Here's a simplified system: connect optical fibres to each slit, and place a photon detector at the other end of each fibre. Now, let the experimenter make a choice (delayed until the light is already traveling in the fibres) whether or not to splice a beam-splitter carefully between the fibre ends and the detectors.
Say the initial wave-function is w=a.w1+b.w2 (where w1 is the wave-function when slit B is blocked). If the photon is allowed to directly reach the detectors (this position measurement, like a which-slit measurement, causes collapse into the basis of w1 or w2), so detection A occurs with probability a^2 etc.
If the beam-splitter is inserted (so that this position measurement, equivalent to measuring the interference or phase difference between the paths, causes collapse into the basis of .7 w1+w2 or .7 w1-w2) then the probability of detection A is .5(a+b)^2, and so forth.
In both cases we've effectively calculated the probabilities by summing the amplitudes of each possible photon-path leading to the detector's position. Of course, when we look at it this way, we actually haven't solved the Schroedinger equation. Perhaps this isn't Copenhagenny enough, so here is an alternative proceedure to apply to Wheeler's experiment:
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Start with the initial assumed wave-function, which is a function of amplitude across the transverse plane (ie. a double top-hat function, representing the double-slit). Next, solve the SE for the evolution of the wave-function. For propagation a long distance through free space, the SE is equivalent to a Fourier transform (giving a sinc function). (For optional propagation through a thin lens, the SE reduces to ... a Fourier untransform.) So we again know the amplitude at each point where we might choose to make a measurement. (Note this detailed procedure is important to confirm the predictions; I think it's incorrect application of the shorthand notation which has given you wrong answers.)
But this hasn't really discussed collapse. Plainly, I think collapse is irrelevant unless we make a second measurement. For example, if I wanted to add additional aperture screens, I would collapse the wave-function at those axial-positions by zeroing the wave-function at transverse-positions blocked by the aperture (then renormalising, all assuming we're only interested in photons that do get through). So understanding collapse is useful if we have a sequence of inter-spaced lenses and apertures in front of our detector (or if we have a multiple entangled particles to measure), but just doesn't enter into Wheeler's experiment. Collapse tells the shape of the wave-function after a particular measurement result, but is not used directly to determine the probability of that result occurring.