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

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dc.creatorAlexeyev, S.
dc.creatorBarrau, A.
dc.creatorBoudoul, G.
dc.creatorKhovanskaya, O.
dc.creatorSazhin, M.
dc.date2002-01-21
dc.date2002-06-26
dc.date.accessioned2026-07-07T11:29:55Z
dc.date.available2026-07-07T11:29:55Z
dc.descriptionOne 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.
dc.description15 pages, accepted to Class. Quant. Grav
dc.identifierhttps://arxiv.org/abs/gr-qc/0201069
dc.identifierhttp://arxiv.org/abs/gr-qc/0201069
dc.identifierClass.Quant.Grav.19:4431-4444,2002
dc.identifierdoi:10.1088/0264-9381/19/16/314
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196872
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleBlack Hole Relics in String Gravity: Last Stages of Hawking Evaporation
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