Correspondence between quasinormal modes and the shadow radius in a wormhole spacetime

DOI10.1007/s10714-021-02856-6zbMath1483.83050arXiv2007.16019OpenAlexW3200206928MaRDI QIDQ2059762

Kimet Jusufi

Publication date: 14 December 2021

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2007.16019

zbMATH Keywords

shadowwormholesquasinormal modes

Mathematics Subject Classification ID

Black holes (83C57) Galactic and stellar dynamics (85A05) Motion of the gyroscope (70E05)

Related Items (3)

Tideless traversable wormholes surrounded by cloud of strings in f(R) gravity ⋮ Wormholes without exotic matter: quasinormal modes, echoes and shadows ⋮ Gravitational Lensing by Traversable Wormholes Supported by Three‐Form Fields

Cites Work

• How to tell the shape of a wormhole by its quasinormal modes
• On gravitational lensing by symmetric and asymmetric wormholes
• Are eikonal quasinormal modes linked to the unstable circular null geodesics?
• Gravitational Field of a Particle Falling in a Schwarzschild Geometry Analyzed in Tensor Harmonics
• Stability of a Schwarzschild Singularity
• Quasinormal modes of bumblebee wormhole
• GRAVITATIONAL LENSING BY WORMHOLES
• BENDING OF LIGHT IN ELLIS WORMHOLE GEOMETRY
• Causality and Multiply Connected Space-Time
• Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
• Deflection angle of light by wormholes using the Gauss–Bonnet theorem
• Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope
• Shadow images of Kerr-like wormholes
• The Particle Problem in the General Theory of Relativity
• Geons
• Upper bound on the radii of black-hole photonspheres

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