This theory holds that in its early history, the observable Universe underwent a period of exponential expansion, doubling in size many dozens of times, growing our observiball a tiny fraction of the size of an atomicnucleus to that of, say, a beach ball.
This is the point when neutrons released during the break-up of an atomicnucleus are more likely to hit and shatter other nuclei (thus releasing further neutrons), than to escape to the outside world where they merely generate Cherenkov radiation and tear up any living tissue that they pass through.