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oldphysicist
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I am unable to find a practical answer to this in any of the conventional texts. Suppose an excited atom drops back down to the ground state and emits a single photon of energy h-nu. The conventional description of this photon is that it is a single excitation of the EM field contained in an arbitrary but specific normalizing volume V, and that it has a definite wavenumber k and polarization vector e. This "wave" can then travel half way across the universe (e.g.) and interact with an identical atom, exciting it back up to the original state. What is the actual shape of the wave that propagates forward? The normalizing box V does not really exist, so what is the precise value of E and H in this wave in its free space flight? Does it really extend to +/- infinity in the perpendicular plane, which is what the definition of a plane wave implies. Also, since this wave must have some of the characteristics of a pulse - after all, it is a single photon - what is the shape in time of the pulse? It is hard to establish the form of a Poynting vector for this field, from which the total energy (h-nu) could be determined. This transition between quantum and classical theory for EM fields seems to fall between the cracks of conventional discourse.