Effective field theory of black hole perturbations with timelike scalar profile: formulation
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Publication:5104217
DOI10.1088/1475-7516/2022/09/010OpenAlexW4226145807MaRDI QIDQ5104217
Vicharit Yingcharoenrat, Shinji Mukohyama
Publication date: 9 September 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2204.00228
Black holes (83C57) Symmetry breaking in quantum theory (81R40) Perturbations in context of PDEs (35B20) Inhomogeneous linear forms (11J20) Matrix models and tensor models for quantum field theory (81T32) Effective quantum field theories (81T12)
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Cites Work
- Unnamed Item
- Starting the universe: stable violation of the null energy condition and non-standard cosmologies
- Effective field theory of black hole quasinormal modes in scalar-tensor theories
- Disforming the Kerr metric
- On the vanishing of Love numbers for Kerr black holes
- Effective field theory for the perturbations of a slowly rotating black hole
- Exact black hole solutions in shift symmetric scalar-tensor theories
- Black holes and stars in Horndeski theory
- Mach's Principle and a Relativistic Theory of Gravitation
- Nonlinear effective theory of dark energy
- Gravitational wave decay into dark energy
- Stealth dark energy in scordatura DHOST theory
- Static response and Love numbers of Schwarzschild black holes
- On rotating black holes in DHOST theories
- Generalized Regge-Wheeler equation from Effective Field Theory of black hole perturbations with a timelike scalar profile
- Inflation with 0 ≤ c s ≤ 1
- Resonant decay of gravitational waves into dark energy
- Weakly-coupled stealth solution in scordatura degenerate theory
- Hairy black holes in DHOST theories: exploring disformal transformation as a solution generating method
- Dark-energy instabilities induced by gravitational waves
- General Relativity solutions with stealth scalar hair in quadratic higher-order scalar-tensor theories
- Black hole perturbations in DHOST theories: master variables, gradient instability, and strong coupling
- Dark energy and modified gravity in degenerate higher-order scalar–tensor (DHOST) theories: A review
- The effective field theory of vector-tensor theories