Speaker
Gabriele Perna
Description
The advent of third generation interferometers marks a new era for Gravitational Wave (GW) searches and will enable to shed light on both early- and late-Universe dynamics. In this context, synergies between different Gravitational Wave detectors are crucial for a better detection and characterization of a GW Background, either of cosmological or astrophysical origin. Different cosmological sources, in fact, predict a broad spectrum which could be detectable in different frequency bands. We present the first collaborative project between the ET and the LISA collaborations, which aims to explore the advantages of a synergic search between the two detectors.