Generalized framework for testing gravity with gravitational-wave propagation. III. Future prospect

Abstract

The properties of gravitational-wave (GW) propagation are modified in alternative theories of gravity and are crucial observables to test gravity at cosmological distance. The propagation speed has already been measured from GW170817 so precisely and pinned down to the speed of light, while other properties of GW propagation have not constrained tightly yet. In this paper, we investigate the measurement precisions of the amplitude damping rate (equivalently, the time variation of the gravitational coupling for GWs) and graviton mass in the generalized framework of GW propagation with the future detectors such as Voyager, Cosmic Explorer, and Einstein Telescope. As a result, we show that the future GW observation can reach 1% error for the amplitude damping. We also study the time variation of the gravitational couplings in Horndeski theory by performing Monte Carlo-based numerical simulations. From the simulation results, we find that the current accelerating Universe prefers the models with less damping of GWs and that the equivalence principle can be tested at the level of 1% by the future GW observation.

22 pages, 16 figures

References in corpus (71)

• Planck 2015 results. XIII. Cosmological parameters
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Modified Gravity and Cosmology
• Multi-messenger Observations of a Binary Neutron Star Merger
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
• Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
• Chameleon Cosmology
• Gravitational Waves from Mergin Compact Binaries: How Accurately Can One Extract the Binary's Parameters from the Inspiral Waveform?
• Generalized G-inflation: Inflation with the most general second-order field equations
• From k-essence to generalised Galileons
• Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era
• Cosmology and Fundamental Physics with the Euclid Satellite
• Dark Energy after GW170817: dead ends and the road ahead
• Strong constraints on cosmological gravity from GW170817 and GRB 170817A
• Dark Energy after GW170817 and GRB170817A
• Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
• Varying constants, Gravitation and Cosmology
• Progress in Lunar Laser Ranging Tests of Relativistic Gravity
• Detection, Measurement and Gravitational Radiation
• Dark Energy vs. Modified Gravity
• Testing General Relativity in Cosmology
• Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity
• A Parameterized Post-Friedmann Framework for Modified Gravity
• Measuring the dark side (with weak lensing)
• Planck 2015 results. XIV. Dark energy and modified gravity
• Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
• Large Scale Structure as a Probe of Gravitational Slip
• Distinguishing Modified Gravity from Dark Energy
• Ultra-high precision cosmology from gravitational waves
• Observational Tests of Modified Gravity
• Effective gravitational couplings for cosmological perturbations in the most general scalar-tensor theories with second-order field equations
• Anisotropic stress as signature of non-standard propagation of gravitational waves
• The gravitational-wave luminosity distance in modified gravity theories
• Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation
• Modified gravitational-wave propagation and standard sirens
• GW170817 Falsifies Dark Matter Emulators
• Vainshtein screening in a cosmological background in the most general second-order scalar-tensor theory
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• Constraints on Einstein-aether theory after GW170817
• Localization accuracy of compact binary coalescences detected by the third-generation gravitational-wave detectors and implication for cosmology
• Tests of Gravitational Symmetries with Pulsar Binary J1713+0747
• What can Cosmology tell us about Gravity? Constraining Horndeski with Sigma and Mu
• Hořava Gravity after GW170817
• Mimicking dark matter and dark energy in a mimetic model compatible with GW170817
• Beyond Concordance Cosmology with Magnification of Gravitational-Wave Standard Sirens
• Cosmological parameter constraints for Horndeski scalar-tensor gravity
• Constraints on deviations from $\Lambda$CDM within Horndeski gravity
• Parity-violating gravity and GW170817
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• Complementarity of Weak Lensing and Peculiar Velocity Measurements in Testing General Relativity
• Effective Theory of Dark Energy at Redshift Survey Scales
• Probing the Friedmann equation during recombination with future CMB experiments
• Direct detection of gravitational waves can measure the time variation of the Planck mass
• Cosmological Constraints on Newton's Constant
• No Slip Gravity
• Large-scale structure phenomenology of viable Horndeski theories
• Polarization test of gravitational waves from compact binary coalescences
• Joint gravitational wave -- gamma-ray burst detection rates in the aftermath of GW170817
• From Cavendish to PLANCK: Constraining Newton's Gravitational Constant with CMB Temperature and Polarization Anisotropy
• The road ahead of Horndeski: cosmology of surviving scalar-tensor theories
• Searching for Modified Gravity: Scale and Redshift Dependent Constraints from Galaxy Peculiar Velocities
• Planck constraints on scalar-tensor cosmology and the variation of the gravitational constant
• Gravity at the horizon: on relativistic effects, CMB-LSS correlations and ultra-large scales in Horndeski's theory
• Phenomenology of Large Scale Structure in scalar-tensor theories: joint prior covariance of $w_{\text{DE}}$, $\Sigma$ and $\mu$ in Horndeski
• Cosmological Bound from the Neutron Star Merger GW170817 in scalar-tensor and $F(R)$ gravity theories
• Observational Consequences of Evolution of Primordial Fluctuations in Scalar-Tensor Cosmology
• Gravity's Islands: Parametrizing Horndeski Stability
• Measurement of Hubble constant with stellar-mass binary black holes
• Primordial gravitational waves in Horndeski gravity

