Dynamical FIMP with phase transition and gravitational waves in the scotogenic model
CTPU seminar room (Theory Building 4th Floor)
CTPU seminar room
Theory Building 4th Floor
IBS Main Campus, Daejeon
We consider the thermal effects into the evaluation of the dark matter production process.The kinematic of decay/inverse decay or annihilation processes can be affected by the finite temperature effects as the Universe cools down. The history of the symmetry respected by the model can be revealed by the DM relic abundance evolution processes. The strong first order electroweak phase transition generated gravitational waves can be probed.