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

被引：8

作者：

Alexeyev, SO ^{[1
]}

Barrow, A

Bowdole, G

Sazhin, MV

Khovanskaya, OS

机构：

[1] Inst Phys Nucl, Grenoble, France

[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2002年 / 28卷 / 07期

关键词：

black holes; evaporation at final stages;

D O I：

10.1134/1.1491964

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 1-10(-3) m(PI). 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. (C) 2002 MAIK "Nauka/Interperiodica".

引用

页码：428 / 433

页数：6

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