- #1
Rafid Mahbub
- 2
- 0
I have been studying primordial black hole formation through inflation for a while and I was curious to know how the parameters in an inflation model are determined such that they are consistent with CMB constraints. In my literature reviews, there are quite a few models that exhibit an inflection point in the inflaton potentials, but with quite a few parameters that need to be tuned. Is some kind of Markov Chain Monte Carlo method used to do this?