Following the discovery of signals from coalescing black hole and neutron star binaries, a new frontier in gravitational wave (GW) research is the detection of sources emitting periodic or quasi-periodic continuous waves (CW). The project "new GEMS" is a three-year project starting in 2022 which has been granted by MIUR, within the PE9 PRIN grants. The proposed multidisciplinary approach that exploits cutting-edge expertise and facilities in both GW science and astrophysics, with the goal of carrying out highly sensitive searches for CW, will be presented. The goal is the detection of CW sources using LIGO-Virgo-Kagra data and/or data of 3rd generation detectors like the Einstein Telescope.
Link zoom: https://uniroma1.zoom.us/j/87038625161?pwd=cEtGRjZNT2VWSlJIWmxaYmxSMDhRZz09#success
L. Cardani, C. Rovelli