Hello conway,
conway said:
I took quite a lot of flak yesterday for suggesting that the pure eigenstates of a hot gas in thermal equilibrium were an artifact of the Copenhagen interpretation. I claimed that it is just as consistent with experiment to assume that all the atoms are in a superposition of eigenstates. I haven't seen anyone post an experiment which shows how you can distinguish these two descriptions. So I'm thinking it might be a nice gesture is someone would acknowledge that I might have been correct on this small point.
I'm not sure anyone is claiming that all the atoms in a hot gas in thermal equilibrium are all in pure energy eigenstates (at least I don't
think anybody is claiming this).
Personally, I agree with you that a given atom, that hasn't just released a photon, is far more likely to be in some sort of superposition of energy eigenstates at any given time. Even if the atom is mostly in a eigenstate, there is likely at least a little superposition of other eigenstates, as long as some sort of perturbation has taken place. So yes, in my opinion, I acknowledge you are correct on this.
I think the objection is only in terms of your claim that an electron radiates energy
merely by being in a superposition of energy eigenstates.
The way I understand the standard theory is as such. Suppose an atom is prepared into a superposition of two energy eigenstates, say a linear combination of one s and one p, and if then left in a vacuum isolated chamber, it will remain in that superposition state for some time. During this time it will not radiate any energy at all (regardless of the fact that the wave-function's expectation value is oscillating). Then suddenly it will emit a photon which has an energy which is exactly the excitation energy from the s state to the p state (whichever two states were in the superposition). Immediately after the emission, the electron is an energy eigenstate (the s state, in this example). Of course if the atom were then perturbed, by being bumped into another atom, it would go back into some sort of superposition of states (not necessarily like it was before, and not necessarily a superposition of just two energy eigenstates).
The amount of time that the atom remains in the superposition of states (before emitting the photon) is a probabilistic function of the relative amounts of the eigenstates in the superposition. A 90% s and 10% p will statistically last longer in the superposition state than a 50-50% combination. The extra energy that can be thought of as "boosting" the energy up to the p state, such that a photon with the right energy can be emitted, is a function of the quantum fluctuations in the zero-point vacuum energy (that might be a very bad way to put it). Perhaps I should reword that. There is a probability that the electron might be found in the p rather than s state, and that probability determines the statistical lifetime of the superposition state. (It has been said that in QM, there really is no such thing as spontaneous emissions and that all emissions can be thought of as stimulated emissions -- the
spontaneous emission case is really just a special case of stimulated emission, where the emission was stimulated by the zero-point vacuum energy.)
The point of all of that, is when it comes to electromagnetic radiation of an electron in a superposition of states, it's either all or nothing. Either the atom remains in the superposition -- radiating nothing, or it emits a photon which has an energy equal to the difference in energy between the two energy eigenstates in the superposition. The ratio of the relative eigenstates in the superposition has no bearing on the photon's energy (well, assuming that the two energy eigenstates are both at least present to some degree) -- it only has an impact on the amount of time it takes for the superposition state to decay. Or in the case of stimulated emission, it affects the probability that stimulated emission will occur.
This is experimentally verifiable. It can be performed with a trip to the Radio-Shack(TM), and a purchase of a small neon bulb, a current limiting resistor, and a diffraction grating or prism. I'm guessing the cost of the experiment materials might be under around $15. Attach one of the resistor's leads to one lead of the neon bulb. Plug the spare leads into a nearby wall socket. Use the diffraction grating or prism to view the spectrum. You'll notice that the only light is in very, very narrow bands in the spectrum. The difference between these bands corresponds to certain excitation energies between different energy eigenstates of neon.
If an electron, in a state of superposition between two energy eigenstates were to continuously radiate (such as gradually becoming less of p and more of s), the resulting spectrum would be more continuous, and you wouldn't see the discrete bands. But continuous (broader) bands are not observed in the $15, Radio-Shack(TM) experiment. The observed data show the radiated bands are very, very narrow.
(All this of course hinges on accepting the idea that E = h \nu, but that's been quite well established going back to 1905.)
[Edit: Sometimes it is advantageous to approximate atoms as only being in pure energy eigenstates, if one is not concerned about position and momentum, and if nearly all of the measured interactions only deal with energy. In QM, what you measure is what you get -- if you measure energy, the wave-function appears to collapse to to an energy eigenstate. If you measure position, the wave-function appears to collapse to a position eigenstate (which resembles a Dirac delta function, and is
necessarily a superposition of energy eigenstates). But if nearly all the interactions of the experiment involve energy, and the measurements involve energy, then approximating everything as only being in pure energy eigenstates is often useful. It certainly simplifies things a lot. On the other hand, this approximation can mislead students into believing that atoms only occur in pure energy eigenstates. It is common for 1st year chemistry students to mistakenly believe that electrons in atoms only occur in these well defined electron orbitals or clouds (represented by the energy eigenstates), and that's it. We know that the shape is quite different (and time varying) when things are in superposition. But the misconception still persists. In all fairness though, even if it is a misconception, it still holds up pretty well as an approximation if the only thing that is of any concern is energy.]