Distinct topological configurations of equatorial timelike circular orbit for spherically symmetric (hairy) black holes
From MaRDI portal
Publication:6175019
DOI10.1088/1475-7516/2023/07/049arXiv2301.04786MaRDI QIDQ6175019
Publication date: 17 August 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2301.04786
Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15) Equations of motion in general relativity and gravitational theory (83C10)
Cites Work
- Gravitational lensing in spherically symmetric static spacetimes with centrifugal force reversal
- Shadows and strong gravitational lensing: a brief review
- Quasinormal modes of black holes with multiple photon spheres
- The geometry of photon surfaces
- Area bound for a surface in a strong gravity region
- Spontaneous scalarisation of charged black holes: coupling dependence and dynamical features
This page was built for publication: Distinct topological configurations of equatorial timelike circular orbit for spherically symmetric (hairy) black holes