Primordial Black Holes from the inflating curvaton
  The primordial black hole (PBH) formation is studied in light of the
inflating curvaton. The typical scale of the PBH formation is determined by
curvaton inflation, which may generate PBH with $10^{14}\mathrm{g}\le
M_\mathrm{PBH}\le 10^{38}\mathrm{g}$ when curvaton inflation gives the number
of e-foldings $5\leq N_2\leq 38$. The non-Gaussianity of the inflating curvaton
does not prevent the PBH formation.
