Black Hole Relics in String Gravity: Last Stages of Hawking Evaporation

Details Black Hole Relics in String Gravity: Last Stages of Hawking Evaporation Black Hole Relics in String Gravity: Last Stages of Hawking Evaporation

2002-01-21

arxiv.org/abs/gr-qc/0201069v5

Class.Quant.Grav.19:4431-4444,2002

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

15 pages, accepted to Class. Quant. Grav

Scientific paper

10.1088/0264-9381/19/16/314

One of the most intriguing problem of modern physics is the question of the endpoint of black hole evaporation. Based on Einstein-dilaton-Gauss-Bonnet four dimensional string gravity model we show that black holes do not disappear and that the end of the evaporation process leaves some relic. The possibility of experimental detection of the remnant black holes is investigated. If they really exist, such objects could be a considerable part of the non baryonic dark matter in our Universe.

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