A new model for the formation of mini black holes

Esmer G., Zebitay S.

GENERAL RELATIVITY AND GRAVITATION, cilt.32, sa.7, ss.1241-1254, 2000 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 32 Sayı: 7
  • Basım Tarihi: 2000
  • Doi Numarası: 10.1023/a:1001986503301
  • Dergi Adı: GENERAL RELATIVITY AND GRAVITATION
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.1241-1254
  • İstanbul Üniversitesi Adresli: Hayır

Özet

A new model different from the Hawking model is suggested to describe the formation of mini (primordial) black holes. It is based on an idea that the fluids, which All in the universe at the beginning just after the big bang, are separated into mini clusters, moving with supersonic velocities and colliding with each other under the forces of gravitational attractions. We show that between the time era from 10(-43) to 10(-8) sec. about 36 various generations of mini black holes with masses ranging in the interval 10(-5)-10(30) gm are possible.