Speaker
Piotr Toczek
(University of Warsaw)
Description
Slow first-order phase transitions generate large inhomogeneities that can lead to the formation of primordial black holes (PBHs). We show that the gravitational wave (GW) spectrum then consists of a primary component sourced by bubble collisions and a secondary one induced by large perturbations. The latter gives the dominant peak if
Author
Piotr Toczek
(University of Warsaw)