terms (VB side) or excited determinants (MO side) are included. Two full derivations, three worked numerical examples, and a systematic trap-table are given. Every claim can therefore be checked by hand.

Key takeaways
  • The simple MO wavefunction for H₂ is one doubly-occupied bonding orbital; expanded in atomic orbitals it contains 50% covalent + 50% ionic character at every internuclear distance, including infinity.
  • The simple VB (Heitler–London) wavefunction is purely covalent, with zero ionic character, which is qualitatively right at large R but misses stabilization near Rₑ.
  • MO theory dissociates to a 1:1 mixture of H + H and H⁺ + H⁻, giving a nonzero, unphysical binding energy at infinite separation.
  • VB theory dissociates correctly to neutral atoms but underestimates the well depth and equilibrium bond strength because it excludes ionic resonance.
  • Adding configuration interaction (MO side: mix in the doubly-excited determinant) or adding ionic structures with a variational weight (VB side) makes the two wavefunctions algebraically identical.
  • Both theories are approximations to one exact non-relativistic wavefunction; the "argument" between them is a disagreement about which truncation of the same expansion is more chemically transparent.
  • Key idea: simple MO and simple VB wavefunctions are complementary linear combinations of the same covalent and ionic Slater determinants — each keeps one term and gets the wrong ratio, and full CI restores the correct mixture at every geometry.

Where this lives today

Modern electronic structure software still descends from both lineages, and the choice of framework is far from academic. Hartree–Fock and Kohn–Sham density functional theory, the workhorses of routine computational chemistry in drug discovery and materials screening, are direct descendants of the molecular orbital picture; their single-determinant (or single-Kohn–Sham-determinant) starting point inherits exactly the same dissociation pathology analyzed here, which is why naive DFT bond-breaking curves for radicals, transition-metal spin states, and homolytic cleavage reactions can be qualitatively wrong unless multireference or broken-symmetry corrections are applied. Anyone modeling a reaction that breaks a covalent bond homolytically — radical polymerization initiation, C–H activation transition states, or photodissociation — needs to know exactly the static-correlation error this article derives, because it silently corrupts single-reference calculations exactly in the bond-breaking region chemists care about most. Valence bond methods, meanwhile, survive both as a pedagogical language (curly arrows, resonance structures, orbital hybridization) and as active modern computational tools: spin-coupled valence bond theory, breathing-orbital VB, and VB self-consistent field methods are used today to dissect reaction mechanisms into explicit covalent and ionic (or diabatic) contributions, particularly useful for charge-transfer states in photochemistry, diradical intermediates in pericyclic reactions, and describing bond-breaking without the artificial symmetry-breaking that plagues restricted MO methods. Multiconfigurational methods such as CASSCF and its variants are, in the language of this article, simply full CI within a chosen active space — they are the rigorous unification point where "VB versus MO" stops being a meaningful distinction, because both limits are contained inside the same configuration expansion, weighted by whatever the variational principle demands at each geometry. Understanding the H₂ case in full — the 50:50 MO ratio, the pure-covalent VB limit, and the CI bridge between them — is the cleanest possible entry point into why every serious quantum chemistry package needs, in one guise or another, a multireference option.

Ask the tutor: Can you show me how the 2×2 VB-CI matrix elements H_cc, H_ii, and H_ci are actually computed from the Coulomb, exchange, and overlap integrals over 1s Slater orbitals?

The physical picture

Consider H₂ with nuclei aa and bb, each carrying a 1s atomic orbital, χa\chi_a and χb\chi_b, and two electrons labeled 1 and 2. Any acceptable two-electron spatial wavefunction for this problem, expanded in just these two atomic orbitals, must be some combination of exactly four possible electron arrangements: electron 1 near aa and electron 2 near bb (or vice versa) — the covalent arrangements — and both electrons near the same nucleus, aa or bb — the ionic arrangements corresponding to H⁻H⁺ and H⁺H⁻. Simple MO theory and simple VB theory are two different, and differently wrong, ways of weighting these four arrangements. The molecular orbital route builds one delocalized bonding orbital,

σg=χa+χb2(1+S),\sigma_g = \frac{\chi_a + \chi_b}{\sqrt{2(1+S)}},

where S=⟨χa∣χb⟩S = \langle \chi_a|\chi_b\rangle is the atomic-orbital overlap integral, and then puts both electrons into it with opposite spins: ΨMO=σg(1)σg(2) [α(1)β(2)−β(1)α(2)]/2\Psi_{\text{MO}} = \sigma_g(1)\sigma_g(2)\,[\alpha(1)\beta(2)-\beta(1)\alpha(2)]/\sqrt2. Because σg\sigma_g itself is delocalized over both centers, squaring it to build the two-electron density automatically generates covalent and ionic terms in a fixed, geometry-independent ratio. This is the root of the dissociation catastrophe: no matter how far apart the atoms sit, the orbital used to describe each electron is still "half on aa, half on bb," so the wavefunction insists on retaining 50% ionic character forever. The valence bond route instead builds the wavefunction directly from the covalent picture: electron 1 in χa\chi_a and electron 2 in χb\chi_b, plus the electron-exchanged term required by indistinguishability, giving the Heitler–London function

ΨVB=χa(1)χb(2)+χb(1)χa(2)2(1+S2).\Psi_{\text{VB}} = \frac{\chi_a(1)\chi_b(2) + \chi_b(1)\chi_a(2)}{\sqrt{2(1+S^2)}}.

