Speaker
Masahiro Kawasaki
Description
Primordial black holes (PBHs) are a promising candidate for the dark matter in the universe. We present mechanisms that produce large density fluctuations that lead to the formation of dark matter PBHs. As PBH formation models, we consider multi-field inflation, the axion-like curvaton model, and the non-topological soliton model.
Details
N/A
| Internet talk | No |
|---|---|
| Is this an abstract from experimental collaboration? | No |
| Name of experiment and experimental site | N/A |
| Is the speaker for that presentation defined? | Yes |
Author
Masahiro Kawasaki