Speaker
Csaba Balazs
(School of Physics and Astronomy, Monash University)
Description
CTA will search for dark matter in the centre of our galaxy and in dwarf spheroidal satellites. I show preliminary results on how we plan to distinguish the astrophysical background from the dark matter signal and which dark matter candidates CTA might have a chance to detect.
Primary author
Csaba Balazs
(School of Physics and Astronomy, Monash University)
