Wormholes without exotic matter: quasinormal modes, echoes and shadows
DOI10.1088/1475-7516/2021/10/010zbMath1486.83019arXiv2107.05977OpenAlexW3202342375MaRDI QIDQ5061897
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Publication date: 14 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2107.05977
Black holes (83C57) String and superstring theories in gravitational theory (83E30) Diffraction, scattering (78A45) Electromagnetic fields in general relativity and gravitational theory (83C50) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Gravitational waves (83C35) Einstein-Maxwell equations (83C22)
Related Items (8)
Cites Work
- Quasinormal modes of black holes in 5D Gauss-Bonnet gravity combined with non-linear electrodynamics
- A novel gravitational lensing feature by wormholes
- How to tell the shape of a wormhole by its quasinormal modes
- Correspondence between quasinormal modes and the shadow radius in a wormhole spacetime
- A note on ``Traversable wormholes in Einstein-Dirac-Maxwell theory
- Particle-like ultracompact objects in Einstein-scalar-Gauss-Bonnet theories
- Wormholes as black hole foils
- Possible wormholes in a brane world
- Wormhole potentials and throats from quasi-normal modes
- Interaction of Neutrinos and Gravitational Fields
- Bound states of the Dirac equation on Kerr spacetime
- An Alternative to Compactification
- Weak deflection angle by Casimir wormhole using Gauss-Bonnet theorem and its shadow
- Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
- Shadow images of Kerr-like wormholes
- Quasinormal modes of Kerr–de Sitter black holes via the Heun function
- Massive particles in the Einstein–Lovelock–anti-de Sitter black hole spacetime
- Instability of wormholes supported by a ghost scalar field: I. Linear stability analysis
- Quasi-normal modes of stars and black holes
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