H2+ Molecular Orbitals: Bonding and Antibonding
Two protons and one electron: this is the entire parts list for H₂⁺. Yet from it emerges the whole logic of the covalent bond. Chemists draw a single line between two atoms a thousand times a day. They rarely ask what that line means in terms of a wavefunction. H₂⁺ is where the question can finally be answered exactly enough to trust. Because there is only one electron, there are no electron-electron repulsion terms to approximate away. The Schrödinger equation is not solvable in closed elementary form. But it can be attacked with a controlled, physically transparent trial function. This trial function is built from two atomic orbitals. The big picture is this: a 1s orbital on proton A can combine with a 1s orbital on proton B. Only two independent combinations are possible by symmetry. There is an in-phase (additive) combination and an out-of-phase (subtractive) combination. These are not arbitrary guesses. They are forced on us by a requirement. The two protons in H₂⁺ are indistinguishable nuclei sitting in a symmetric trap. So the electron density must look the same from either proton's point of view. One combination piles up electron density in the internuclear region. This pulls the nuclei together — this is the bonding orbital. The other combination creates a nodal plane exactly between the nuclei. It starves the bonding region of density and pushes the nuclei apart. This is the antibonding orbital. This article builds those two molecular orbitals explicitly from the LCAO Approximation. It works out the normalization constants in terms of the overlap integral. Then it plots and interprets the resulting electron densities. Every step uses the exact framework already established for The Hydrogen Molecule Ion H2+ as the Reference System. That framework has two fixed nuclei, one electron, and a variational trial wavefunction. What is new here is the symmetry argument. It fixes the coefficients of the linear combination before any energy is computed. Also new is the physical reading of the resulting density difference. The redistribution of charge into or out of the bonding region is the origin of chemical bonding itself. By the end, you will be able to write down both H₂⁺ molecular orbitals with correctly normalized coefficients. You will sketch their electron density profiles along the internuclear axis. You will explain, in terms of constructive/destructive interference, why one is bonding and the other antibonding. And you will see exactly where the machinery of overlap, Coulomb, and resonance integrals will enter next. These integrals form the quantitative backbone of the energies.
- H₂⁺ has one electron and two fixed protons; the LCAO trial function combines 1s orbitals on each center: .
- Symmetry (the two nuclei are identical) forces , leaving only two independent combinations: and .
- Normalizing each combination brings in the overlap integral , giving normalization constants and .
- (bonding, ) enhances electron density between the nuclei; (antibonding, ) has a nodal plane there and depletes it.
- The density difference is not simply the sum of atomic densities: cross terms () are entirely responsible for the buildup or depletion between the nuclei.
- Key idea: the bonding/antibonding split comes purely from the sign of the linear combination of atomic orbitals — constructive interference concentrates density in the bond, destructive interference removes it.
Where this lives today
The bonding/antibonding split constructed here for H₂⁺ is the seed of essentially all of modern electronic structure theory. Every quantum chemistry package — from teaching-level Hartree–Fock codes to industrial density functional theory software used in pharmaceutical and materials research — represents molecular electrons in orbitals built as linear combinations of atomic-centered basis functions, and every one of those calculations produces filled bonding orbitals and empty (or higher-lying) antibonding orbitals whose qualitative character is exactly the pattern derived above, just dressed up with many more basis functions and electrons. In spectroscopy, the antibonding orbital of H₂⁺ (and its analogue in H₂) is the destination orbital in photoionization and Rydberg-state experiments, and its nodal structure directly explains why populating it — as happens, for instance, in electron-impact or photon-driven excitation of H₂ — weakens and eventually breaks the bond. This bonding/antibonding logic underlies why π orbitals in carbonyl and alkene chromophores are the acceptor orbitals in UV-visible spectroscopy, why σ orbitals along C–halogen bonds are the targets of nucleophilic backside attack in Sₙ2 reactions (hyperconjugative donation into σ* is a mainstay explanation in physical organic chemistry), and why frontier molecular orbital theory (HOMO/LUMO reasoning in Woodward–Hoffmann rules and Fukui's frontier orbital theory) can predict reactivity trends across huge swaths of organic and organometallic chemistry. Materials scientists use the same bonding/antibonding band-formation logic, scaled up to solids, to explain why partially filled bonding bands give metals their cohesion and why band gaps open when bonding and antibonding combinations split apart in energy — the tight-binding model of solid-state band structure is, structurally, an infinite generalization of exactly the two-orbital problem solved here.
