Topology of the charged AdS black hole in restricted phase space
arXiv:2406.08793 · doi:10.1088/1674-1137/ad57b0
Abstract
The local topological properties of black hole systems can be expressed by the winding numbers as the defects. As so far, AdS black hole thermodynamics is often depicted by the dual parameters of in the extended phase space, while there is several study on the black hole thermodynamics in the restricted phase space. In this paper, we analyze the topological properties of the charged AdS black holes in the restricted phase space under the higher dimensions and higher order curvature gravities frame. The results show that the topological number of the charged black hole in the same canonical ensembles is a constant and is independent of the concrete dual thermodynamical parameters. However, the topological number in the grand canonical ensemble is different from that in the canonical ensemble for the same black hole system. Furthermore, these results are independent of the dimension , the highest order of the Lanczos-Lovelock densities.
References in corpus (11)
- Multiple Reentrant Phase Transitions and Triple Points in Lovelock Thermodynamics
- Black Hole Solutions as Topological Thermodynamic Defects
- Superfluid Black Holes
- Topology of black hole thermodynamics
- Topological Charge and Black Hole Photon Spheres
- Classifying topology of consistent thermodynamics of the four-dimensional neutral Lorentzian NUT-charged spacetimes
- Restricted phase space thermodynamics for AdS black holes via holography
- Thermodynamics of Kerr-AdS black holes in the restricted phase space
- Van der Waals criticality in AdS black holes: a phenomenological study
- Thermogeometric phase transition in a unified framework
- Thermodynamics for higher dimensional rotating black holes with variable Newton constant