This function never lets both electrons sit on the same nucleus — it is purely covalent by construction — so it dissociates flawlessly to two neutral, spin-paired hydrogen atoms. Its failure is the opposite one: near the equilibrium distance, where quantum mechanics really does want a modest admixture of ionic character to lower the energy further, simple VB has no ionic terms available to mix in, so it underestimates the binding energy and gets a bond length slightly too long.

Figure
Four atomic-orbital arrangements underlying both wavefunctions
The four terms hidden inside every H₂ wavefunction 1 2 χₐ(1)χᵦ(2) covalent 2 1 χᵦ(1)χₐ(2) covalent 1,2 χₐ(1)χₐ(2) ionic H⁻H⁺ 1,2 χᵦ(1)χᵦ(2) ionic H⁺H⁻ Simple VB keeps only the two covalent terms (equal weight). Simple MO keeps all four terms, but forces covalent : ionic = 1 : 1 at every R. Full CI finds the correct, R-dependent mixture of all four.

At the equilibrium bond distance, the exact ratio of ionic to covalent weight is small but nonzero — chemical intuition and experiment agree that H₂ is overwhelmingly covalent but slightly "ionic-resonance-stabilized." Simple MO theory forces a 50:50 ratio that is wildly too ionic; simple VB theory forces a 0% ionic ratio that is too covalent. Both are wrong in exactly the direction their construction predicts, and the size of each error can be computed explicitly, which is the point of the two derivations below.

Figure
Potential energy curves: the two failure modes
E(R) for H₂: simple MO, simple VB, and exact R E 2 × E(H atom) exact / full CI simple VB (too shallow, right limit) simple MO (wrong asymptote, too low) MO never reaches the correct dissociation limit

The core ideas

The whole comparison rests on writing every wavefunction in the same four-term atomic-orbital basis and reading off the covalent and ionic coefficients directly.

ΨMO(1,2)=σg(1)σg(2)=12(1+S)[χa(1)χa(2)+χb(1)χb(2)+χa(1)χb(2)+χb(1)χa(2)]\Psi_{\text{MO}}(1,2) = \sigma_g(1)\sigma_g(2) = \frac{1}{2(1+S)}\Big[\chi_a(1)\chi_a(2) + \chi_b(1)\chi_b(2) + \chi_a(1)\chi_b(2) + \chi_b(1)\chi_a(2)\Big]

where: σg=(χa+χb)/2(1+S)\sigma_g = (\chi_a+\chi_b)/\sqrt{2(1+S)} is the normalized bonding MO, and the spin singlet factor is suppressed since it is common to both theories. Reading: expanding the square of the sum (χa+χb)(\chi_a+\chi_b) over both electrons produces all four arrangements — two covalent, two ionic — with identical coefficients. The MO wavefunction cannot distinguish "ionic" from "covalent" weighting because it was never given the freedom to do so; the ratio is baked in by the algebra of squaring a delocalized orbital.

ΨVB(1,2)=12(1+S2)[χa(1)χb(2)+χb(1)χa(2)]\Psi_{\text{VB}}(1,2) = \frac{1}{\sqrt{2(1+S^2)}}\Big[\chi_a(1)\chi_b(2) + \chi_b(1)\chi_a(2)\Big]

where: this is the Heitler–London function, containing only the two covalent arrangements with equal weight and no ionic terms at all. Reading: VB theory imposes the opposite constraint — ionic terms are simply absent — which is exact only in the limit R→∞R \to \infty, where the true wavefunction genuinely has zero ionic weight (moving an electron from one atom to the other costs a finite ionization/affinity energy that becomes infinitely expensive relative to zero coupling at infinite separation).

ΨCI=ccov ΨVB+cion Ψion,Ψion=χa(1)χa(2)+χb(1)χb(2)2(1+S2)\Psi_{\text{CI}} = c_{\text{cov}}\,\Psi_{\text{VB}} + c_{\text{ion}}\,\Psi_{\text{ion}}, \qquad \Psi_{\text{ion}} = \frac{\chi_a(1)\chi_a(2)+\chi_b(1)\chi_b(2)}{\sqrt{2(1+S^2)}}

where: ccovc_{\text{cov}} and cionc_{\text{ion}} are variationally optimized mixing coefficients found by diagonalizing the 2×22\times2 Hamiltonian matrix in the {covalent, ionic} basis, and Ψion\Psi_{\text{ion}} is the normalized symmetric combination of the two ionic structures. Reading: this is the full valence bond CI wavefunction — VB theory's route to the exact answer. It contains the same four determinants as ΨMO\Psi_{\text{MO}} but with a variable, RR-dependent ratio cion/ccovc_{\text{ion}}/c_{\text{cov}} instead of the fixed ratio 1 that simple MO theory imposes.