Ask the tutor: How do the Coulomb integral and resonance integral combine with to actually produce the bonding and antibonding energies from these two orbitals?
The physical picture
Picture the electron in H₂⁺ as a wave that must be simultaneously "listened to" by both protons, A and B, held a fixed distance apart along the internuclear axis. Far from either nucleus the electron behaves like a hydrogen 1s electron centered on whichever proton it is near, so a natural trial wavefunction is a linear combination of atomic orbitals,
where and are normalized hydrogen 1s orbitals centered on nucleus A and nucleus B respectively. This is the LCAO Approximation applied to the simplest possible molecule. The key physical constraint is nuclear symmetry. Because both nuclei are protons, swapping labels A ↔ B must leave all observable properties — above all, the electron probability density — unchanged. If , the electron would be found preferentially near one specific proton, which is unphysical for a homonuclear system with no reason to prefer either center. This symmetry argument, not an appeal to energy minimization, is what fixes and leaves only two allowed combinations: the in-phase sum and the out-of-phase difference. The Coulomb and resonance integrals that eventually assign energies to these two combinations belong to the analysis in Coulomb, Resonance, and Overlap Integrals; here the goal is only to build the orbitals and see their shapes. Take the sum first:
At every point in space, the two atomic wavefunctions are added in phase. Directly between the nuclei, both and are still appreciable (each nucleus is close enough that its 1s orbital has not fully decayed), so they add constructively — the resulting amplitude, and hence the probability density , is enhanced relative to what you would get from the two isolated atomic densities added independently. This pile-up of negative charge in the internuclear region is precisely what is needed to screen the mutual repulsion of the two positively charged protons and glue them together: this is the bonding molecular orbital. Now the difference:
Along the perpendicular bisecting plane of the bond — the plane equidistant from A and B — and are numerically equal, so their difference vanishes identically. This defines an exact nodal plane perpendicular to the bond axis at the midpoint. Approaching this plane from either side, the wavefunction changes sign, and the probability density is driven to zero exactly at the midpoint and suppressed throughout the internuclear region. With the negative charge evacuated from between the nuclei, the bare protons repel each other with nothing to shield them: this is the antibonding molecular orbital.
The reason both combinations require careful normalization rather than a naive prefactor is that and are not orthogonal — they overlap in space, and this overlap is quantified by the overlap integral
depends on the internuclear distance : at the two orbitals coincide and ; at they no longer overlap and . At typical bonding distances in H₂⁺ ( pm), is a substantial positive fraction, of order – depending on how it's evaluated — this nonzero overlap is exactly what forces the normalization constants for and to differ from each other and from the naive guess .
The upshot: the two LCAO combinations of a single pair of 1s orbitals already reproduce the entire qualitative content of the covalent bond — an attractive, density-enhancing combination and a repulsive, density-depleting combination — with no need to invoke electron-electron interactions at all, since H₂⁺ has only one electron. The energetics that turn "more density between the nuclei" into "lower total energy" are worked out quantitatively once the Coulomb integral and resonance integral are introduced; the symmetry labels and used loosely above are made precise in the treatment of Sigma and Pi Molecular Orbitals and Symmetry Labels.
