How to tell the shape of a wormhole by its quasinormal modes

DOI10.1016/j.physletb.2018.07.025zbMath1411.83016arXiv1805.04718OpenAlexW2801951622MaRDI QIDQ1738471

Roman A. Konoplya

Publication date: 18 April 2019

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1805.04718

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (10)

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 ⋮ Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory ⋮ Thermodynamical properties of an ideal gas in a traversable wormhole ⋮ On the linear instability of the Ellis-Bronnikov-Morris-Thorne wormhole ⋮ Effective field theory of black hole quasinormal modes in scalar-tensor theories ⋮ Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations ⋮ Ringing of the regular black-hole/wormhole transition ⋮ Correspondence between quasinormal modes and the shadow radius in a wormhole spacetime

Cites Work

• Unnamed Item
• Wormholes, warp drives and energy conditions
• Perturbations and quasi-normal modes of black holes in Einstein-aether theory
• Detection of gravitational waves from black holes: is there a window for alternative theories?
• Are eikonal quasinormal modes linked to the unstable circular null geodesics?
• Wormholes as black hole foils
• Wormhole potentials and throats from quasi-normal modes
• Ultra compact stars: reconstructing the perturbation potential
• Quasi-normal modes of stars and black holes

This page was built for publication: How to tell the shape of a wormhole by its quasinormal modes