Constraints on the distance duality relation with standard sirens

Abstract

We use gravitational wave (GW) standard sirens, in addition to Type Ia supernovae (SNIa) and baryon acoustic oscillation (BAO) mock data, to forecast constraints on the electromagnetic and gravitational distance duality relations (DDR). We make use of a parameterised approach based on a specific DDR violation model, along with a machine learning reconstruction method based on the Genetic Algorithms. We find that GW provide an alternative to the use of BAO data to constrain violations of the DDR, reaching $3\%$ constraints on the violation parameter we consider when combined with SNIa, which is only improved by a factor of $\approx 1.4$ if one instead considers the combination of BAO and SNIa. We also investigate the possibility that a neglected modification of gravity might lead to a false detection of DDR violations, even when screening mechanisms are active. We find that such a false detection can be extremely significant, up to $\approx 10\sigma$ for very extreme modified gravity scenarios, while this reduces to $\approx 4\sigma$ in a more realistic case. False detections can also provide a smoking gun for the modified gravity mechanism at play, as a result of the tension introduced between the SNIa+GW and SNIa+BAO combinations.

arXiv comment31 pages, 13 figures. Version 2 aligns with the published version in JCAP (references and details added to the introduction, more discussion of modified gravity parameterisation and the genetic algorithm results included)

References in corpus (78)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Efficient Computation of CMB anisotropies in closed FRW models
• f(R) Theories Of Gravity
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
• GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4M_{\odot }$
• A gravitational-wave standard siren measurement of the Hubble constant
• Science Case for the Einstein Telescope
• Sensitivity Studies for Third-Generation Gravitational Wave Observatories
• Dark Energy after GW170817: dead ends and the road ahead
• Supernova Constraints and Systematic Uncertainties from the First 3 Years of the Supernova Legacy Survey
• Dark Energy after GW170817 and GRB170817A
• Using gravitational-wave standard sirens
• GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses
• CMB power spectrum parameter degeneracies in the era of precision cosmology
• PolyChord: nested sampling for cosmology
• Gravitational waves from inspiralling compact binaries: Parameter estimation using second-post-Newtonian waveforms
• Nonperturbative Continuity in Graviton Mass versus Perturbative Discontinuity
• PolyChord: next-generation nested sampling
• Excess Electronic Recoil Events in XENON1T
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• Dark Energy Survey Year 1 Results: Constraints on Extended Cosmological Models from Galaxy Clustering and Weak Lensing
• f(R) Gravity and Chameleon Theories
• Short GRB and binary black hole standard sirens as a probe of dark energy
• Matter density perturbations and effective gravitational constant in modified gravity models of dark energy
• Ultra-high precision cosmology from gravitational waves
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Cosmography with the Einstein Telescope
• Tension and constraints on modified gravity parametrizations of $G_{\text{eff}}(z)$ from growth rate and Planck data
• Dimming Supernovae without Cosmic Acceleration
• Cosmic distance-duality as probe of exotic physics and acceleration
• The gravitational-wave luminosity distance in modified gravity theories
• Modified gravitational-wave propagation and standard sirens
• The detectability of baryonic acoustic oscillations in future galaxy surveys
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys
• Bounds on the possible evolution of the Gravitational Constant from Cosmological Type-Ia Supernovae
• Testing the Distance-Duality Relation with Galaxy Clusters and Type Ia Supernovae
• Constraints on cosmic opacity and beyond the standard model physics from cosmological distance measurements
• Piercing the Vainshtein screen with anomalous gravitational wave speed: Constraints on modified gravity from binary pulsars
• Matter density perturbations in modified gravity models with arbitrary coupling between matter and geometry
• The response of primordial abundances to a general modification of $G_{\mathrm{N}}$ and/or of the early universe expansion rate
• Curvature vs Distances: testing the FLRW cosmology
• Constraining chameleon models with cosmology
• Evolving Newton's Constant, Extended Gravity Theories and SnIa Data Analysis
• A new perspective on Dark Energy modeling via Genetic Algorithms
• The Distance Duality Relation from Strong Gravitational Lensing
• Solar axions cannot explain the XENON1T excess
• A test for cosmic distance duality
• A Profile Likelihood Analysis of the Constrained MSSM with Genetic Algorithms
• Unraveling the effective fluid approach for $f(R)$ models in the subhorizon approximation
• Consistency among distance measurements: transparency, BAO scale and accelerated expansion
• A model independent null test on the cosmological constant
• Multi-messenger tests of gravity with weakly lensed gravitational waves
• What can Machine Learning tell us about the background expansion of the Universe?
• Type Ia supernovae, standardisable candles, and gravity
• Breaking of the equivalence principle in the electromagnetic sector and its cosmological signatures
• Forecast for cosmological parameter estimation with gravitational-wave standard siren observation from the Cosmic Explorer
• Genetic Algorithms and Supernovae Type Ia Analysis
• Galaxy morphology rules out astrophysically relevant Hu-Sawicki $f(R)$ gravity
• Extending the supernova Hubble diagram to z~1.5 with the Euclid space mission
• Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens
• Designing Horndeski and the effective fluid approach
• Dimming of Supernovae by Photon-Pseudoscalar Conversion and the Intergalactic Plasma
• Comparative analysis of model-independent methods for exploring the nature of dark energy
• Newton's constant in f(R,R_{μν}R^{μν},\Box R) theories of gravity and constraints from BBN
• Hints of dark energy anisotropic stress using Machine Learning
• Is the Universe Transparent?
• Horndeski gravity and standard sirens
• Dark Energy coupling with electromagnetism as seen from future low-medium redshift probes
• The cosmic distance duality relation with strong lensing and gravitational waves: an opacity-free test
• Machine Learning meets the redshift evolution of the CMB Temperature
• Limitations on Standard Sirens tests of gravity from screening
• The Linear Point: A cleaner cosmological standard ruler
• Cosmology with Photometric Surveys of Type Ia Supernovae
• The Linear Point Standard Ruler for galaxy survey data: validation with mock catalogues
• Constraining axionlike particles using the distance-duality relation

