摘要

I show that cosmological bubble walls in the thin wall approximation are unstable to the creation of "barnacles" - loci of different wall tension adjacent to regions filled with a third vacuum. Barnacle formation appears to have the same observational consequences as the extensively studied bubble collision scenario, but occurs exponentially more often. The process is described by a saddle point of the thin wall action with two negative modes.

  • 出版日期2012-7-9