2019/02/27 by E. Contreras, Ernesto Contreras, Ángel Rincón +3
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Black hole thermodynamics #Constant (computer programming) #Constant curvature #Cosmology and Gravitation Theories #Curvature #Entropy (arrow of time) #Event horizon #Extremal black hole #Gravitation #Noncommutative and Quantum Gravity Theories #gr-qc #hep-th
paper · pdf · doi:10.1140/epjc/s10052-020-7936-4
9 pages. Some comments added
openalex created_date 2019/02/21 · arxiv created 2019/02/27 · openalex publication_date 2020/05/01 · arxiv updated 2020/05/20 · openalex updated_date 2026/08/05
Abstract 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.