Thermal dimensional reduction and black hole evaporation

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Campo DC	Valor	Idioma
dc.creator	Lobo, I. P.	-
dc.creator	Santos, G. B.	-
dc.date.accessioned	2022-06-10T22:26:35Z	-
dc.date.available	2022-06-10T22:26:35Z	-
dc.date.issued	2021-06	-
dc.identifier.citation	LOBO, 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.uri	http://repositorio.ufla.br/jspui/handle/1/50196	-
dc.description.abstract	We 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.language	en	pt_BR
dc.publisher	Elsevier	pt_BR
dc.rights	acesso aberto	pt_BR
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/	*
dc.source	Physics Letters B	pt_BR
dc.subject	Lorentz violation	pt_BR
dc.subject	Black hole evaporation	pt_BR
dc.subject	Dimensional reduction	pt_BR
dc.subject	Violações de Lorentz	pt_BR
dc.subject	Buraco negro - Evaporação	pt_BR
dc.subject	Redução dimensional	pt_BR
dc.title	Thermal dimensional reduction and black hole evaporation	pt_BR
dc.type	Artigo	pt_BR
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