Geodesics and optical properties of a rotating black hole in Randall-Sundrum brane with a cosmological constant
From MaRDI portal
Publication:6496438
DOI10.1016/J.CJPH.2022.06.017MaRDI QIDQ6496438
Publication date: 3 May 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
Quantum field theory; related classical field theories (81Txx) General relativity (83Cxx) Unified, higher-dimensional and super field theories (83Exx)
Cites Work
- Unnamed Item
- The hierarchy problem and new dimensions at a millimeter
- Heterotic and type I string dynamics from eleven dimensions
- Eleven-dimensional supergravity on a manifold with boundary
- Shadow of a black hole surrounded by dark matter
- The cosmological constant and dark energy
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Large Mass Hierarchy from a Small Extra Dimension
- Quasinormal modes: the characteristic `sound' of black holes and neutron stars
- The apparent shape of a rotating charged black hole, closed photon orbits and the bifurcation set A 4
- Shadow cast and deflection angle of Kerr-Newman-Kasuya spacetime
- Curvature radius and Kerr black hole shadow
- Toward the event horizon—the supermassive black hole in the Galactic Center
This page was built for publication: Geodesics and optical properties of a rotating black hole in Randall-Sundrum brane with a cosmological constant