ΨMO-CI=c1 σg(1)σg(2)−c2 σu(1)σu(2),σu=χa−χb2(1−S)\Psi_{\text{MO-CI}} = c_1\,\sigma_g(1)\sigma_g(2) - c_2\,\sigma_u(1)\sigma_u(2), \qquad \sigma_u = \frac{\chi_a-\chi_b}{\sqrt{2(1-S)}}

where: σu\sigma_u is the antibonding MO, c1,c2c_1,c_2 are CI coefficients, and the minus sign convention keeps both terms real and the ionic content controllable. Reading: this is MO theory's route to the exact answer — mixing in the doubly-excited configuration (σu)2(\sigma_u)^2 subtracts away ionic character as c2/c1c_2/c_1 grows, precisely canceling the excess ionic weight that plain (σg)2(\sigma_g)^2 carries. At R→∞R\to\infty, c1→c2c_1 \to c_2 in magnitude and the ionic terms cancel exactly, restoring the correct dissociation limit.

Derivation AWhy simple MO theory is exactly 50% ionic, and only 50% ionic, at every R

Goal. Show algebraically that squaring the bonding MO forces equal covalent and ionic weight regardless of internuclear distance, and quantify the resulting dissociation error.

Step 1 — Write the bonding orbital and normalize it. Take real, normalized 1s orbitals χa,χb\chi_a,\chi_b with overlap S=⟨χa∣χb⟩S=\langle\chi_a|\chi_b\rangle. The symmetric (bonding) combination is

σg=N(χa+χb),N2∫(χa+χb)2 dτ=1.\sigma_g = N(\chi_a + \chi_b), \qquad N^2\int(\chi_a+\chi_b)^2\,d\tau = 1.

Expanding the normalization integral, ∫(χa+χb)2=∫χa2+∫χb2+2∫χaχb=1+1+2S\int(\chi_a+\chi_b)^2 = \int\chi_a^2 + \int\chi_b^2 + 2\int\chi_a\chi_b = 1+1+2S, so

N=12(1+S).N = \frac{1}{\sqrt{2(1+S)}}.

Step 2 — Place both electrons in σg\sigma_g with opposite spin. The spatial part of the two-electron ground configuration is the simple product

ΨMO(1,2)=σg(1) σg(2)=N2[χa(1)+χb(1)][χa(2)+χb(2)].\Psi_{\text{MO}}(1,2) = \sigma_g(1)\,\sigma_g(2) = N^2\big[\chi_a(1)+\chi_b(1)\big]\big[\chi_a(2)+\chi_b(2)\big].

Step 3 — Expand the product into the four atomic-orbital arrangements. Multiplying out term by term,

ΨMO(1,2)=N2[χa(1)χa(2)⏟ionic a+χb(1)χb(2)⏟ionic b+χa(1)χb(2)⏟covalent+χb(1)χa(2)⏟covalent].\Psi_{\text{MO}}(1,2) = N^2\Big[\underbrace{\chi_a(1)\chi_a(2)}_{\text{ionic }a} + \underbrace{\chi_b(1)\chi_b(2)}_{\text{ionic }b} + \underbrace{\chi_a(1)\chi_b(2)}_{\text{covalent}} + \underbrace{\chi_b(1)\chi_a(2)}_{\text{covalent}}\Big].

Every one of the four terms carries the same coefficient N2=1/[2(1+S)]N^2 = 1/[2(1+S)] — nothing in this expansion distinguishes covalent from ionic weighting, because σg\sigma_g itself has equal amplitude on both centers by symmetry, and squaring a sum of equal-amplitude terms always redistributes weight equally among the cross terms.

Step 4 — Read off the covalent-to-ionic ratio. Grouping covalent and ionic pieces,

ΨMO∝[χa(1)χb(2)+χb(1)χa(2)]⏟covalent, weight 2N2+[χa(1)χa(2)+χb(1)χb(2)]⏟ionic, weight 2N2.\Psi_{\text{MO}} \propto \underbrace{\big[\chi_a(1)\chi_b(2)+\chi_b(1)\chi_a(2)\big]}_{\text{covalent, weight }2N^2} + \underbrace{\big[\chi_a(1)\chi_a(2)+\chi_b(1)\chi_b(2)\big]}_{\text{ionic, weight }2N^2}.

The probability weight ratio (before final normalization, which is common to both groups) is

PionicPcovalent=(2N2)2(2N2)2=1\frac{P_{\text{ionic}}}{P_{\text{covalent}}} = \frac{(2N^2)^2}{(2N^2)^2} = 1

independent of SS, and therefore independent of RR. This holds even as R→∞R\to\infty, where S→0S\to 0 but the ratio stays exactly 1.

Step 5 — Translate into a physical error at dissociation. At R→∞R\to\infty the true wavefunction must be purely covalent (an electron transferring from a neutral H atom to its distant partner costs the full ionization energy minus electron affinity, roughly 13.6−0.75≈12.85 eV13.6 - 0.75 \approx 12.85\text{ eV} per H, with no compensating overlap stabilization). Simple MO theory nonetheless keeps 50% ionic (H⁻H⁺ + H⁺H⁻) weight forever, which is why the restricted Hartree–Fock dissociation energy of H₂ converges to a value corresponding to a 1:1 mixture of neutral atoms and ion pairs rather than to two free atoms — the classic symptom of static correlation error in single-determinant theory.

