Speaker
Prof.
Thomas Hambye
Description
After a very short review of the WIMP dark matter scenario and constraints, I will discuss another possibility to account for the necessary suppression of the number of dark matter particles during the early Universe radiation dominated era: "super-cool dark matter".
This is based on the recent work, arXiv:1805.01473, in collaboration with A. Strumia and D. Teresi.
Author
Prof.
Thomas Hambye
