Seminars/Colloquia
Rethinking false vacuum decay
by
→
Europe/Berlin
https://tum-conf.zoom.us/j/843685110?pwd=TEFqOEdOZ1FJWjBYa0lURFpmT09mZz09 (HS2 (5101.EG.502) and online)
https://tum-conf.zoom.us/j/843685110?pwd=TEFqOEdOZ1FJWjBYa0lURFpmT09mZz09
HS2 (5101.EG.502) and online
Description
Future gravitational wave interferometers may provide the first direct probe of the first second of our Universe. A first order phase transition in the early Universe would have sourced a stochastic gravitational wave background (SGWB). However, existing methods used to predict this SGWB are limited to weakly-coupled theories and often plagued by large uncertainties. In this talk, I will motivate that some of these obstacles can be overcome through an alternate definition of the action which has a natural implementation in the functional renormalization group. I will demonstrate how the proposal works in a toy model example, and sketch a roadmap towards accurate gravitational phenomenology and other applications.