Go deeper · Derivation B · 2 minWhy simple VB theory underbinds at equilibrium, and how mixing in ionic structures fixes it
Derivation BWhy simple VB theory underbinds at equilibrium, and how mixing in ionic structures fixes it

Goal. Set up the 2×22\times 2 ionic–covalent CI problem explicitly and show that including even a small ionic admixture always lowers the ground-state energy relative to pure Heitler–London, recovering part of the missing binding.

Step 1 — Define the covalent and ionic VB structures. Let

Ψcov=χa(1)χb(2)+χb(1)χa(2)2(1+S2),Ψion=χa(1)χa(2)+χb(1)χb(2)2(1+S2),\Psi_{\text{cov}} = \frac{\chi_a(1)\chi_b(2)+\chi_b(1)\chi_a(2)}{\sqrt{2(1+S^2)}}, \qquad \Psi_{\text{ion}} = \frac{\chi_a(1)\chi_a(2)+\chi_b(1)\chi_b(2)}{\sqrt{2(1+S^2)}},

both built from the same singlet spin function, both individually normalized. Note ⟨Ψcov∣Ψion⟩≠0\langle\Psi_{\text{cov}}|\Psi_{\text{ion}}\rangle \neq 0 in general because they share atomic orbitals, but for a clean variational treatment one works in the basis where this overlap is retained explicitly (generalized eigenvalue problem) or removed by Löwdin orthogonalization; the qualitative conclusion below is unaffected.

Step 2 — Build the 2×22\times2 Hamiltonian matrix. Define

Hcc=⟨Ψcov∣H^∣Ψcov⟩=EHL,Hii=⟨Ψion∣H^∣Ψion⟩,Hci=⟨Ψcov∣H^∣Ψion⟩,H_{\text{cc}} = \langle \Psi_{\text{cov}}|\hat H|\Psi_{\text{cov}}\rangle = E_{\text{HL}}, \qquad H_{\text{ii}} = \langle \Psi_{\text{ion}}|\hat H|\Psi_{\text{ion}}\rangle, \qquad H_{\text{ci}} = \langle \Psi_{\text{cov}}|\hat H|\Psi_{\text{ion}}\rangle,

where EHLE_{\text{HL}} is exactly the simple (pure covalent) Heitler–London energy. Physically Hii>HccH_{\text{ii}} > H_{\text{cc}} near equilibrium — placing both electrons on one proton costs real energy (electron-electron repulsion on the same center is large, and no compensating overlap term rescues it) — but HciH_{\text{ci}}, the resonance integral coupling covalent and ionic structures, is nonzero because both structures share the same atomic-orbital basis and the Hamiltonian connects them through the electron-transfer terms in the two-electron repulsion operator.

Step 3 — Diagonalize. The secular equation (ignoring the cov–ion overlap for clarity, which is the standard simplified treatment) is

∣Hcc−EHciHciHii−E∣=0,\begin{vmatrix} H_{\text{cc}} - E & H_{\text{ci}} \\ H_{\text{ci}} & H_{\text{ii}} - E \end{vmatrix} = 0,

giving

E±=Hcc+Hii2±(Hii−Hcc2)2+Hci2.E_\pm = \frac{H_{\text{cc}}+H_{\text{ii}}}{2} \pm \sqrt{\left(\frac{H_{\text{ii}}-H_{\text{cc}}}{2}\right)^2 + H_{\text{ci}}^2}.

The lower root E−E_- is the ground-state VB-CI energy.

Step 4 — Show E−<Hcc=EHLE_- < H_{\text{cc}} = E_{\text{HL}} whenever Hci≠0H_{\text{ci}}\neq 0. Since the square root term is strictly greater than ∣Hii−Hcc∣/2|H_{\text{ii}}-H_{\text{cc}}|/2 whenever Hci≠0H_{\text{ci}}\neq 0,

E−=Hcc+Hii2−(Hii−Hcc2)2+Hci2<Hcc+Hii2−Hii−Hcc2=Hcc.E_- = \frac{H_{\text{cc}}+H_{\text{ii}}}{2} - \sqrt{\left(\frac{H_{\text{ii}}-H_{\text{cc}}}{2}\right)^2+H_{\text{ci}}^2} < \frac{H_{\text{cc}}+H_{\text{ii}}}{2} - \frac{H_{\text{ii}}-H_{\text{cc}}}{2} = H_{\text{cc}}.

So mixing in any amount of ionic character, however small HciH_{\text{ci}} is, strictly lowers the energy below the pure covalent Heitler–London value — this is the algebraic reason ionic-covalent resonance always stabilizes a bond, never destabilizes it, at the variational level.

Step 5 — Extract the ground-state mixing coefficient. The optimal ground-state wavefunction is Ψ−=cos⁡θ Ψcov+sin⁡θ Ψion\Psi_- = \cos\theta\,\Psi_{\text{cov}} + \sin\theta\,\Psi_{\text{ion}} with

tan⁡2θ=2HciHcc−Hii.\tan 2\theta = \frac{2H_{\text{ci}}}{H_{\text{cc}}-H_{\text{ii}}}.

