Lecture B8 Molecular Orbital Theory, Part 3. Moving to the Suburbs

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Lecture B8 Molecular Orbital Theory, Part 3 Moving to the Suburbs

Molecular Orbital Theory - LCAO-MO Robert S. Mulliken realized that a Linear Combination of Atomic Orbitals (LCAO) could be used to make a set of new Molecular Orbitals (MO). The energies of these new molecular orbitals could be calculated and then filled with valence electrons. Robert S. Mulliken 1896-1986 Mulliken received the 1966 Nobel Prize for his work.

MO energies come from Quantum Mechanics, of course! WHEN we solve the Schrödinger equation, we always obtain two things: 1. a set of eigenstates. 2. a set of eigenstate energies. If you are interested, please look up the "Hartree-Fock Method" and "Slater Determinants." D. R. Hartree 1897-1958 V. A. Fock 1898-1974 J. C. Slater 1900-1976

A final homonuclear example: C2 - Number of valence electrons?

For homonuclear diatomic molecules, you should be able to predict: 1. Electron Configuration II. Bond Order III. Paramagnetic or Diamagnetic IV. Number of electrons in the HOMO V. Estimate (set limits on) the IP of the molecule

A final homonuclear example: C2-8 electrons - state ordering same as N2

A final example: C2-8 electrons - state ordering same as N2 We predict: bond order = 1/2(6-2) = 2 C2 is diamagnetic IP is greater than 11.26 ev electron configuration is: σ2s 2 σ*2s 2 π2p 4 Four electrons in the HOMO

By the way, does C2 exist?

By the way, does C2 exist? Yes it does -- in outer space!

Here's some of the "Mulliken bands" of interstellar C2

But C2 also exists inside your bunsen burner: Swan bands are a characteristic of the spectra of carbon stars, comets and of burning hydrocarbon fuels. They are named for the Scottish physicist William Swan who first studied the spectral analysis of carbon C2 in 1856. Identified as C2 by J. D. Shea in 1927: Phys. Rev. 30 (1927) 825 843.

The Swan bands are the blue emission lines in a Bunsen burner. Spectrum of a blue flame from a pocket butane torch clearly showing non-continuum spectral emission. Spectrum taken by me using an Ocean Optics HR2000 spectrometer.

The fool-proof procedure for constructing energy correlation diagrams for heteronuclear diatomics: 0. Draw the vacuum level. Heteronuclear Diatomics 1. Put the atomic orbitals for each bonding partner in your diagram. Position the HOAO based upon the IP of the atom. 2. Draw in the energy levels for your MOs. You ll need one for each atomic state. 3. Fill them with electrons. Make sure to follow Aufbau and Hund s rules. Easy as Toast!

A example: Carbon Monoxide (CO) 0 C O vacuum level 11.3 ev 13.6 ev potential energy, ev 2p 2s 2p 2s

An example: Carbon Monoxide (CO) potential energy, ev 0 C O 2p 2s 2p 2s vacuum level sigma orbitals 11.3 ev 13.6 ev σ2p * σ2p σ2s * σ2s

An example: Carbon Monoxide (CO) potential energy, ev 0 C O 2p 2s 2p 2s vacuum level pi orbitals 11.3 ev 13.6 ev σ2p * π2p * σ2p π2p σ2s * σ2s

An example: Carbon Monoxide (CO) - 10 valence electrons C O 0 vacuum level potential energy, ev 2p 2s σ2p * π2p * σ2p π2p σ2s * 2p 2s 13.6 ev σ2s

So heteronuclear diatomic molecules are a bit more complicated, but still we can make predictions: For CO: bond order = 3.0 CO is diamagnetic IP is greater than 13.6 ev (Actual is 14.0 ev) Electron configuration is: σ2s 2 σ*2s 2 π2p 4 σ2p 2 Two electrons in the HOMO

Some additional facts about CO: Bond Length: 112.8 pm Dipole Moment: 0.112D δ+ δ- : C O: Opposite of Lewis Dot Structure Formal Charge!

