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.
Primary author
Dr
Camilo Garcia Cely
(DESY)