Cited by in corpus (43)

• Science with the Einstein Telescope: a comparison of different designs
• Testing modified gravity at cosmological distances with LISA standard sirens
• The Gravitational-Wave Physics II: Progress
• Waveform of gravitational waves in the general parity-violating gravities
• 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
• Probing modified gravity theories and cosmology using gravitational-waves and associated electromagnetic counterparts
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• Gaussian processes reconstruction of modified gravitational wave propagation
• Gravitational-Wave Implications for the Parity Symmetry of Gravity at GeV Scale
• Current and future constraints on cosmology and modified gravitational wave friction from binary black holes
• Forecast constraints on $f(T)$ gravity with gravitational waves from compact binary coalescences
• Cosmology with Standard Sirens at Cosmic Noon
• Gravitational-Wave Detector Networks: Standard Sirens on Cosmology and Modified Gravity Theory
• Standard Sirens as a novel probe of dark energy
• Impacts of overlapping gravitational-wave signals on the parameter estimation: Toward the search for cosmological backgrounds
• Gravitational waves and geometrical optics in scalar-tensor theories
• Nonlocal gravity and gravitational-wave observations
• Limitations on Standard Sirens tests of gravity from screening
• Cosmological perturbations in Gauss-Bonnet quasi-dilaton massive gravity
• New probe of gravity: strongly lensed gravitational wave multi-messenger approach
• Analyzing clustering of astrophysical gravitational-wave sources: Luminosity-distance space distortions
• Gravitational-wave cosmological distances in scalar-tensor theories of gravity
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Parameter estimation of eccentric gravitational waves with a decihertz observatory and its cosmological implications
• Parity violation in gravitational waves and observational bounds from third-generation detectors
• Testing gravity with gravitational wave friction and gravitational slip
• Cosmological evolution of viable models in the generalized scalar-tensor theory
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• Space-borne atom interferometric gravitational wave detections. Part I. The forecast of bright sirens on cosmology
• No slip gravity in light of LISA standard sirens
• Cosmology and perturbations in tachyonic massive gravity
• Early warning of precessing compact binary merger with third-generation gravitational-wave detectors
• Gravitational couplings in Chameleon models
• A model-independent tripartite test of cosmic distance relations
• Gravitational waveforms from the inspiral of compact binaries in the Brans-Dicke theory in an expanding Universe
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Cosmological Study in Myrzakulov $F(R,T)$ Quasi-dilaton Massive Gravity
• Forecast Analysis of Astrophysical Stochastic Gravitational Wave Background beyond general relativity: A Case Study on Brans-Dicke Gravity
• Quantization of the nonstandard propagating gravitational waves in the cosmological background
• The Cosmological Impact of Brane-Chern-Simons Massive Gravity
• Cosmology of Quasi-Dilaton Massive Gravity with Non-minimal Kinetic Coupling