Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory

Abstract

Gravitational waves (GW) are generally affected by modification of a gravity theory during propagation in cosmological distance. We numerically perform a quantitative analysis on Horndeski theory at cosmological scale to constrain the Horndeski theory by GW observations in model-independent way. We formulate a parameterization for a numerical simulation based on the Monte Carlo method and obtain the classification of the models that agrees with cosmic accelerating expansion within observational errors of the Hubble parameter. As a result, we find that a large group of the models in the Horndeski theory that mimic cosmic expansion of $\Lambda$CDM model can be excluded from the simultaneous detection of a GW and its electromagnetic transient counterpart. Based on our result and the latest detection of GW170817 and GRB170817A, we conclude that the subclass of Horndeski theory including arbitrary functions $G_4$ and $G_5$ can hardly explain cosmic accelerating expansion without fine-tuning.

arXiv comment10 pages, 6 figures, PRD submitted version, PRD published

References in corpus (49)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Observation of Gravitational Waves from a Binary Black Hole Merger
• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• The Cosmological Constant and Dark Energy
• f(R) theories
• Multi-messenger Observations of a Binary Neutron Star Merger
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• The galileon as a local modification of gravity
• Essentials of k-essence
• Chameleon Cosmology
• Kinetically Driven Quintessence
• A gravitational-wave standard siren measurement of the Hubble constant
• Generalized G-inflation: Inflation with the most general second-order field equations
• Covariant Galileon
• Dark Energy after GW170817: dead ends and the road ahead
• Dark Energy after GW170817 and GRB170817A
• Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
• Imperfect Dark Energy from Kinetic Gravity Braiding
• The Large Scale Structure of f(R) Gravity
• The Effective Field Theory of Dark Energy
• Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
• Essential Building Blocks of Dark Energy
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Breaking a Dark Degeneracy with Gravitational Waves
• Anisotropic stress as signature of non-standard propagation of gravitational waves
• Effective Field Theory of Cosmic Acceleration: an implementation in CAMB
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• Lower Bound on the Propagation Speed of Gravity from Gravitational Cherenkov Radiation
• Speed of Gravitational Waves and the Fate of Scalar-Tensor Gravity
• Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory
• hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
• Nonlinear structure formation in the Cubic Galileon gravity model
• Effective Theory of Interacting Dark Energy
• Constraints on Shift-Symmetric Scalar-Tensor Theories with a Vainshtein Mechanism from Bounds on the Time Variation of G
• Measuring Speed of Gravitational Waves by Observations of Photons and Neutrinos from Compact Binary Mergers and Supernovae
• A comparison of Einstein-Boltzmann solvers for testing General Relativity
• KIC 10080943: An eccentric binary system containing two pressure- and gravity-mode hybrid pulsators
• Challenges in Connecting Modified Gravity Theory and Observations
• Gravity at the horizon: on relativistic effects, CMB-LSS correlations and ultra-large scales in Horndeski's theory
• Parametrizing modified gravity for cosmological surveys
• Measurement of Hubble constant with stellar-mass binary black holes
• Constraining the propagation speed of gravitational waves with compact binaries at cosmological distances
• The parameter space of Cubic Galileon models for cosmic acceleration

Cited by in corpus (115)