Because Hii>HccH_{\text{ii}} > H_{\text{cc}} near ReR_e, this mixing angle is small and positive, meaning the exact wavefunction is mostly covalent with a modest ionic admixture — quantitatively consistent with the qualitative resonance picture from Covalent and Ionic Contributions to the Bond, now derived rather than merely asserted. As R→∞R\to\infty, Hci→0H_{\text{ci}}\to 0 exponentially (it depends on orbital overlap) while Hii−HccH_{\text{ii}}-H_{\text{cc}} approaches a finite positive constant, so θ→0\theta\to 0: ionic character correctly vanishes at dissociation.

Worked examples

Example 1 — Foundational: confirming the 50:50 MO ratio numerically at a specific, non-symmetric overlap. Take a deliberately non-round overlap value, S=0.4637S = 0.4637 (a realistic value near the H₂ equilibrium distance for Slater 1s orbitals with an effective exponent), rather than a convenient round number, to make sure the 50:50 result isn't an artifact of a special choice. The normalization constant is

N2=12(1+S)=12(1.4637)=12.9274=0.34160.N^2 = \frac{1}{2(1+S)} = \frac{1}{2(1.4637)} = \frac{1}{2.9274} = 0.34160.

Expanding ΨMO=N2[χa(1)χa(2)+χb(1)χb(2)+χa(1)χb(2)+χb(1)χa(2)]\Psi_{\text{MO}} = N^2[\chi_a(1)\chi_a(2)+\chi_b(1)\chi_b(2)+\chi_a(1)\chi_b(2)+\chi_b(1)\chi_a(2)], each of the four bracketed terms carries coefficient N2=0.34160N^2 = 0.34160 exactly. Grouping,

covalent weight=2N2=0.68320,ionic weight=2N2=0.68320.\text{covalent weight} = 2N^2 = 0.68320, \qquad \text{ionic weight} = 2N^2 = 0.68320.

The ratio is

ioniccovalent=0.683200.68320=1.0000\frac{\text{ionic}}{\text{covalent}} = \frac{0.68320}{0.68320} = 1.0000

regardless of the specific numerical value of SS chosen — confirming algebraically that the 1:1 covalent–ionic split of simple MO theory does not depend on distance, basis exponent, or any other parameter; it is a structural feature of building the wavefunction from one delocalized product orbital.

Limiting check: setting S→0S\to 0 (the large-RR limit) gives N2→1/2N^2 \to 1/2, covalent weight →1\to 1, ionic weight →1\to 1, ratio still exactly 1 — the pathology persists undiminished all the way to infinite separation, which is precisely the dissociation catastrophe stated in the overview.

Example 2 — Applied: the VB-CI stabilization energy for asymmetric, off-round trial matrix elements. Suppose (units of eV, chosen to be non-symmetric and non-round so the formula is genuinely exercised) that at some intermediate H–H distance the diagonal and off-diagonal VB matrix elements are

Hcc=−31.7 eV,Hii=−19.4 eV,Hci=−4.3 eV.H_{\text{cc}} = -31.7\ \text{eV}, \qquad H_{\text{ii}} = -19.4\ \text{eV}, \qquad H_{\text{ci}} = -4.3\ \text{eV}.

(These are illustrative numbers of the right order of magnitude and sign pattern — Hii>HccH_{\text{ii}} > H_{\text{cc}} because the ionic structure is higher in energy — used to exercise the formula, not literature-tabulated H₂ integrals.) Compute the average and half-difference:

Hcc+Hii2=−31.7+(−19.4)2=−51.12=−25.55 eV,\frac{H_{\text{cc}}+H_{\text{ii}}}{2} = \frac{-31.7 + (-19.4)}{2} = \frac{-51.1}{2} = -25.55\ \text{eV},
Hii−Hcc2=−19.4−(−31.7)2=12.32=6.15 eV.\frac{H_{\text{ii}}-H_{\text{cc}}}{2} = \frac{-19.4-(-31.7)}{2} = \frac{12.3}{2} = 6.15\ \text{eV}.

The discriminant:

(6.15)2+(−4.3)2=37.82+18.49=56.31=7.504 eV.\sqrt{(6.15)^2 + (-4.3)^2} = \sqrt{37.82 + 18.49} = \sqrt{56.31} = 7.504\ \text{eV}.

Ground-state VB-CI energy:

E−=−25.55−7.504=−33.05 eV.E_- = -25.55 - 7.504 = -33.05\ \text{eV}.

Compare to the pure covalent (simple VB) value Hcc=−31.7H_{\text{cc}} = -31.7 eV: the ionic admixture lowers the energy by

ΔE=E−−Hcc=−33.05−(−31.7)=−1.35 eV,\Delta E = E_- - H_{\text{cc}} = -33.05 - (-31.7) = -1.35\ \text{eV},

a genuine, computable stabilization purely from allowing ionic resonance — confirming Step 4 of the second derivation (E−<HccE_- < H_{\text{cc}}) with concrete asymmetric numbers. The mixing angle:

tan⁡2θ=2(−4.3)−31.7−(−19.4)=−8.6−12.3=0.6992  ⟹  2θ=34.98∘  ⟹  θ=17.49∘.\tan 2\theta = \frac{2(-4.3)}{-31.7-(-19.4)} = \frac{-8.6}{-12.3} = 0.6992 \implies 2\theta = 34.98^\circ \implies \theta = 17.49^\circ.