The core ideas
The trial wavefunction, forced by A↔B symmetry to have , reduces to exactly two possibilities:
where:
- is the symmetric (bonding) combination, the antisymmetric (antibonding) combination
- are normalized 1s hydrogenic orbitals centered on nuclei A and B
- are real normalization constants (assuming real, non-negative , so )
Reading: there are only two ways to combine one orbital from each of two equivalent centers while keeping symmetric under nuclear exchange — add them, or subtract them. Normalization requires , which brings in the overlap integral explicitly:
where:
- is the (dimensionless) overlap integral, a function of
- the sign in goes with , the sign in goes with
Reading: because and overlap ( for finite), the bonding combination needs a smaller normalization constant than (the two lobes reinforce, so less amplitude per orbital is needed to reach total probability 1), while the antibonding combination needs a larger one (the lobes partially cancel, so more amplitude per orbital is needed). The electron density built from each MO is
where:
- and are the densities the electron would have if localized purely on A or purely on B
- the cross term is the interference term, present only because the electron is genuinely delocalized over both centers
Reading: without the cross term, would just be an average of two atomic densities — no chemistry would happen. The entire physical content of "bonding" versus "antibonding" lives in the sign and magnitude of this cross term.
Goal. Find such that is normalized, given that are each individually normalized and have overlap .
Step 1 — write the normalization integral. Demand
Step 2 — expand the square. Since are real functions,
Step 3 — integrate term by term. Using (normalized atomic orbital), , and by definition of the overlap integral,
Step 4 — solve for . Substituting back,
Step 5 — repeat with a minus sign for . The only change is the cross term flips sign, , giving and hence
Note that since for any finite bonding distance, always: the antibonding orbital needs a larger prefactor precisely because subtraction partially cancels amplitude, and more of it must be "put back" to reach unit total probability.
Go deeper · Derivation B · 1 minDensity difference between bonding and antibonding orbitals — where the charge goes
Goal. Show explicitly that builds up density between the nuclei relative to the free-atom average, while removes it, and quantify the redistribution.
Step 1 — define the "no-interference" reference density. If the electron were a 50/50 classical mixture of "on A" and "on B" with no quantum interference, the density would simply be the average
This is what you'd get by ignoring the cross term and normalizing with regardless of sign.
Step 2 — write the true bonding density using the correct . From the core equations,
Split the numerator to isolate the reference density:
Step 3 — compare to the reference at the midpoint. At the bond midpoint, by symmetry , so and the cross term is also . Then
Since makes whenever , the bonding density at the midpoint exceeds the naive average — genuine enhancement, not just relabeling.
Step 4 — do the same for the antibonding density.
and at the midpoint, where , the bracket vanishes identically:
This confirms the node found geometrically: the antibonding density is exactly zero at the midpoint, for any value of , not approximately zero.
Step 5 — interpret the normalization denominators physically. The factor in is smaller than would be, meaning normalization alone tends to suppress the bonding density everywhere except where the cross term compensates; but because the cross term is positive everywhere between the nuclei for , the net effect is still a pile-up in the bonding region and (by overall normalization to a fixed total of 1 electron) a slight depletion in the outer, non-bonding regions. The reverse happens for : density is pulled away from the middle and pushed to the outer lobes and beyond.
Worked examples
Example 1 — Foundational: normalization constants at the equilibrium-like separation of H₂⁺. Take (close to the true equilibrium bond length of H₂⁺, pm) and use the standard exact overlap integral for two 1s Slater orbitals with effective charge ,
with in units of . Substituting :
Since ,
Now the normalization constants:
Sanity check on the asymmetry: — the antibonding orbital's prefactor is nearly double the bonding one's at this fairly short distance, exactly as expected since is large enough here that is small. As , and both constants converge to the textbook value , recovering the naive normalization for non-overlapping, effectively orthogonal orbitals — a useful limiting-case check.
Example 2 — Applied: electron density at the bond midpoint versus far outside the molecule. Continue with and locate the midpoint, a distance from each nucleus. For a hydrogenic 1s orbital (, in atomic units),
At the midpoint, . Bonding density at the midpoint (using Step 3 of the second derivation):
Antibonding density at the same point: exactly , as shown generally above. Now compare to a point outside the bond, say beyond nucleus B (so from B, from A) — far into the antibonding-favored region. There, and . The cross term is tiny compared to , so both densities are dominated by the single-atom tail:
Outside the bond, the antibonding density is now larger than the bonding density (unlike at the midpoint) — the antibonding orbital does not destroy density everywhere, it specifically redistributes it away from the internuclear region and into the outer lobes, consistent with the qualitative picture and confirming the redistribution is a shift, not a uniform suppression.
