  In this follow-up to our paper from 2005, we briefly discuss the implications
of the apparent detection of B modes in the Cosmic Microwave Background for the
issues raised in that paper. We argue that under the assumptions of eternal
inflation, there is now stronger support for the detectability of a Coleman-De
Luccia bubble nucleation event in our past. In particular, the odds that the
spatial curvature of the universe is large enough to be detectable by near
future experiments are increased.
