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dc.contributor.authorEstrada, Milko
dc.contributor.authorTello Ortiz, Francisco
dc.date.accessioned2021-12-02T15:22:41Z
dc.date.available2021-12-02T15:22:41Z
dc.date.issued2021-06-28
dc.identifier.issn1286-4854
dc.identifier.other10.1209/0295-5075/ac0ed0
dc.identifier.urihttps://hdl.handle.net/20.500.12536/1449
dc.description.abstractWe provide a new regular black hole solution in (2 + 1) dimensions with presence of matter fields in the energy momentum tensor. The inclusion of our proposed energy density plus a negative cosmological constant allows that the solution can have both flat as de–Sitter or Anti de–Sitter core. This latter is a proper characteristic of our solution, because other models of regular black holes have only a single type of core. Since the first law of thermodynamics for regular black holes is modified by the presence of the matter fields, we provide a new version of the first law, where a local definition of the variation of energy is defined, and, where the entropy and temperature are consistent with the previously known in literature. At the hypothetical limit when the horizon radius r + → ∞ the usual first law dM = T dS is recovered. The effectiveness of the formalism used to compute the mass of our regular black holes in (2+ 1) suggests the potential applicability of this method to calculate the mass of other models of regular black holes in d ≥ 4 dimensions.es_ES
dc.language.isoenes_ES
dc.sourceEurophysics letterses_ES
dc.titleA new model of regular black hole in (2 + 1) dimensionses_ES
dc.typeArtículo de revistaes_ES
uvm.escuelaEscuela de Ingeniería y Negocioses_ES
uvm.indexScopuses_ES


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