We've studied atomic structure. We started in the 1800s with Dalton's atomic theory. He stated that all matter consists of atoms. But what makes up atoms? We discovered electrons with the cathode ray experiment. But that left us with the confusing plum pudding model. Thankfully, Ernest Rutherford performed his famous gold foil experiment. We developed the nuclear model!
The nuclear model only got us so far. We didn't understand how electrons worked. Neils Bohr's model proposed that electrons reside in orbits. That helped account for Planck's quantum theory. But Einstein altered everything! How? He explained the photoelectric effect via the wave-particle duality. Soon after, Lewis De Broglie applied it to electrons. Suddenly, we entered the age of quantum mechanics!
Erwin Schrodinger developed the quantum mechanical model. Soon we understood that electrons reside in atomic orbitals. We describe them with quantum numbers. They tell us the energy, shape, and electron spin. But, we still didn't understand everything! We needed to figure out how bonding worked.
Previously, we studied valence bond theory. It's one of the two theories that use quantum mechanics to describe bonds. Today, we'll look at the Molecular Orbital Theory.
Basics of Molecular Orbital Theory
In valence bond theory, bonded atoms share electrons. The electrons experienced electrostatic attraction to each nucleus. The assumption is that they remain localized between the nuclei. But, let's think about atomic orbitals. Electrons can move around all sides of an atom. In molecular orbital theory, the electrons can move around the whole molecule. Why does this make more sense? Let's imagine a massive molecule. Something like octadecane. Its molecular formula is C18H38. The electrons can interact with any of the nuclei. There is nothing that keeps them between two atoms.
So, what happens to the atomic orbitals when two atoms bond? They combine into molecular orbitals. Every atomic orbital produces a molecular orbital. For example, let's consider a hydrogen molecule. Its two 1s-orbitals overlap. So, they create two molecular orbitals. How do we get two? Remember, we can describe orbitals as waves. So, the orbitals can constructively or destructively interfere. The constructive interference creates a bonding molecular orbital. Destructive interference generates an antibonding molecular orbital.
Here's how we write it mathematically.
BondingM.O=Ψ=1sa+1sb
AntibondingM.O=Ψ∗=1sa−1sb
The fancy term for this math is a linear combination of atomic orbitals. Doesn't that sounds complicated?! But it just means addition and subtraction of the orbitals.
What does any of this have to do with bonding? The bonding molecular orbital is more stable. So, the electrons fill it first. The antibonding molecular orbital is at a higher energy level. So, it would be the excited state.
What about larger molecules? Like atomic orbitals, the p orbitals have higher energy than the s. So, when we draw our orbital diagram, s overlaps are below p overlaps. The only other thing we need to add is sigma and pi orbitals. Sigma orbitals form with a straight-on overlap. That happens between two s-orbitals or an s orbital and px orbitals. The py and pz overlaps generate pi orbitals. In pi orbitals, the overlap is lateral. They bend over the top or sides of the molecule. The sigma bonding orbital has the lowest energy. The sigma antibonding has the highest. The pi orbitals energies are between them.
Dioxygen Example
As an example, let's consider dioxygen. We have 12 valence electrons between the two oxygen atoms. Each oxygen brings a 2s orbital and three 2p orbitals. So, we would form eight molecular orbitals. But where do we put the electrons? Let's look at each set of orbitals.
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The two s orbitals form a sigma bonding and antibonding orbital. Each will hold a pair of electrons. That's four out of twelve electrons.
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The two p_{x} orbitals will yield a sigma bonding and antibonding set. Two of the electrons fill the bonding orbital. That's six out of twelve electrons.
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The py and pz orbitals will each produce a pi bonding and antibonding set. An electron pair fills each of the pi bonding orbitals. What about the last two electrons? They each half fill one of the pi antibonding orbitals. That's all twelve electrons!
- The electrons only half-fill the pi antibonding orbitals. Why? Because unpaired electrons have lower energy. Remember, spin pairing increases the electrostatic repulsion. So, it's more stable to half-fill each pi antibonding orbital.
Advantages and Disadvantages of Molecular Orbital Theory
There seems to be a competition between Molecular Orbital Theory and Valence bond Theory. Many people will say that Molecular Orbital Theory is superior. But, they are two sides of the same coin. Computational chemists use both theories. Sometimes, one is more descriptive. Sometimes the other is easier to apply. It depends on the molecule. But, for any molecule, both theories should generate the same result. It's more about which model is more intuitive.
So, what are its advantages? The main benefit is that we get a picture of the whole molecule. For example, let's imagine dispersion forces. If the electrons can move freely about the molecule, it's easy to imagine a temporary dipole. Valence bond theory can still explain dispersion. But, when electrons are more localized, it's harder to envision. Another advantage is its explanation of excited states. Like atoms, molecules absorb and emit light. An electron can get excited into an antibonding orbital. That's the basic premise of UV-visible spectroscopy.
What are the disadvantages? Both ionic and covalent bonding become more abstract. It's easier to think of bonds between atoms. That makes intuitive sense. The electrostatic interactions keep everything together. But, in molecular orbital theory, we are thinking of orbitals. It's not always clear how overlapping orbitals make bonds.