Speaker
Jorge Armando Rueda Hernandez
(ICRANet)
Description
There is an open debate about whether some galactic centers (including Sgr A*) could actually be supermassive dark matter cores made of fermions with masses in the range of 60-350 keV. We discuss the possibility of pinpointing mergers of such cores using mHz gravitational waves with the forthcoming space-based interferometers and assess the consequences of the possible outcomes from the physical and astrophysical viewpoint.
Primary authors
Carlos Raúl Argüelles
(La Plata National University & ICRANet)
Jorge Armando Rueda Hernandez
(ICRANet)
Jose Fernando Rodriguez Ruiz
(Universidad Industrial de Santander)
Remo Ruffini
(ICRANet, ICRA, INAF)