A simple model for the evaporation of black holes at final stages |
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| Authors: | S O Alexeyev A Barrow G Bowdole M V Sazhin O S Khovanskaya |
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| Institution: | (1) Institut de Physique Nucleair, Grenoble, France;(2) Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119899, Russia |
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| 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 1–103 m P1. 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. |
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| Keywords: | black holes evaporation at final stages |
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