6.8  That Reminds Me of Something

 

Cormorant, who has studied a bit of Chemistry in his time, remarks “You know, those wavefunctions we've discovered remind me a bit of atomic orbitals. I mean like s-orbitals seem a bit like the n=1 function and p-orbitals are like n=2. Is that cool, or what”.

“What” replies Nefertiti. “I think you’re comparing apples to oranges there. But, we may still learn something if we pick apart your confused notion”. Cormorant considers this concession to be a minor triumph.

Let’s take a quick look at this issue.  In Chemistry, we learn that electrons in atoms are confined – or, at least, are most likely to be found - in regions of space, surrounding the nucleus, which we call orbitals. Cormorant is correct that these are, in reality, based on wavefunctions that describe the probability density for the position of the electron within the atom.  They were discovered not by experiment but by Erwin himself, solving his own equation - in three dimensions - with the electrostatic potential field arising from the positive charge of the nucleus. The solutions are three-dimensional wavefunctions

Because of the spherical symmetry of the potential field surrounding the nucleus, it is mathematically extremely helpful to abandon the usual Cartesian x,y,z coordinates and instead use polar coordinates, which means these wavefunctions are of the form ψ(r,θ,φ), where r is the distance from the nucleus and θ,φ are angles,  relative to the x- and z-axes. This has the effect of making the wavefunction separable, so ψ(r,θ,φ) = ψr(r)ψθ(θ)ψφ(φ). We already know, from what we've been able to do by separating the time and spatial parts of the overall wavefunction, just how precious this separability is. 

An electron in an atom is - in a sense - confined in a “box”, just like our model particle, but that box is an infinite sphere, with the nucleus in the middle and infinity at the outside. The three-dimensional wavefunction must, therefore, go to zero at the edges of the box (in other words, as r tends to infinity), to meet the smoothness requirement that led to the same thing in our one-dimensional box and also to allow the function to be normalised. There are more boundary conditions too, resulting from the need for the wave function along a line at an angle θ relative to the coordinate system to be the same at an angle θ+2π, or θ+4π etc, because these physically represent the same line. As a result, the physically possible wavefunctions are limited by quantum numbers and the possible energies are, correspondingly, limited to certain possible values. The detail of this is mathematically fearsome but we can see that - in general terms - what we foresaw back in chapter 1 is indeed the case:   the quantisation of energy in an atom is a consequence of the need for a stable standing wavefunction for an electron. Hurrah!

We should be careful to be clear what we are looking at in the familiar pictures of s- and p-orbitals we learn in Chemistry: