7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Using mHz gravitational waves to catch galactic center mergers of supermassive dark matter cores

12 Jul 2024, 17:40
20m
Aula 38 (Palazzo Micara of the ‘Gabriele d’Annunzio’ University)

Aula 38

Palazzo Micara of the ‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Talk in a parallel session Low frequency gravitational waves: sciences and detections Low frequency gravitational waves: sciences and detections

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)

Presentation materials

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