Effective field theory of black hole perturbations in vector-tensor gravity
From MaRDI portal
Publication:6558398
DOI10.1088/1475-7516/2024/03/012zbMATH Open1543.83115MaRDI QIDQ6558398
Katsuki Aoki, Vicharit Yingcharoenrat, Kazufumi Takahashi, Shinji Mukohyama, M. A. Gorji
Publication date: 19 June 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Cosmic acceleration from abelian symmetry breaking
- Derivative self-interactions for a massive vector field
- L'univers en expansion.
- Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
- Black holes in the generalized Proca theory
- General relativity solutions in modified gravity
- Beyond generalized Proca theories
- Cosmological constant -- the weight of the vacuum
- Exact black hole solutions in shift symmetric scalar-tensor theories
- Black holes and Abelian symmetry breaking
- The cosmological constant and dark energy
- DYNAMICS OF DARK ENERGY
- Black holes in vector-tensor theories
- A class of minimally modified gravity theories
- Extended mimetic gravity: Hamiltonian analysis and gradient instabilities
- Nonlinear effective theory of dark energy
- Extended cuscuton: formulation
- The effective theory of shift-symmetric cosmologies
- Extended vector-tensor theories
- Minimally modified gravity: a Hamiltonian construction
- Stealth dark energy in scordatura DHOST theory
- Existence and instability of hairy black holes in shift-symmetric Horndeski theories
- Generalized Regge-Wheeler equation from Effective Field Theory of black hole perturbations with a timelike scalar profile
- Inflation with 0 ≤ c s ≤ 1
- Nonlinear definition of the shadowy mode in higher-order scalar-tensor theories
- Weakly-coupled stealth solution in scordatura degenerate theory
- 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
- A theory of type-II minimally modified gravity
- Effective field theory of gravitating continuum: solids, fluids, and aether unified
- Effective field theory of black hole perturbations with timelike scalar profile: formulation
- Black holes in the quadratic-order extended vector–tensor theories
- Dark energy and modified gravity in degenerate higher-order scalar–tensor (DHOST) theories: A review
- A unifying description of dark energy
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- The cosmological constant problem
- Mimetic gravity as DHOST theories
- The effective field theory of vector-tensor theories
- Generalized disformal Horndeski theories: Cosmological perturbations and consistent matter coupling
- Stability of hairy black holes in shift-symmetric scalar-tensor theories via the effective field theory approach
- Quasinormal modes and grey-body factors of regular black holes with a scalar hair from the Effective Field Theory
- Effective description of generalized disformal theories
- Some disquisitions on cosmological 2-form dualities
- Quasinormal modes from EFT of black hole perturbations with timelike scalar profile
Related Items (2)
CMB spectrum in unified EFT of dark energy: scalar-tensor and vector-tensor theories ⋮ Tidal Love numbers from EFT of black hole perturbations with timelike scalar profile
This page was built for publication: Effective field theory of black hole perturbations in vector-tensor gravity
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6558398)