Mulliken Population Analysis Mulliken outlined a systematic method for obtaining quantitative information from the LCAO-MOs in terms of atomic populations (net and gross), overlap populations, promotion and the total charge on each atom. In 1955. Robert S. Mulliken 1896-1986

Mulliken Population Analysis For a diatomic molecule AB, consider a molecular orbital ϕmo that is made from a linear combination of two atomic orbitals, one from atom A, and one from atom B.

Mulliken Population Analysis For a diatomic molecule AB, consider a molecular orbital ϕmo that is made from a linear combination of two atomic orbitals, one from atom A, and one from atom B. The molecular orbital and both of the atomic orbitals are all normalized to a probability of one over all space:

Mulliken Population Analysis The Born Interpretation states that Φ 2 is the probability density for the molecular orbital:

Mulliken Population Analysis The Born Interpretation states that Φ 2 is the probability density for the molecular orbital: If we integrate this equation to get the probability, we end up with three terms:

Mulliken Population Analysis If we integrate this equation to get the probability, we end up with three terms: one one one where SAB is called the overlap integral:

Mulliken Population Analysis If there are N electrons in the molecular orbital Φ, then:

Mulliken Population Analysis If there are N electrons in the molecular orbital Φ, then: Mulliken called NcA 2 the net atomic population on atom A and NcB 2 the net atomic population on atom B.

Mulliken Population Analysis If there are N electrons in the molecular orbital Φ, then: Mulliken called NcA 2 the net atomic population on atom A and NcB 2 the net atomic population on atom B. Mulliken called 2NcAcBSAB the overlap population, and used it as a measure of the amount of bonding in the orbital.

Mulliken Population Analysis If there are N electrons in the molecular orbital Φ, then: Mulliken called NcA 2 the net atomic population on atom A and NcB 2 the net atomic population on atom B. Mulliken called 2NcAcBSAB the overlap population, and used it as a measure of the amount of bonding in the orbital. "These three sub-populations may be likened to those of two cities and a (joint) suburb which lies between them." R. S. Mulliken

Mulliken Population Analysis Gross Atomic Populations: Mulliken also created gross atomic populations in which the charge in an orbital was assigned to either atom A or atom B. The overlap population was equally divided between the two atoms. N(A) N(B)

Gross Atomic Populations: Mulliken Population Analysis Gross Atomic Charges: Mulliken also created gross atomic charges by subtracting the gross atomic populations from the number of electrons originally in the atomic orbitals: N0(A) and N0(B).

Mulliken Population Analysis All of the equations I have used were for one MO: Mulliken generalized these equations to ALL of the MOs in a molecule. See the Handouts Section of the Chem H2A web page to download his 1955 paper. R. S. Mulliken, J. Chem. Phys.10 1833-1840 (1955).

Mulliken did an example molecule: Carbon Monoxide! He used the LCAO-MOs from someone else (Sahni): Nomenclature: Mulliken just named the orbitals nσ or nπ: Ours: σ1s 2 σ*1s 2 σ2s 2 σ*2s 2 π2p 4 σ2p 2 His: 1σ 2 2σ 2 3σ 2 4σ 2 1π 2 5σ 2

Mulliken did an example molecule: Carbon Monoxide! Here are the highest energy occupied MOs: 5σ = 0.187ΨO(2s) - 0.189ΨO(2pσ) + 0.615ΨC(2s) - 0.763ΨC(2pσ) 1π = 0.8145ΨO(2pπ) + 0.4162ΨC(2pπ) The sigma orbitals are all linear combinations of four orbitals; the pi orbitals of two.

An example: CO Using the atomic populations, we find: On the Carbon(1s 2 2s 2 2p 2 ): 1s 2.00 2s 1.49 2p 2.42 On the Oxygen(1s 2 2s 2 2p 4 ): 1s 2.00 2s 1.86 2p 4.23 Pauling was right: sp promotion and hybridization exists!

