Please use this identifier to cite or link to this item: http://repositorio.ufla.br/jspui/handle/1/50196
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dc.creatorLobo, I. P.-
dc.creatorSantos, G. B.-
dc.date.accessioned2022-06-10T22:26:35Z-
dc.date.available2022-06-10T22:26:35Z-
dc.date.issued2021-06-
dc.identifier.citationLOBO, I. P.; SANTOS, G. B. Thermal dimensional reduction and black hole evaporation. Physics Letters B, [S.I.], v. 817, 136272, June 2021. DOI: https://doi.org/10.1016/j.physletb.2021.136272.pt_BR
dc.identifier.urihttp://repositorio.ufla.br/jspui/handle/1/50196-
dc.description.abstractWe analyze how a quantum-gravity-induced change in the number of thermal dimensions (through a modified dispersion relation) affects the geometry and the thermodynamics of a charged black hole. To that end we resort to Kiselev's solution as the impact such modifications have on the evaporation rate of the black hole becomes more clear. As an application, we study the case for which the thermal dimension is reduced to two.pt_BR
dc.languageenpt_BR
dc.publisherElsevierpt_BR
dc.rightsacesso abertopt_BR
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourcePhysics Letters Bpt_BR
dc.subjectLorentz violationpt_BR
dc.subjectBlack hole evaporationpt_BR
dc.subjectDimensional reductionpt_BR
dc.subjectViolações de Lorentzpt_BR
dc.subjectBuraco negro - Evaporaçãopt_BR
dc.subjectRedução dimensionalpt_BR
dc.titleThermal dimensional reduction and black hole evaporationpt_BR
dc.typeArtigopt_BR
Appears in Collections:DFI - Artigos publicados em periódicos

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