Orateur
Dr
Ville Vaskonen
(IFAE)
Description
The merger rate of $\mathcal{O}(10M_\odot)$ black holes inferred from the LIGO-Virgo observations indicates that these binaries generate a sizeable gravitational wave foreground. In this talk I will present a simple analysis quantifying the impact of this foreground on the detectability of the primordial gravitational wave background by future gravitational wave experiments.
Authors
Dr
Ville Vaskonen
(IFAE)
Dr
Marek Lewicki
(University of Warsaw)
