Ultra compact stars: reconstructing the perturbation potential

DOI10.1088/1361-6382/aa82dezbMath1372.85001arXiv1704.07517OpenAlexW2609430912WikidataQ63410610 ScholiaQ63410610MaRDI QIDQ5369364

Kostas D. Kokkotas, Sebastian H. Völkel

Publication date: 17 October 2017

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1704.07517

zbMATH Keywords

inverse problemquasi-normal modesgravitational wavesWKBcompact stars

Mathematics Subject Classification ID

Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Galactic and stellar dynamics (85A05) Gravitational waves (83C35) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (8)

Wormhole potentials and throats from quasi-normal modes ⋮ The quasinormal modes of quasinormal modes ⋮ Quasinormal modes and greybody factors of \(f(R)\) gravity minimally coupled to a cloud of strings in \({2+1}\) dimensions ⋮ How to tell the shape of a wormhole by its quasinormal modes ⋮ Echoes from the scattering of wavepackets on wormholes ⋮ Extreme gravity tests with gravitational waves from compact binary coalescences: II: Ringdown ⋮ Echoes from hairy black holes ⋮ On gravitational echoes from ultracompact exotic stars

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