stevendaryl said:
I don't at all understand what you're saying. Could you take some very simple example and demonstrate what you mean?
An excited atom emits a photon and the electron descends to a lower orbital, removing energy from the atom into the photon (or it's wave function.) This energy is stored in the wave function of the photon (for where else can it reside as the wave function spreads out and evolves over time?) Now, this atom was on the surface of a star, and the wave function (carrying the energy) spreads out through the Universe, subtending a considerable volume of likely interactions. The wave function interacts with another atom, exciting it (this time in my retina) and, on its decay, and I "see" the light owing to the collapse of the wave function within the atom in my eye. This means the little green man 500 light years away cannot see the photon now, even though he is "equidistant" from the star's atom.
However, the same happens when the photon attempts to warm two rocks, lying near me, and near the little green man. So, the collapse of the wave function does not need an observer, or any other special situation. It simply needs to transfer energy. Once the energy is transferred, the wave function must necessarily instantaneously collapse everywhere in the Universe, all at one, otherwise there would be no such concept as the conservation of energy. Ipso-facto, as we say.
If this were not the case, there would be no such thing as the conservation of energy, and believe me, the Universe would be a very different place.
Therefore, I propose that there is no such thing as the "observer effect." There is just plain old physics, doing the conservation of energy thing.
As for the "aspect style experiment", I was proposing that the community explore the nature of collapse. Is there a case where the photon has so much energy, it can excite both atoms? This is the sort of "exploration" I am proposing. Is the transfer "sharp" in time, or has it a "shape" in space-time that can be explored?