Fri, May 25, 2018
11:00 am - 12:00 pm
PRB M2005
I will show that a bound state with colored quark-like constituents can be a weakly interacting dark matter candidate. I will also discuss a mechanism how it becomes the dominant component of the total dark matter abundance. At the same time an unavoidable consequence will be a subdominant population of dark matter with strong interactions with visible matter and interesting phenomenology.