“…However, under reasonable assumptions, depending on the temperature behavior of the bias term, PBHs with masses in the range M ∼ 10 4 − 10 7 M and representative fraction f 10 −6 can be created. Interestingly, such heavy PBHs can play an important role as seeds for the formation of cosmological structure, alleviating several problems of the CDM scenario on sub-galactic scales, and providing an avenue to explain the origin of the supermassive BHs [9,10].…”