Five-dimensional scale-dependent black holes with constant curvature and Solv horizons

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Título: Five-dimensional scale-dependent black holes with constant curvature and Solv horizons
Autor/es: Contreras, Ernesto | Rincón, Ángel | Bargueño, Pedro
Grupo/s de investigación o GITE: Astrofísica Relativista
Centro, Departamento o Servicio: Universidad de Alicante. Departamento de Física Aplicada
Palabras clave: Five-dimensional | Scale-dependent | Black holes | Constant curvature | Solv horizons
Área/s de conocimiento: Física Aplicada
Fecha de publicación: 6-may-2020
Editor: Springer Nature
Cita bibliográfica: The European Physical Journal C. 2020, 80:367. doi:10.1140/epjc/s10052-020-7936-4
Resumen: In this work, we investigate five-dimensional scale-dependent black hole solutions by modelling their event horizon with some of the eight Thurston three-dimensional geometries. Specifically, we construct constant curvature scale-dependent black holes and also the more exotic scale-dependent Solv black hole. These new solutions are obtained by promoting both the gravitational and the cosmological couplings to r-dependent functions, in light of a particular description of the effective action inspired by the high energy philosophy. Interestingly, the so-called running parameter, together with the topology of the event horizon, control the asymptotic structure of the solutions found. Finally, differences in both the entropy and the temperature between the classical and the scale-dependent Solv black hole are briefly commented.
Patrocinador/es: A. R. was supported by the CONICYT-PCHA/Doctorado Nacional/2015-21151658. P. B. is funded by the Beatriz Galindo contract BEAGAL 18/00207 (Spain).
URI: http://hdl.handle.net/10045/107262
ISSN: 1434-6044 (Print) | 1434-6052 (Online)
DOI: 10.1140/epjc/s10052-020-7936-4
Idioma: eng
Tipo: info:eu-repo/semantics/article
Derechos: Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
Revisión científica: si
Versión del editor: https://doi.org/10.1140/epjc/s10052-020-7936-4
Aparece en las colecciones:INV - Astrofísica Relativista - Artículos de Revistas

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