Weakly-coupled stealth solution in scordatura degenerate theory

DOI10.1088/1475-7516/2020/01/030zbMath1489.83057arXiv1912.00378OpenAlexW2991251461MaRDI QIDQ5067814

Shinji Mukohyama, Hayato Motohashi

Publication date: 4 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1912.00378

zbMATH Keywords

modified gravityGR black holes

Mathematics Subject Classification ID

Black holes (83C57) Degenerate elliptic equations (35J70) Quantum field theory on curved space or space-time backgrounds (81T20) Phase transitions (general) in equilibrium statistical mechanics (82B26) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Dispersion theory, dispersion relations arising in quantum theory (81U30) Effective quantum field theories (81T12)

Related Items (26)

On rotating black holes in DHOST theories ⋮ 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 ⋮ Positivity vs. Lorentz-violation: an explicit example ⋮ Inflation with 0 ≤ c _s ≤ 1 ⋮ Hairy black holes in DHOST theories: exploring disformal transformation as a solution generating method ⋮ General Relativity solutions with stealth scalar hair in quadratic higher-order scalar-tensor theories ⋮ Scale-dependence in DHOST inflation ⋮ Black hole perturbations in higher-order scalar–tensor theories: initial value problem and dynamical stability ⋮ Stability of hairy black holes in shift-symmetric scalar-tensor theories via the effective field theory approach ⋮ On the effective metric of axial black hole perturbations in DHOST gravity ⋮ The effective field theory approach to the strong coupling issue in f(T) gravity ⋮ Effective field theory of black hole perturbations with timelike scalar profile: formulation ⋮ Electromagnetically and gravitationally stealth fields ⋮ Approximately stealth black hole in higher-order scalar-tensor theories ⋮ Effective description of generalized disformal theories ⋮ Quasinormal modes from EFT of black hole perturbations with timelike scalar profile ⋮ Axial perturbations of black holes in scalar-tensor gravity: near-horizon behaviour ⋮ Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land ⋮ Black holes in the quadratic-order extended vector–tensor theories ⋮ Disforming the Kerr metric ⋮ Stealth black hole perturbations in kinetic gravity braiding ⋮ The effective field theory of vector-tensor theories ⋮ Self-tuning kinetic gravity braiding: cosmological dynamics, shift symmetry, and the tadpole ⋮ Stealth dark energy in scordatura DHOST theory ⋮ Partial UV completion of P(X) from a curved field space

Cites Work

• Starting the universe: stable violation of the null energy condition and non-standard cosmologies
• Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order
• Ghost-free theories with arbitrary higher-order time derivatives
• General relativity solutions in modified gravity
• Exact black hole solutions in shift symmetric scalar-tensor theories
• Gravitational wave decay into dark energy
• Effective description of higher-order scalar-tensor theories
• Hairy black holes in DHOST theories: exploring disformal transformation as a solution generating method
• Perturbations of a rotating black hole in DHOST theories
• Effective field theory approach to modified gravity including Horndeski theory and Hořava–Lifshitz gravity
• A unifying description of dark energy

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