So cos⁡2θ=0.9098\cos^2\theta = 0.9098 and sin⁡2θ=0.0902\sin^2\theta = 0.0902: the exact-in-this-basis ground state is about 91.0% covalent, 9.0% ionic — a small but non-negligible ionic weight, exactly the qualitative pattern chemists invoke when they say H₂ is "mostly covalent with a little ionic resonance."

Limiting check: if Hci→0H_{\text{ci}} \to 0 (structures decoupled — e.g., orbitals on infinitely separated atoms), then tan⁡2θ→0\tan 2\theta \to 0, so θ→0\theta \to 0, E−→HccE_- \to H_{\text{cc}}: the ionic admixture vanishes and VB-CI collapses back exactly to simple Heitler–London, as it must at dissociation.

Example 3 — Exam/competition level: showing MO-CI reproduces the VB-CI ground state exactly (same numbers, both routes). This example demonstrates the central claim of the article — that full CI on the MO side and full CI on the VB side give the same wavefunction — using the same non-symmetric matrix elements framework, now built from the MO configurations (σg)2(\sigma_g)^2 and (σu)2(\sigma_u)^2. The two-configuration MO wavefunction is

ΨMO-CI=c1(σg)2−c2(σu)2.\Psi_{\text{MO-CI}} = c_1 (\sigma_g)^2 - c_2(\sigma_u)^2.

Expand each configuration in atomic orbitals. From the earlier derivation,

(σg)2∝χaχa+χbχb+χaχb+χbχa(equal covalent, ionic weight 1:1).(\sigma_g)^2 \propto \chi_a\chi_a+\chi_b\chi_b+\chi_a\chi_b+\chi_b\chi_a \quad(\text{equal covalent, ionic weight 1:1}).

By the same method with σu=M(χa−χb)\sigma_u = M(\chi_a-\chi_b), M2=1/[2(1−S)]M^2 = 1/[2(1-S)],

(σu)2∝χaχa+χbχb−χaχb−χbχa(ionic weight +1, covalent weight −1).(\sigma_u)^2 \propto \chi_a\chi_a + \chi_b\chi_b - \chi_a\chi_b - \chi_b\chi_a \quad(\text{ionic weight }+1,\text{ covalent weight }-1).

So the combination, written schematically in un-normalized covalent/ionic amplitudes (dropping the constants N2,M2N^2,M^2 for the moment and tracking only relative signs and weights):

ΨMO-CI∝(c1N2+c2M2) [χaχa+χbχb]+(c1N2−c2M2) [χaχb+χbχa].\Psi_{\text{MO-CI}} \propto (c_1 N^2 + c_2 M^2)\,[\chi_a\chi_a+\chi_b\chi_b] + (c_1 N^2 - c_2 M^2)\,[\chi_a\chi_b+\chi_b\chi_a].

Matching coefficients to the VB-CI ground state Ψ−∝cos⁡θ Ψcov+sin⁡θ Ψion\Psi_- \propto \cos\theta\,\Psi_{\text{cov}} + \sin\theta\,\Psi_{\text{ion}} from Example 2 (cos⁡θ=0.9539\cos\theta = 0.9539, sin⁡θ=0.3003\sin\theta = 0.3003, taking square roots of the population figures found there), the condition for the two routes to agree is

c1N2+c2M2c1N2−c2M2=sin⁡θcos⁡θ=tan⁡θ=tan⁡(17.49∘)=0.3151.\frac{c_1N^2 + c_2M^2}{c_1N^2 - c_2M^2} = \frac{\sin\theta}{\cos\theta} = \tan\theta = \tan(17.49^\circ) = 0.3151.

Solving for the ratio c2/c1c_2/c_1 (with S=0.4637S=0.4637 as before, so N2=0.3416N^2 = 0.3416 and M2=1/[2(1−0.4637)]=1/1.0726=0.9323M^2 = 1/[2(1-0.4637)] = 1/1.0726 = 0.9323):

c1(0.3416)+c2(0.9323)c1(0.3416)−c2(0.9323)=0.3151.\frac{c_1(0.3416) + c_2(0.9323)}{c_1(0.3416) - c_2(0.9323)} = 0.3151.

Let x=c2/c1x = c_2/c_1. Then

0.3416+0.9323x=0.3151(0.3416−0.9323x)0.3416 + 0.9323x = 0.3151(0.3416 - 0.9323x)
0.3416+0.9323x=0.1076−0.2938x0.3416 + 0.9323x = 0.1076 - 0.2938x
0.9323x+0.2938x=0.1076−0.34160.9323x + 0.2938x = 0.1076 - 0.3416
1.2261x=−0.23401.2261x = -0.2340
x=−0.1908.x = -0.1908.

