Astronomy Letters

, Volume 28, Issue 7, pp 428–433 | Cite as

A simple model for the evaporation of black holes at final stages

  • S. O. Alexeyev
  • A. Barrow
  • G. Bowdole
  • M. V. Sazhin
  • O. S. Khovanskaya
Article

Abstract

We present a simple model for the evaporation of primordial black holes at final stages with the formation of a relic remnant with a mass of 1–103mP1. The model takes into account the conservation of energy and the impossibility of passing through the state with the minimum possible mass. These relic remnants may account for a substantial fraction of dark matter in the Universe.

Key words

black holes evaporation at final stages 

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Copyright information

© MAIK "Nauka/Interperiodica" 2002

Authors and Affiliations

  • S. O. Alexeyev
    • 1
    • 2
  • A. Barrow
    • 1
  • G. Bowdole
    • 1
  • M. V. Sazhin
    • 2
  • O. S. Khovanskaya
    • 2
  1. 1.Institut de Physique NucleairGrenobleFrance
  2. 2.Sternberg Astronomical InstituteMoscowRussia

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