Normalizing Wave-functions
Most recent answer: 01/19/2015
- Alok (age 26)
Kingston, RI
Actually, the normalization condition is applied to that whole state:
|c1|2+ |c2|2+...|cn|2=1.
That makes the spatial integral of the absolute square of ψ come out 1, because the different ψj are orthogonal to each other and thus their products drop out of that integral. Here I'm assuming that your ψj's are meant to be the energy eigenstates.
Mike W.
posted without vetting until Lee gets back.
(published on 01/19/2015)
Follow-Up #1: superpositions of different energies
- Alok (age 26)
Kingston, RI, USA
If the atom is in the ground state, it's just plain in the ground state and not a superposition of states with different energies. More general states do indeed have amplitudes for states with different energies. Despite how quantum mechanics is often taught, there's nothing more or less mysterious about having states with a range of different energies than there is about having states with a range of different positions and a range of different momenta. Those spreads are of course basic properties of all quantum states. States with a single fixed energy (energy eigenstates) play a special role because their physical properties don't change in time. So you know right away that such states must be atypical, because things happen.
Mike W.
posted without vetting until Lee returns
(published on 01/20/2015)
Follow-Up #2: discrete photon energies from atoms
- Alok (age 26)
The Schroedinger equation is completely linear. That means that the output state after some time has passed is exactly the sum of the output states of the various components of the initial state. So all we have to think about is what becomes of each of those various energy eigenstates separately, since we can always add up things like that to get what becomes of the initial state that is a superposition of them.
Each so-called energy eigenstate (other than the ground state) is actually not quite an eigenstate of the full Hamiltonian, which includes the quantized electromagnetic field. Nonetheless, the electromagnetic field will not end up in a lower energy state than it started in, so conservation of energy tells us that the atom will not end up in a higher energy state than it started in. If the atom changes, it can only change to some superposition of the discrete batch of lower-energy quasi-eigenstates. For each of those components energy conservation requires that the EM field carry off the particular energy lost by the atom going from the initial to the final state. So that leaves a discrete set of energies for the field. Generally, the fastest processes involve emitting a single photon, so those discrete energy differences give the set of single-photon energies. For rarer multi-photon processes only the sum of the photon energies is set by that constraint. So those processes can give a smooth spectrum, rather than sharp emission lines.
A quick search turns up an accessible article on this effect from quantum wells (), rather than atoms, but the basic ideas should be the same. The two-photon emission spectrum is very broad. Note that even the single-photon spectrum already has a bit of width. That's a reminder that the electron eigenstates aren't quite true eigenstates once the quantized field is included.
Mike W.
posted without vetting until Lee returns
(published on 01/20/2015)