Rotating five-dimensional electrically charged Bardeen regular black holes
arXiv:2005.00307 · doi:10.1088/1361-6382/ab8eb7
Abstract
We derive a rotating counterpart of the five-dimensional electrically charged Bardeen regular black holes spacetime by employing the Giampieri algorithm on static one. The associated nonlinear electrodynamics source is computed in order to justify the rotating solution. We thoroughly discuss the energy conditions and the other properties of the rotating spacetime. The black hole thermodynamics of the rotating spacetime is also presented. In particular, the thermodynamic quantities such as the Hawking temperature and the heat capacity are calculated and plotted to see the thermal behavior. The Hawking temperature profile of the black hole implies that the regular black holes are thermally colder than its singular counterpart. On the other hand, we find that the heat capacity has two branches: the negative branch corresponds to the unstable phase and the positive branch corresponds to that of the stable phase for a suitable choice of the physical parameters characterizing the black holes.
24 pages, 8 figures, accepted for publication in CQG
References in corpus (8)
- First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
- First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring
- Rotating regular black holes
- Regular black holes with a nonlinear electrodynamics source
- Generating rotating regular black hole solutions without complexification
- Rotating Regular Black Hole Solution
- Janis-Newman algorithm: generating rotating and NUT charged black holes
- Generating five-dimensional Myers-Perry black hole solution using quaternions