Four dimensional Einstein-power-Maxwell black hole solutions in scale-dependent gravity

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dc.contributor.authorRincon, Angel
dc.contributor.authorContreras, Ernesto
dc.contributor.authorBargueno, Pedro
dc.contributor.authorKoch, Benjamin
dc.contributor.authorPanotopoulos, Grigoris
dc.date.accessioned2025-01-20T23:52:11Z
dc.date.available2025-01-20T23:52:11Z
dc.date.issued2021
dc.description.abstractIn the present work, we extend and generalize our previous work regarding the scale dependence applied to black holes in the presence of non-linear electrodynamics (Rincon et al., 2017). The starting point for this study is the Einstein-power-Maxwell theory with a vanishing cosmological constant in (3+1) dimensions, assuming a scale dependence of both the gravitational and the electromagnetic coupling. We further examine the corresponding thermodynamic properties and how these quantities experience deviations from their classical counterparts. We solve the effective Einstein's field equations using the "null energy condition'' to obtain analytical solutions. The implications of quantum corrections are also briefly discussed. Finally, we analyze our solutions and compare them to related results in the literature. (C) 2021 Elsevier B.V. All rights reserved.
dc.fuente.origenWOS
dc.identifier.doi10.1016/j.dark.2021.100783
dc.identifier.eissn2212-6864
dc.identifier.urihttps://doi.org/10.1016/j.dark.2021.100783
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/94897
dc.identifier.wosidWOS:000630235100041
dc.language.isoen
dc.revistaPhysics of the dark universe
dc.rightsacceso restringido
dc.subjectBlack holes
dc.subject3+1 dimensions
dc.subjectScale-dependence
dc.subjectExact Solutions
dc.subjectNon-linear electrodynamics
dc.titleFour dimensional Einstein-power-Maxwell black hole solutions in scale-dependent gravity
dc.typeartículo
dc.volumen31
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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