Black hole perturbations in vector-tensor theories: the odd-mode analysis
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Publication:5022091
DOI10.1088/1475-7516/2018/02/048OpenAlexW3098503679WikidataQ57655971 ScholiaQ57655971MaRDI QIDQ5022091
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Publication date: 18 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1801.01787
Related Items
Odd-parity perturbations in the most general scalar–vector–tensor theory ⋮ Instability of hairy black holes in regularized 4-dimensional Einstein-Gauss-Bonnet gravity ⋮ To half-be or not to be? ⋮ Coupled vector Gauss-Bonnet theories and hairy black holes ⋮ Odd-parity perturbations of the wormhole-like geometries and quasi-normal modes in Einstein-Æther theory ⋮ Positivity bounds in vector theories
Cites Work
- Cosmic acceleration from abelian symmetry breaking
- Derivative self-interactions for a massive vector field
- \(f(R)\) theories
- Black holes and solitons in an extended Proca theory
- Black holes with vector hair
- Event horizon in static scalar-vacuum space-times
- Exact black hole solutions in shift symmetric scalar-tensor theories
- Black holes and Abelian symmetry breaking
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- A small cosmological constant from Abelian symmetry breaking
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- Stability of a Schwarzschild Singularity
- DYNAMICS OF DARK ENERGY
- Modified Gravity Models of Dark Energy
- Linear stability of Schwarzschild under perturbations which are non-vanishing on the bifurcation 2-sphere
- Black holes in vector-tensor theories
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- Black holes and neutron stars in vector Galileons
