Speaker
Dipan Sengupta
(University of New South Wales)
Description
Astronomical and Cosmological data irrefutably point towards an invisible matter component of the universe 5 times denser than the visible matter. The masses of particle physics dark matter masses can span over 30 orders of magnitude. On the heavy dark matter mass, high energy gamma ray telescopes provide an unique opportunity to probe the parameter space of well-motivated models. I will review the potential of CTA to discover and probe heavy dark matter models, including the conclusions of the Snowmass ultra-heavy dark matter working group.
Primary author
Dipan Sengupta
(University of New South Wales)