Example 3 — Exam/competition level: how much extra charge sits between the nuclei for , and the total-probability bookkeeping. A common exam question asks: integrate over all space and show it equals 1, then quantify the "overlap population" — the fraction of total probability that is attributable purely to the cross term. From the second derivation,
confirming normalization holds globally, as it must by construction — the local enhancement at the midpoint found in Example 2 is compensated by a slight depletion elsewhere so the grand total is unchanged. Now define the "overlap population" as the contribution of the cross term alone to the total probability:
At with :
So at this separation, roughly 37% of the total electron probability in the bonding MO is carried by the cross (interference) term rather than by the "atomic" and terms individually — a striking quantitative statement that the covalent bond in H₂⁺ is not a minor perturbation on two separate atoms but is dominated by genuine quantum delocalization at this distance. For the antibonding orbital the analogous quantity is negative,
whose magnitude exceeding 1 in size (though the total must still integrate to once combined with the positive atomic terms) reflects how strongly antibonding character concentrates the deficit right where and overlap most, requiring a correspondingly large compensating normalization . As a limiting-case check, letting (large ) gives for both orbitals — at large separations there is no interference left to speak of, and each MO reduces to an equal, incoherent mixture of the two atomic densities.
Limiting cases, scope & common traps
| Regime / check | What happens | Why |
|---|---|---|
| ; ; | Orbitals stop overlapping; cross term vanishes; MOs reduce to an incoherent 50/50 mix — no bonding, no antibonding distinction survives | |
| ; ; (divergent, unphysical) | United-atom limit is not correctly described by this simple two-1s LCAO; 's normalization blowing up signals the basis set is breaking down, not a real physical divergence | |
| At the bond midpoint | enhanced; exactly | Symmetric vs antisymmetric combination of equal atomic amplitudes |
| Far outside the bond (outer lobes) | can exceed | Antibonding redistributes density outward, it does not uniformly destroy it |
| This is a one-electron system | No electron-electron repulsion terms appear anywhere | H₂⁺ is exactly solvable in principle (in prolate spheroidal coordinates); LCAO here is a variational approximation, not a many-body mean-field trick |
| Real H₂⁺ ground state vs LCAO | LCAO gives , true value ; binding energy underestimated by roughly 40% | Simple LCAO with undistorted 1s orbitals omits polarization/contraction of the atomic orbitals in the molecular field |
The chemist behind it
The LCAO treatment of H₂⁺ traces to the earliest days of applying the new quantum mechanics to chemical bonding, in the years immediately following Schrödinger's 1926 papers. The molecular-orbital viewpoint — building wavefunctions delocalized over the whole molecule from atomic building blocks — is inseparable from the names Friedrich Hund and Robert Mulliken, who independently developed the molecular orbital framework as an alternative to the valence-bond picture that Heitler and London had pioneered for H₂. Mulliken in particular pushed hard for the view that electrons in molecules occupy orbitals extending over all the nuclei, exactly the picture realized concretely by and for H₂⁺, and he later systematized the symmetry notation (, , etc.) that chemists still use today.
Origins · 1 minRobert S. Mulliken and how this was discovered
Mulliken trained originally as a chemist at MIT and Chicago, working on isotope separation before turning, in the late 1920s, to the emerging quantum theory of molecular structure. Alongside Hund, he championed the molecular orbital approach — describing electrons with orbitals delocalized over an entire molecule, built by combining atomic orbitals — as opposed to the localized bond-pair picture of valence bond theory. His painstaking analysis of diatomic spectra let him assign electron configurations, symmetry labels, and bonding/antibonding character to molecular orbitals with a rigor that made MO theory usable, not just conceptually appealing. He was awarded the Nobel Prize in Chemistry in 1966 "for his fundamental work concerning chemical bonds and the electronic structure of molecules by the molecular orbital method." The , , , , and asterisk (antibonding) notation used throughout molecular orbital theory is largely his legacy.
