Speaker
Mrs.
Esipova Ekaterina
(NRNU MEPhi)
Description
In the report, self-interacting dark matter is considered. It is supposed that it can form bound states (with possible successive annihilation) due to long-range dark forces. In the course of cosmological evolution, such dark matter may form two components: "passive" one in the form bound-states and "active" (possibly small) one in the form of free dark-charged dark matter particles. Such scenario may have implications for different astrophysical and cosmological issuses.
Primary author
Mrs.
Esipova Ekaterina
(NRNU MEPhi)