Quasi-normal modes of loop quantum black holes formed from gravitational collapse
From MaRDI portal
Publication:6636423
DOI10.1088/1475-7516/2024/10/070MaRDI QIDQ6636423
Publication date: 12 November 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Cites Work
- Title not available (Why is that?)
- Extreme gravity tests with gravitational waves from compact binary coalescences: II: Ringdown
- Über das Gravitationsfeld eines Massenpunktes nach der \textit{Einstein}schen Theorie.
- How to tell the shape of a wormhole by its quasinormal modes
- Wormhole potentials and throats from quasi-normal modes
- Stability of a Schwarzschild Singularity
- Quasinormal modes of black holes and black branes
- Black-hole entropy in loop quantum gravity
- Constraints on self-dual black hole in loop quantum gravity with S0-2 star in the galactic center
- Hořava gravity at a Lifshitz point: A progress report
- A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes
- Speeds of propagation in classical and relativistic extended thermodynamics
- Gravitational waves from eccentric extreme mass-ratio inspirals as probes of scalar fields
- Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory
- Scalar quasi-normal modes of accelerating Kerr-Newman-AdS black holes
- On the improved dynamics approach in loop quantum black holes
- Scalar fields around a rotating loop quantum gravity black hole: waveform, quasi-normal modes and superradiance
- Analytical models of supermassive black holes in galaxies surrounded by dark matter halos
- Scalar quasi-normal modes of a loop quantum black hole
This page was built for publication: Quasi-normal modes of loop quantum black holes formed from gravitational collapse
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6636423)
