Dark energy in Horndeski theories after GW170817: A review

DOI10.1142/S0218271819420057zbMath1423.83058arXiv1809.08735WikidataQ128605841 ScholiaQ128605841MaRDI QIDQ5242594

Ryotaro Kase, Shinji Tsujikawa

Publication date: 12 November 2019

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1809.08735

zbMATH Keywords

cosmologymodified gravitydark energy

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)

Related Items (43)

Shift-symmetric Horndeski gravity in the asymptotic-safety paradigm ⋮ General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter ⋮ Dark energy loopholes some time after GW170817 ⋮ Effective field theory of dark energy: a review ⋮ Cosmic acceleration from string induced Galileons ⋮ A data-driven reconstruction of Horndeski gravity via the Gaussian processes ⋮ J-PAS: forecasts on interacting vacuum energy models ⋮ Coupled vector dark energy ⋮ Quantum gravity and gravitational-wave astronomy ⋮ Limitations on Standard Sirens tests of gravity from screening ⋮ Tailoring cosmologies in cubic shift-symmetric Horndeski gravity ⋮ Simple traversable wormholes violating energy conditions only near the Planck scale ⋮ hi_class background evolution, initial conditions and approximation schemes ⋮ Probing cosmological fields with gravitational wave oscillations ⋮ Unveiling the Galileon in a three-body system: scalar and gravitational wave production ⋮ Scaling solutions and weak gravity in dark energy with energy and momentum couplings ⋮ Horndeski under the quantum loupe ⋮ Limited modified gravity ⋮ Is local H₀at odds with dark energy EFT? ⋮ Confronting quantum-corrected teleparallel cosmology with observations ⋮ Neutron stars in modified teleparallel gravity ⋮ Classical and quantum cosmology of Fab Four John theories ⋮ Second-order teleparallel gauge theory ⋮ An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations ⋮ Probing modified gravity with integrated Sachs-Wolfe CMB and galaxy cross-correlations ⋮ Stability of Schwarzshild black holes in quadratic gravity with Weyl curvature domination ⋮ Constraining Horndeski theory with gravitational waves from coalescing binaries ⋮ Cosmological stability in \(f(\phi, \mathcal{G})\) gravity ⋮ On two body gravitational scattering within perturbative gravity ⋮ Symmetry restoration in the vicinity of neutron stars with a nonminimal coupling ⋮ Einstein Yang–Mills Higgs dark energy revisited ⋮ Gravastar model in Randall–Sundrum braneworld ⋮ Well-tempered Minkowski solutions in teleparallel Horndeski theory ⋮ Dark energy beyond quintessence: constraints from the swampland ⋮ The Lanczos equation on light-like hypersurfaces in a cosmologically viable class of kinetic gravity braiding theories ⋮ Stealth black hole perturbations in kinetic gravity braiding ⋮ Dark sector evolution in Horndeski models ⋮ Instability of compact stars with a nonminimal scalar-derivative coupling ⋮ Spin precession as a new window into disformal scalar fields ⋮ Self-tuning kinetic gravity braiding: cosmological dynamics, shift symmetry, and the tadpole ⋮ Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids ⋮ Modified gravity in the interior of population II stars ⋮ Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology

Cites Work

• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• Variational aspects of relativistic field theories, with application to perfect fluids
• \(1/R\) gravity and scalar-tensor gravity
• Cosmological evolution of the rolling tachyon
• Cosmological constant -- the weight of the vacuum
• A quintessential axion
• The string dilaton and a least coupling principle
• A new type of isotropic cosmological models without singularity
• Manifestly Local Theory of Vacuum Energy Sequestering
• The cosmological constant and dark energy
• Singularity Problem with<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Models for Dark Energy
• Are<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>Dark Energy Models Cosmologically Viable?
• Mach's Principle and a Relativistic Theory of Gravitation
• DYNAMICS OF DARK ENERGY
• The Scalar-Tensor Theory of Gravitation
• CURVATURE QUINTESSENCE
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• The Einstein Tensor and Its Generalizations
• 4D gravity on a brane in 5D Minkowski space
• \(k\)-inflation

This page was built for publication: Dark energy in Horndeski theories after GW170817: A review