Stability analysis of geodesics and quasinormal modes of a dual stringy black hole via Lyapunov exponents
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Publication:2059745
DOI10.1007/s10714-021-02845-9zbMath1483.83045arXiv2108.05772OpenAlexW3191649910MaRDI QIDQ2059745
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/2108.05772
Black holes (83C57) Characteristic and Lyapunov exponents of ordinary differential equations (34D08) Electromagnetic fields in general relativity and gravitational theory (83C50) Geodesics in global differential geometry (53C22) Orbital mechanics (70M20)
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- Null geodesics in a magnetically charged stringy black hole spacetime
- Are eikonal quasinormal modes linked to the unstable circular null geodesics?
- On black hole structures in scalar–tensor theories of gravity
- Geodesic motion in a charged 2D stringy black hole spacetime
- The dark matter problem from f(R) gravity viewpoint
- Quasinormal modes of black holes and black branes
- String Theory
- Lyapunov timescales and black hole binaries
- Rotating charged black hole solution in heterotic string theory
- Null geodesics and observables around the Kerr–Sen black hole
- A Relativist's Toolkit
- Chaos in static axisymmetric spacetimes: I. Vacuum case
- Quasinormal modes: the characteristic `sound' of black holes and neutron stars
- Geodesic stability and quasi normal modes via Lyapunov exponent for Hayward black hole
- Quasi-normal modes and the area spectrum of a near extremal de Sitter black hole with conformally coupled scalar field
- Bardeen–de Sitter black holes
- Black hole mergers and unstable circular orbits
- General Relativity
- Quasi-normal modes of stars and black holes
