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Exercises · 4.34

Q.Write the important conditions required for the linear combination of atomic orbitals to form molecular orbitals.

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The formation of molecular orbitals via LCAO requires three conditions: the combining atomic orbitals must have comparable energies, they must have the same symmetry about the internuclear axis, and they must overlap significantly. These ensure effective constructive and destructive interference, yielding bonding and antibonding MOs.

The Core Idea: Why Conditions Matter

When two atomic orbitals combine to form molecular orbitals, we are essentially asking: can these wavefunctions interfere constructively and destructively in a stable, meaningful way? Just like two waves in a pond — if they have different frequencies or meet at an angle, they won't produce a clean standing wave. The same logic governs orbital mixing.

The Linear Combination of Atomic Orbitals (LCAO) method is built on the idea that the molecular orbital wavefunction ψMO\psi_{MO} is a linear combination:

ψMO=c1ϕA+c2ϕB\psi_{MO} = c_1 \phi_A + c_2 \phi_B

where ϕA\phi_A and ϕB\phi_B are atomic orbitals on two atoms. For this combination to yield physically meaningful bonding (ψ+\psi_+) and antibonding (ψ−\psi_-) orbitals, three conditions must be satisfied.


The Three Essential Conditions

1. Comparable Energies of the Combining Orbitals

The atomic orbitals must have similar energies. Why? Because the extent of mixing depends on the energy difference ΔE=∣EA−EB∣\Delta E = |E_A - E_B|. If the energies are too different, the resulting MO will be almost identical to the lower-energy AO, with negligible contribution from the higher-energy one — no real bonding occurs.

The mixing coefficient ratio is approximately:

c2c1≈HABEA−EB\frac{c_2}{c_1} \approx \frac{H_{AB}}{E_A - E_B}

where HABH_{AB} is the resonance integral (overlap energy). If ∣EA−EB∣|E_A - E_B| is large, c2c_2 becomes tiny — the orbitals barely mix.

Example: In HF, the 1s orbital of H (−13.6-13.6 eV) and the 2pz_z orbital of F (−18.6-18.6 eV) have a moderate energy difference, so they mix to form a polar bond. But the 1s of H and the 2s of F (−40.2-40.2 eV) are too far apart — they do not combine.

Watch out

A common mistake is to think that any two orbitals with the same principal quantum number will combine. They won't if their energies differ significantly — e.g., 2s and 2p in the same atom have different energies (in multi-electron atoms), so they do not mix directly across atoms unless symmetry allows.

2. Same Symmetry About the Internuclear Axis

The orbitals must have the same symmetry with respect to rotation around the bond axis. This ensures that the overlap integral ∫ϕAϕB dτ\int \phi_A \phi_B \, d\tau is non-zero.

  • Sigma (σ\sigma) symmetry: Orbitals that are cylindrically symmetric about the bond axis (e.g., s orbitals, pz_z orbitals if the axis is z). They overlap end-to-end.
  • Pi (π\pi) symmetry: Orbitals with one nodal plane containing the bond axis (e.g., px_x, py_y). They overlap side-to-side.
  • Delta (δ\delta) symmetry: Two nodal planes containing the axis (e.g., dxy_{xy}).

Only orbitals of the same symmetry type can combine. A pz_z (sigma) and a px_x (pi) have zero net overlap — their positive and negative lobes cancel.

Tip

Think of it like matching puzzle pieces: a round peg (s orbital) fits into a round hole (end of a pz_z), but not into a slot (side of a px_x). The symmetry must match for constructive interference to be possible.

3. Significant Overlap

Even if energies match and symmetry aligns, the orbitals must physically overlap to a sufficient degree. The overlap integral S=∫ϕAϕB dτS = \int \phi_A \phi_B \, d\tau must be appreciable (typically S>0.1S > 0.1 for meaningful bonding).

Overlap depends on:

  • Distance between nuclei: Too far apart → negligible overlap. …

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