General approach on shadow radius and photon spheres in asymptotically flat spacetimes and the impact of mass-dependent variations
From MaRDI portal
Publication:6561127
DOI10.1016/j.physletb.2024.138758MaRDI QIDQ6561127
Ali Övgün, Vitalii D. Vertogradov
Publication date: 24 June 2024
Published in: Physics Letters B (Search for Journal in Brave)
Cites Work
- Shadows and strong gravitational lensing: a brief review
- Calculating black hole shadows: review of analytical studies
- Strong gravitational lensing and shadow constraint from M87* of slowly rotating Kerr-like black hole
- Spherical null geodesics of rotating Kerr black holes
- The geometry of photon surfaces.
- Quintessence and black holes
- Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope
- Scalar–tensor–vector gravity theory
- Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors
- Shadows of Kerr–Vaidya-like black holes
- Probing Schwarzschild-like black holes in metric-affine bumblebee gravity with accretion disk, deflection angle, greybody bounds, and neutrino propagation
Related Items (3)
Probing barrow entropy models with future event horizon as IR cutoff ⋮ Viewing the holographic image of the Bardeen-AdS black hole ⋮ Exact regular black hole solutions with de Sitter cores and Hagedorn fluid
This page was built for publication: General approach on shadow radius and photon spheres in asymptotically flat spacetimes and the impact of mass-dependent variations