With Schrö(dinger), I meant old Erwin.
The wavefunction of an electron depends on 3 spatial dimension and the time - depending on what you're interested in, you can aggregate the spin to that, and it should be all unless I make a blunder.
Some wavefunctions are "stationary", that is, only their phase varies like exp(2iπEt/h) where E is a definite energy, and their amplitude depends only on x, y, z but not t. So for instance the probability |ψ|
2 to find the electron around a location does not depend on the time, hence "stationary".
When the electron is trapped in an atom, that is, is has too little energy to escape, stationary wavefunctions are called "orbitals". These are especially interesting because their energies are well spaced, so usual heat doesn't send the electron from one orbital to the other; as a consequence,
at equilibrium, the electrons fill the deepest available orbitals. That's simple (...except that electrons interact, so the filling depends an all electrons, and the orbitals aren't exactly the relatively simple ones we know for a hydrogen atom).
The orbitals are centered on the nucleus and don't move, that is, |ψ|
2 is static. This is why the electron doesn't radiate in an atom at rest. That's why QM was needed historically , and it solves it brilliantly.
Though, the stationary solutions are not the only ones. ψ
1 and ψ
2 being solutions, any a
1*ψ
1 + a
2*ψ
2 is a solution too. While orbitals have definite energies, their linear combinations have no definite energy as they can't be written as ψ(x,y,z)*exp(2iπEt/h), and they evolve over time.
Take a weighed sum of 1s and 2p orbitals. 1s is spherical, so apart from the exp(2iπE
1St/h) phase, it has the same phase and sign all around the nucleus. 2p is a peacock, with one side + and the other -, all multiplied by its exp(2iπE
2Pt/h).
http://winter.group.shef.ac.uk/orbitron/ (choose in the left margin)
Now, because E
1S ≠ E
2P, and since the exp(...t) combine with the + and - to define the phase, at some t the 1s and 2p orbitals will be in phase at the right side and |ψ|
2 increases there and decreases at the left side, while at other t, |ψ|
2 increases at left. This is an eccentric position that moves over time, with a speed and acceleration.
The bulge in |ψ|
2 makes a complete cycle around the nucleus at the frequency (E
2P - E
1S)/h, and because the charge accelerates, it radiates light with that frequency, or a photon energy E
2P - E
1S.
By the way, peacocks are not the only solution for the 2p orbitals. Doughnuts are just as good and as fundamental; peacocks are linear combinations of doughnuts and vice versa. Other linear combinations give elliptic orbitals. And if you combine a doughnut 2p with a 1s, then the bulge in |ψ|
2 orbits the nucleus instead of wobbling between right and left of the nucleus. Correspondingly, the emitted photon is polarized circularly, while it's linear with a peacock 2p.
2p and 1s differ by the adequate amount, so |ψ|
2's bulge moves properly. As opposed, 2s and 1s still make a pulsating linear combination, but this pulsation is spherical, so it doesn't radiate light, as light is polarized as a vector (the photon's spin is 1, in other terms). While such linear combinations are possible, there is no radiative transition between 2s and 1s: this is a "forbidden transition". The same happens between 3d and 1s: their linear combination has two bulges orbiting the nucleus at 180° or, depending on the 3d you choose, wobbling between right and left simultaneously and both at the centre. This makes no electric dipole but a quadripole instead, which doesn't radiate efficiently an electromagnetic field, so that transition too is forbidden.