So a modest admixture of the doubly-excited (σu)2(\sigma_u)^2 configuration, with c2/c1=−0.1908c_2/c_1 = -0.1908 (about 19% of the amplitude of the ground configuration, entering with the sign that removes ionic character since (σu)2(\sigma_u)^2 carries a minus sign on the covalent terms), reproduces exactly the same 91:9 covalent:ionic population that the VB route obtained by explicitly mixing in an ionic structure with tan⁡2θ=0.6992\tan 2\theta = 0.6992. This is the demonstration promised throughout: MO-CI with one excited determinant and VB-CI with one ionic structure are two parametrizations of the identical two-configuration wavefunction.

Limiting check: at R→∞R\to\infty, S→0S\to 0 so N2→M2→1/2N^2\to M^2\to 1/2, and the physical requirement that ionic character vanish entirely forces c1N2=c2M2c_1N^2 = c_2M^2, i.e., c2/c1→1c_2/c_1 \to 1 — the well-known result that full CI on the MO side needs equal weighting of (σg)2(\sigma_g)^2 and (σu)2(\sigma_u)^2 at dissociation to cancel the ionic terms completely, recovering the correct Heitler–London limit from the MO side.

Limiting cases, scope & common traps

RegimeSimple MO predictionSimple VB predictionExact behavior
R→∞R \to \infty50% ionic forever; energy converges to average of neutral-atom and ion-pair energies; wrong, too high100% covalent; correctly two free H atoms100% covalent — VB right, MO wrong
R=ReR = R_e (equilibrium)Overbinds relative to reality is not generally true — actually underbinds less than VB in some treatments but for the wrong reason (spurious ionic stabilization at short range compensates missing correlation)Underbinds — well depth too shallow, ReR_e slightly too long, because ionic resonance stabilization is entirely absentSmall but nonzero ionic admixture (a few percent to ~10–20% population depending on atom pair) gives the correct, deeper well
R→0R \to 0 (united-atom limit)Both orbitals collapse toward a He-like orbital; MO framework remains formally well-behavedVB covalent-only function becomes increasingly poor since ionic terms dominate the true united-atom limit (it is just one nucleus with two electrons — fully "ionic" in the diatomic sense)Ionic weight → 1, covalent weight → 0: exactly opposite limit from R→∞R\to\infty, showing why neither simple theory is uniformly good
Configuration interaction includedMO + one doubly-excited determinant removes excess ionic characterVB + one ionic structure adds missing ionic characterBoth converge to the same two-configuration wavefunction (shown explicitly in Example 3)
Heteronuclear bonds (e.g., HF)Same 1:1 covalent:ionic problem at dissociation, now with badly mismatched atomic energies — even worse breakdownNaturally handles unequal covalent/ionic weighting once ionic structures with the correct polarity are included with a single variational coefficientExact answer strongly ionic-weighted toward F⁻H⁺, which plain covalent-only VB must recover via CI, and plain MO must recover by asymmetrizing the LCAO coefficients (heteronuclear polarization), not by simple CI alone

The chemist behind it

Walter Heitler and Fritz London, working together in Zürich in 1927, produced the calculation that both launched valence bond theory and, in a real sense, launched quantum chemistry as a discipline. Their treatment of H₂ was the first application of the new quantum mechanics to a genuine chemical bond, and it succeeded in explaining, from first principles, why two neutral hydrogen atoms attract each other at all — a question classical physics could not answer since two neutral, spherically symmetric atoms have no obvious source of attraction. Heitler and London showed the attraction was a purely quantum mechanical exchange effect tied to the symmetry requirements of the two-electron wavefunction under spin pairing. The molecular orbital alternative grew up alongside it through the work of Robert Mulliken and Friedrich Hund in the late 1920s and early 1930s, framed around delocalized orbitals built from linear combinations of atomic orbitals and filled according to an aufbau-like scheme. For several decades the two camps were genuinely in competition — Linus Pauling championed and extended VB theory into a general chemical language (hybridization, resonance, electronegativity), while Mulliken's MO approach proved better suited to spectroscopy, symmetry classification, and eventually to computational implementation via Roothaan's equations. The reconciliation described in this article — that both are truncations of the same exact expansion — became fully explicit only once configuration interaction and multiconfigurational self-consistent field methods matured in the mid-20th century, showing that "VB versus MO" was never really a disagreement about the physics, only about which basis to truncate first.

Origins · 1 minWalter Heinrich Heitler and how this was discovered
WH
Walter Heinrich Heitler
1904–1981 · Zürich, 1927, alongside Fritz London

Heitler and London's joint 1927 paper solved the H₂ problem using the then brand-new Schrödinger wavefunction and Pauli's exclusion principle, obtaining a bond energy and equilibrium distance in respectable agreement with experiment using only two atomic 1s orbitals and a symmetric spin-paired combination. Heitler went on to make major contributions to quantum field theory and the theory of radiation, but the H₂ calculation remained the foundational demonstration that covalent bonding is an exchange phenomenon, not an electrostatic one, and it directly seeded the entire valence bond tradition later systematized by Pauling and Slater.

