Does accelerating cosmological expansion increase beam spread?
In the standard textbook case, a transmitter of diameter can produce an electromagnetic beam of wavelength that has spread angle . But what happens in an expanding cosmology, especially one that accelerates so that there is an event horizon? Does increase with distance?
Obviously each photon will travel along a null geodesic and after conformal time have travelled units of co-moving distance. The distance between the beam edges would in flat space be growing as . Now, co-moving coordinates are nice and behave well with conformal time, so I would be mildly confident that this distance is true as measured in co-moving coordinates.
But that means that in proper distance the beam diameter is multiplied by the scale factor, (where is the time corresponding to ), and hence increases. However, the distance to the origin in these coordinates has also increased to , so that seems to cancel the expansion - if we measure globally by dividing the lengths.
But it seems that locally we should see the edges getting separated at an accelerating pace; after all, the local observers will see the emitter accelerating away from them, producing a wider and wider beam near their location since it was emitted further away. From this perspective as time goes by the beam ends up closer and closer to (and ever more red-shifted, which presumably keeps the total power across it constant).
Does this analysis work, or did I slip on one or more coordinate systems?