Speaker
Dr
Camilo Garcia Cely
(DESY)
Description
A rather minimal possibility is that dark matter consists of the gauge bosons of a
spontaneously broken symmetry. Here we explore the possibility of detecting the gravitational waves produced by the phase transition associated with such breaking. Particularly promising for LISA is the super-cool dark matter regime,
with DM masses above 100 TeV, for which we find that the gravitational wave signal
is notably strong. ONLINE TALK.
Author
Dr
Camilo Garcia Cely
(DESY)