History
- 1927 — Heitler and London solve H₂ with a purely covalent, spin-paired two-electron wavefunction, founding valence bond theory.
- 1928–1932 — Mulliken, Hund, and Lennard-Jones develop the molecular orbital / LCAO framework as a competing description of diatomic bonding.
- 1931–1933 — Pauling and Slater extend VB theory with hybridization and resonance, making it the dominant language of structural organic chemistry.
- 1949 — Weinbaum and later Coulson–Fischer show that adding ionic structures to the Heitler–London function, or equivalently CI in the MO picture, closes most of the gap to the exact H₂ energy.
- 1950s onward — Roothaan's matrix formulation of Hartree–Fock and the rise of configuration-interaction and multiconfigurational methods make explicit that VB-CI and MO-CI converge to the same multideterminant wavefunction.
Is valence bond theory "wrong" and molecular orbital theory "right"?

Neither is simply right or wrong; both are truncations of the same exact wavefunction expansion, and each fails in a different regime. Simple VB theory (Heitler–London) is exact in spirit at infinite separation but misses ionic stabilization near equilibrium. Simple MO theory keeps a fixed, geometry-independent 50:50 covalent:ionic ratio that is badly wrong at large separation but happens to partially compensate for missing electron correlation near equilibrium in some systems. Once configuration interaction is added on either side, the two frameworks converge to the identical multi-configurational wavefunction — the "disagreement" is really a disagreement about which single configuration to start counting from.

Why does restricted Hartree-Fock give a nonzero binding energy for H2 even at 20 angstroms of separation?

Because the restricted single-determinant wavefunction forces both electrons into the same spatial bonding orbital σg\sigma_g, which is delocalized over both nuclei by construction. Squaring this orbital always produces equal covalent and ionic weight, so the RHF wavefunction at any separation still describes a coherent superposition of neutral atoms and an ion pair (H⁺H⁻/H⁻H⁺), which costs real energy relative to two genuinely independent atoms. The resulting curve flattens out at an energy above the true dissociation limit, producing a spurious energy gap that is a textbook symptom of static (nondynamic) correlation error, fixable by unrestricted Hartree-Fock (which breaks spin symmetry to localize the electrons) or by explicit configuration interaction.

How much ionic character does real H2 actually have at its equilibrium bond length?

Accurate multi-configurational calculations put the ionic weight in the ground-state H₂ wavefunction at roughly 5-15% of the total probability, depending on the basis set and the precise definition of "weight" used, with covalent (Heitler–London-type) character dominating at 85-95%. This is broadly consistent with the illustrative 9% ionic figure obtained algebraically in the worked example here from representative matrix elements. The key qualitative point — small but nonzero ionic admixture, vanishing smoothly as the bond stretches — is robust across methods, even though the precise percentage is basis- and method-dependent.

Does this covalent/ionic mixing argument generalize beyond H2?

Yes, and it becomes even more important for heteronuclear bonds. For a bond like H–F, the two ionic structures (H⁺F⁻ and H⁻F⁺) are no longer degenerate — H⁺F⁻ is far lower in energy because fluorine holds extra electron density much more favorably — so the exact wavefunction is strongly weighted toward that one ionic structure, consistent with a large bond dipole. Simple MO theory built from equal-coefficient LCAO orbitals gets this badly wrong for the same 50:50 reason as H₂; the fix on the MO side is to let the bonding orbital have unequal atomic coefficients (polarization), while the fix on the VB side is to let the ionic structure's CI coefficient be large and asymmetric between the two possible polarities.

Why is the doubly-excited configuration (σᵤ)² the key missing piece on the MO side rather than some other excitation?

Because (σu)2(\sigma_u)^2 is the only doubly-excited configuration of the correct spatial and spin symmetry (totally symmetric, singlet) that can mix with the ground configuration (σg)2(\sigma_g)^2 under the H₂ point group, by the same symmetry selection rules used throughout configuration interaction theory. Its atomic-orbital expansion carries covalent and ionic terms with opposite relative sign compared to (σg)2(\sigma_g)^2, so adding a controlled amount of −(σu)2-(\sigma_u)^2 selectively cancels excess ionic character without disturbing the covalent terms — precisely the surgical correction the dissociation limit requires, and precisely why no other single excited configuration would do the job as efficiently.

Is Heitler-London theory ever used directly in modern calculations, or is it purely historical?

It is far from purely historical. Modern spin-coupled and generalized valence bond (GVB) methods are direct descendants: they allow each electron to occupy its own optimized, typically non-orthogonal orbital, recovering much of the correlation energy that single-determinant MO theory misses, without needing large CI expansions. These methods are used today specifically in regimes where bonds are stretched, broken, or forming — reaction path calculations, diradical characterization, and photodissociation dynamics — precisely the regime where the simple MO dissociation catastrophe analyzed in this article would otherwise cause serious qualitative errors.

How does this comparison connect to resonance structures drawn in organic chemistry?

Directly — the ionic and covalent VB structures for H₂ are the simplest possible example of resonance: two legitimate Lewis-type structures (one covalent, two degenerate ionic) that are mixed variationally rather than treated as separate interconverting species. The mixing coefficient derived from the 2×2 secular equation is the quantum mechanical version of "how much a resonance structure contributes," and the strict energy-lowering result proven in the second derivation (mixing always lowers the energy relative to either pure structure alone) is the rigorous justification for why chemists say resonance is always stabilizing, never destabilizing, provided the mixed structures have appreciable coupling.

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