Black holes thermodynamics to all orders in the Planck length in extra dimensions

dc.creatorNouicer, Khireddine
dc.date2007-06-19
dc.date2007-11-22
dc.date.accessioned2026-07-07T11:17:00Z
dc.date.available2026-07-07T11:17:00Z
dc.descriptionWe investigate the effects to all orders in the Planck length, from a generalized uncertainty principle, on the thermodynamic parameters of radiating Schwarzschild black holes in a scenario with large extra dimesions. We show that black holes in this framework are hotter, decay faster and are less classical objects. Particularly, we show that the final stage of the radiation process is a black hole remnant with zero entropy, zero heat capacity and non zero finite temperature. We finally compare our results with the ones obtained in the standard Hawking picture and with the generalized uncertainty principle to leading order in the Planck length.
dc.description21 pages, 6 figures, 1 table; Figure 2 replaced and section 4 improved
dc.identifierhttps://arxiv.org/abs/0706.2749
dc.identifierhttp://arxiv.org/abs/0706.2749
dc.identifierClass.Quant.Grav.24:5917-5934,2007; Erratum-ibid.24:6435,2007
dc.identifierdoi:10.1088/0264-9381/24/23/014 10.1088/0264-9381/24/24/C02
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192865
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack holes thermodynamics to all orders in the Planck length in extra dimensions
dc.typetext

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