Why does H2+ only have two possible LCAO combinations instead of many?
Because there are only two atomic orbitals in the minimal basis — one 1s orbital on each proton — and only two linearly independent combinations can be built from two functions. Symmetry further restricts these two combinations to have equal-magnitude coefficients, since the two nuclei are chemically and physically identical. That leaves exactly the symmetric sum and the antisymmetric difference , normalized separately because the overlap integral enters with opposite sign in each case. Adding more atomic orbitals per center (2p, 2s, etc.) or using more nuclei generates more combinations, but for the minimal one-orbital-per-atom treatment of H₂⁺, two is the whole story.
Why is the normalization constant different for the bonding and antibonding orbitals?
Normalization forces , and expanding produces a cross term whose integral is . For the bonding combination this adds constructively to the two unit atomic-orbital integrals, giving a normalization integral of ; for the antibonding combination it subtracts, giving . Since these two raw integrals differ, the constants needed to rescale each combination back down to total probability 1 must also differ: is smaller than whenever , which is always true at finite bonding distances.
Does the bonding orbital just look like two separate atomic 1s clouds added together?
Not quite — the naive sum of two independent atomic 1s densities would be , with no cross term at all. The true bonding density contains an extra term, , scaled by the normalization , and this cross term is what physically represents quantum mechanical interference between the two atomic wavefunctions. At the bond midpoint this cross term equals the average atomic term itself, so the true density there is roughly double what a naive incoherent mixture would predict — the enhancement is a genuinely quantum effect, not just bookkeeping.
Is the antibonding orbital ever occupied in real molecules, and what happens if it is?
Yes — in H₂⁺ itself the antibonding orbital is simply empty in the ground state (the single electron occupies ), but in excited states, in molecular ions with more electrons, or under photoexcitation, antibonding orbitals can become populated. Filling an antibonding orbital removes stabilizing bonding density from between the nuclei and typically weakens or breaks the bond, which is exactly the mechanism behind photodissociation of H₂ upon excitation to a state with significant character, and behind bond weakening whenever electrons are added to antibonding orbitals in a Walsh-diagram or molecular-orbital-diagram analysis of a bigger molecule.
How does this LCAO treatment compare to the exact solution of H2+?
H₂⁺ can be solved essentially exactly by separating the Schrödinger equation in prolate spheroidal coordinates, since it is a one-electron, two-center Coulomb problem; this gives numerically precise energies and wavefunctions used as the benchmark. The simple two-1s LCAO trial function captures the qualitative bonding/antibonding split correctly and gives a real, if less accurate, bound ground state (equilibrium separation near 2.5 a0 versus the true 2.00 a0, and a binding energy too small by roughly 40%). The gap between LCAO and exact results is closed by allowing the atomic orbitals themselves to distort — for instance letting the effective nuclear charge or orbital exponent vary — which is the natural next refinement built on top of the rigid-1s LCAO picture developed here.
Why does the antibonding orbital have a node exactly at the midpoint rather than somewhere else?
The node's location is fixed by symmetry, not by any energetic optimization. On the plane perpendicular to the bond axis and passing through its midpoint, every point is equidistant from nucleus A and nucleus B, so and , which depend only on distance from their respective nucleus, are numerically identical there. Subtracting two identical numbers gives exactly zero, for any bond length R and for any orbital exponent used to define and . This is why the antibonding node is exact and geometry-independent within the model, unlike, say, the radial nodes of atomic orbitals, whose positions depend on quantum numbers and effective charge.
What role does the overlap integral S play beyond just normalization?
Beyond fixing the normalization constants derived here, S also enters directly into the energy expressions for the bonding and antibonding states through the secular equations of the variational method, where it appears in the denominator alongside the Coulomb integral and resonance integral . A larger S generally signals stronger orbital interaction and, other things equal, a larger bonding stabilization and antibonding destabilization — this quantitative energy story, built directly on the orbitals constructed here, is the natural next topic once the shapes of and are established.