• Science with the Einstein Telescope: a comparison of different designs
• Cosmology with the Laser Interferometer Space Antenna
• New Horizons for Fundamental Physics with LISA
• Dark Energy and Modified Gravity in Degenerate Higher-Order Scalar-Tensor (DHOST) theories: a review
• Black holes with scalar hair in light of the Event Horizon Telescope
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• Modified gravitational-wave propagation and standard sirens
• Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy
• Limits on the number of spacetime dimensions from GW170817
• Evolution of Einstein-scalar-Gauss-Bonnet gravity using a modified harmonic formulation
• No-Hair Theorem in the Wake of Event Horizon Telescope
• The Gravitational-Wave Physics II: Progress
• Standard sirens with a running Planck mass
• Waveform of gravitational waves in the general parity-violating gravities
• Alive and well: mimetic gravity and a higher-order extension in light of GW170817
• Self-accelerating universe in scalar-tensor theories after GW170817
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• The Science of the Einstein Telescope
• Probing observational bounds on scalar-tensor theories from standard sirens
• Cosmology and dark energy from joint gravitational wave-GRB observations
• Cosmological parameter constraints for Horndeski scalar-tensor gravity
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• Gravitational wave lensing beyond general relativity: birefringence, echoes and shadows
• Parity-violating gravity and GW170817
• Direct detection of dark energy: the XENON1T excess and future prospects
• Constraints on scalar-tensor theory of gravity by the recent observational results on gravitational waves
• Direct detection of gravitational waves can measure the time variation of the Planck mass
• Positivity in the sky
• Spectrum of Primordial Gravitational Waves in Modified Gravities: A Short Overview
• Cosmology and modified gravitational wave propagation from binary black hole population models
• Propagation of the gravitational waves in a cosmological background
• Probing modified gravity theories and cosmology using gravitational-waves and associated electromagnetic counterparts
• Combined search for anisotropic birefringence in the gravitational-wave transient catalog GWTC-1
• Positivity Bounds on Dark Energy: When Matter Matters
• Generalized framework for testing gravity with gravitational-wave propagation. III. Future prospect
• Gravitational wave constraints on dark sector models
• Gaussian processes reconstruction of modified gravitational wave propagation
• Primordial Gravitational Waves Predictions for GW170817-compatible Einstein-Gauss-Bonnet Theory
• Testing the Schwarzschild metric in a strong field region with the Event Horizon Telescope
• Gravitational-Wave Implications for the Parity Symmetry of Gravity at GeV Scale
• Cosmological constraints on dark energy in light of gravitational wave bounds
• Forecast constraints on $f(T)$ gravity with gravitational waves from compact binary coalescences
• Gravity in the infrared and effective nonlocal models
• Reviving non-Minimal Horndeski-like Theories after GW170817: Kinetic Coupling Corrected Einstein-Gauss-Bonnet Inflation
• The Well-Tempered Cosmological Constant
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Standard Sirens as a novel probe of dark energy
• Primordial gravitational waves in Horndeski gravity
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Forecasts on the speed of gravitational waves at high $z$
• Minimally modified gravity with an auxiliary constraint: a Hamiltonian construction
• Nonlocal gravity and gravitational-wave observations
• Theoretical and observational constraints on regularized 4$D$ Einstein-Gauss-Bonnet gravity
• Non-Abelian $S$-term dark energy and inflation
• Gravitational waves and extra dimensions: a short review
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• Limitations on Standard Sirens tests of gravity from screening
• Cosmological perturbations in Gauss-Bonnet quasi-dilaton massive gravity
• Learning how to surf: Reconstructing the propagation and origin of gravitational waves with Gaussian Processes
• New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
• $\text{Hi-COLA}$: Fast, approximate simulations of structure formation in Horndeski gravity
• Testing general relativity with TianQin: the prospect of using the inspiral signals of black hole binaries
• Scalar Fields Near Compact Objects: Resummation versus UV Completion
• Lunar Laser Ranging constraints on nonminimally coupled dark energy and standard sirens
• Observational Constraints in Nonlocal Gravity: the Deser-Woodard Case
• Gravitational-wave cosmological distances in scalar-tensor theories of gravity
• Probing the speed of gravity with LVK, LISA, and joint observations
• Modified gravitational wave propagation and the binary neutron star mass function
• Amplification of Primordial Gravitational Waves by a Geometrically Driven non-canonical Reheating Era
• Constraint on Brans-Dicke theory from intermediate/extreme mass ratio inspirals
• Gravity in mimetic scalar-tensor theories after GW170817
• $f(R)$-Gravity Generated Post-inflationary Eras and their Effect on Primordial Gravitational Waves
• Superradiant energy extraction from rotating hairy Horndeski black holes
• Phantom crossing dark energy in Horndeski's theory
• Constraining Horndeski theory with gravitational waves from coalescing binaries
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Testing the Speed of Gravity with Black Hole Ringdown
• No Slip CMB
• Propagation of scalar and tensor gravitational waves in Horndeski theory
• Limited Modified Gravity
• Probing modified gravitational-wave propagation with extreme mass-ratio inspirals
• Testing gravity with gravitational wave friction and gravitational slip
• Cosmological evolution of viable models in the generalized scalar-tensor theory
• Observational Constraints and Cosmographic Analysis of $f(T,T_G)$ Gravity and Cosmology
• Quintessence in the Weyl-Gauss-Bonnet model
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• On spin optics for gravitational waves lensed by a rotating object
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• No Run Gravity
• Jointly fitting weak lensing, X-ray and Sunyaev-Zel'dovich data to constrain scalar-tensor theories with clusters of galaxies
• Shift-symmetric Horndeski gravity in the asymptotic-safety paradigm
• Light propagation in the field of the N-body system and the application in the TianQin mission
• On tachyonic stability priors for dark energy
• Effects of a Late Gravitational Transition on Gravitational Waves and Anticipated Constraints
• Cosmology with LIGO/Virgo dark sirens: Hubble parameter and modified gravitational wave propagation
• Constraints on Quasi-dilaton Massive Gravity
• Gravitational waveforms from the inspiral of compact binaries in the Brans-Dicke theory in an expanding Universe
• Cosmology and the Early Universe
• Accelerating the standard siren method: Improved constraints on modified gravitational-wave propagation with future data
• The speed of gravitational waves and power-law solutions in a scalar-tensor model
• A Forecast for Large Scale Structure Constraints on Horndeski Gravity with Line Intensity Mapping
• Modified propagation of gravitational waves from the early radiation era
• Effective field theory of coupled dark energy and dark matter
• Oscillating solutions of the matter density contrast in Horndeski's theory
• Dark matter candidate induced by Horndeski theory: dark matter halo and cosmological evolution
• On phenomenological parametrizations for the luminosity distance of gravitational waves
• Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling
• The Cosmological Impact of Brane-Chern-Simons Massive Gravity
• Cosmic evolution in DHOST theories with scaling solutions
• Gravitational wave propagation beyond general relativity: waveform distortions and echoes
• Testing No slip model with pulsar timing arrays: NANOGrav and IPTA
• Parameterized tests of general relativity with gravitational wave generation and propagation
• Constraining Scalar Charge in Neutron Stars through Gravitational Wave Signals from NSBH Mergers
• Multiple-scale analysis of modified gravitational-wave propagation
• Probing modified gravitational wave propagation with strongly lensed coalescing binaries