Throw (slowly, compared to c) a black hole (BH) through a Bonnor beam (BB). Throw a white hole (WH) through a Bonnor beam. Ignore technical difficulties in superimposing the exact solutions for the moment. The breaking of the axial/spherical symmetries is deliberate.
Qualitatively what happens, in your view, when the WH touches the beam? Is it just the time reversed picture of the BH intercepting the BB? There's a part of the first spacetime where some of the light is trapped in the BH as it flies off to infinity after its encounter with the beam. Is there a part of the second spacetime in which some of the light is trapped in the WH? If so, where is it if the initial conditions are a Bonnor beam at large spacelike separation from the white hole? Does the WH cut a gap into the beam?
Alternatively, take two widely separated BHs. Grind out the Raychaudhuri equation, bearing in mind the focusing theorem. Now take two widely separated WHs. What's different? How does a circular orbit of two WHs evolve? Outgoing GWs tend to circularize elliptical binary BH orbits. Can a circular binary WH orbit decircularize? How? ("Incoming GWs from initial conditions" is not very satisfying).
The problem I think is confusing the reversal of the entire BH spacetime with a WH stitched into an ordinary Minkowski in the asymptotic limit, or into a cosmology. (Bonnor is essesntially the latter). More broadly, a WH should be able to live with future-directed null geodesics.
Of course, I could only agree with a response like, "well such a WH is almost certainly unphysical", but maybe we could ignore that in order to think about what happens when a plane wave hits a WH.