Cited by in corpus (33)

• Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
• The Science of the Einstein Telescope
• Testing the general theory of relativity using gravitational wave propagation from dark standard sirens
• Testing Late Time Cosmic Acceleration with uncorrelated Baryon Acoustic Oscillations dataset
• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
• The resilience of the Etherington-Hubble relation
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Constraints on the Parameterized Deceleration Parameter in FLRW Universe
• Scalar and tensor gravitational waves
• Revisiting the cosmic distance duality relation with machine learning reconstruction methods: the combination of HII galaxies and ultra-compact radio quasars
• Dancing in the dark: detecting a population of distant primordial black holes
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Machine learning forecasts of the cosmic distance duality relation with strongly lensed gravitational wave events
• Data Analysis of three parameter models of deceleration parameter in FRW Universe
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Model-independent study for a quintessence model of dark energy: Analysis and Observational constraints
• Non-Canonical Volume-Form Formulation of Modified Gravity Theories and Cosmology
• Cosmographic Footprints of Dynamical Dark Energy
• Diagnostic and Comparative Analysis of Dark Energy Models with $q(z)$ Parametrizations
• Mapping the inhomogeneous Universe with Standard Sirens: Degeneracy between inhomogeneity and modified gravity theories
• No slip gravity in light of LISA standard sirens
• Cosmological Tests of Gravity: A Future Perspective
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• GEO-FPT: a model of the galaxy bispectrum at mildly non-linear scales
• A model-independent tripartite test of cosmic distance relations
• The impact of 2D and 3D BAO measurements on the Cosmic Distance Duality Relation with HII galaxies
• Resilience and implications of adiabatic CMB cooling
• Climbing out of the shadows: building the distance ladder with black hole images
• An investigation of a varying G through Strong Lensing and SNe Ia observations
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Forecast cosmological constraints from the number counts of Gravitational Waves events