An example: CO Using the gross atomic populations, we find: On the Carbon(N0 = 4): N(C) = 3.912 On the Oxygen(N0 = 6): N(O) = 6.088 Gross Charge -0.088e +0.088e The CO molecule has a small dipole moment in the direction of Oxygen.

An example: CO Using the gross atomic populations, we find: 1π orbital: N(C) = 1.020; N(O) = 2.980 The pi orbital sits primarily on the Oxygen atom (C + O - polarization).

An example: CO Using the gross atomic populations, we find: 5σ orbital: N(C) = 1.889; N(O) = 0.111 The HOMO sits primarily on the Carbon atom (C - O + polarization). CO forms strong bonds in metal complexes such as Fe(CO)5. Bonding occurs through the Carbon atom end, but uses π* orbitals.

An example: CO Using the overlap populations, we find: 3σ (σ2s) overlap population 4σ (σ*2s) overlap population 1π (π2p) overlap population 5σ (σ2p) overlap population = 0.732 = -0.308 = 0.654 = -0.060 3σ and 1π are bonding orbitals. 4σ and 5σ are nonbonding orbitals!

An example: CO Using the overlap populations, we find: 3σ (σ2s) overlap population 4σ (σ*2s) overlap population 1π (π2p) overlap population 5σ (σ2p) overlap population = 0.732 = -0.308 = 0.654 = -0.060 σ overlap: 0.364 π overlap: 0.654 (1 σ and 2 π bonds) Total overlap: 1.018 (80% of N2 =1.276) a triple bond

A final example: Nitric Monoxide (NO) 0 N O vacuum level 14.53 ev 13.6 ev potential energy, ev 2p 2s 2p 2s

A final example: Nitric Monoxide (NO) 0 N O σ2p * vacuum level 14.53 ev 13.6 ev potential energy, ev 2p 2s σ2p σ2s * 2p 2s σ2s

A final example: Nitric Monoxide (NO) potential energy, ev 0 N O 2p 2s σ2p * 14.53 ev 13.6 ev π2p * σ2p π2p σ2s * 2p 2s vacuum level σ2s

A final example: Nitric Monoxide (NO) - 11 electrons N O 0 σ2p * vacuum level π2p * potential energy, ev 2p 2s π2p σ2s * σ2p 2p 2s σ2s

A final example: Nitric Monoxide (NO) - 11 electrons For NO: bond order = 2.5 13.6 ev NO is paramagnetic IP is less than 13.6 ev Electron configuration is: σ2s 2 σ*2s 2 π2p 4 σ2p 2 π*2p 1 One electron in the HOMO

The fool-proof procedure for constructing energy correlation diagrams: 0. Draw the vacuum level. 1. Put the atomic orbitals for each bonding partner in your diagram. Position the HOAO based upon the IP of the atom. 2. Draw in the energy levels for your MOs. You ll need one for each atomic state. 3. Fill them with electrons. Make sure to follow Aufbau and Hund s rules. Easy as Toast!

Another example: H2O Nomenclature: Mulliken includes 1s MOs: Ours (8 electrons): 1a1 2 1b2 2 2a1 2 1b1 2 His (10 electrons): 1a1 2 2a1 2 1b2 2 3a1 2 1b1 2

Another example: H2O Using the gross atomic populations, we find: atomic populations: Oxygen: 1s 2.00 2s 1.85 2p 4.50 Hydrogens (each): 1s 0.82

Another example: H2O Using the gross atomic populations, we find: On the Oxygen (N0 = 8): N(O) = 8.349 On the Hydrogens (N0 = 2): N(H2) = 1.645 Gross Charge -0.35e +0.35e

Another example: H2O Bonding occurs through the 2a1 and 1b2 orbitals. The higher energy 3a1 and 1b1 do not contribute to the bonding.