Speaker
Hardi Veermae
(NICPB, Tallinn)
Description
We will discuss how gravitational wave astronomy can probe various primordial black hole (PBH) scenarios. This includes gravitational waves originating from coalescing PBH binaries in the late universe or from PBH formation in the early universe. These channels can be accessed by LISA if PBHs occupy the (sub)solar or the asteroid mass range, respectively.
Primary author
Hardi Veermae
(NICPB, Tallinn)
