Speaker
Erdenebulgan Lkhagvadorj
(Sungkyunkwan University)
Description
We propose a model of baryogenesis achieved by the annihilation of non-thermally produced WIMPs from Primordial Black Hole (PBH). Dark Matter (DM) particles can be produced by PBH evaporation and consequently re-annihilate into lighter particles even after thermal freeze-out. The re-annihilation of DM provides the observed baryon asymmetry and the correct relic abundance of DM depending on the PBH evaporation temperature.
| Secondary category for the parallel session (optional) | Dark Matter Physics |
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Primary authors
Erdenebulgan Lkhagvadorj
(Sungkyunkwan University)
Ki-Young Choi
(Sungkyunkwan University)
