Quasi-normal modes of hairy scalar tensor black holes: odd parity
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Publication:5161800
DOI10.1088/1361-6382/ab839bzbMath1478.83178arXiv1911.07593OpenAlexW3103952529WikidataQ113390344 ScholiaQ113390344MaRDI QIDQ5161800
Publication date: 1 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1911.07593
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Gravitational waves (83C35) Matrix models and tensor models for quantum field theory (81T32)
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Cites Work
- Quasinormal modes of the electrically charged dilaton black hole
- Effective field theory of black hole quasinormal modes in scalar-tensor theories
- Challenges to self-acceleration in modified gravity from gravitational waves and large-scale structure
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- Black hole stability under odd-parity perturbations in Horndeski gravity
- Stability of a Schwarzschild Singularity
- Quasinormal modes of black holes and black branes
- On an expansion method for black hole quasinormal modes and Regge poles
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Black-hole spectroscopy: testing general relativity through gravitational-wave observations
- Quasinormal modes: the characteristic `sound' of black holes and neutron stars
- Quasi-normal modes of stars and black holes
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