Listening to the sound of dark sector interactions with gravitational wave standard sirens

Abstract

We consider two stable Interacting Dark Matter -- Dark Energy models and confront them against current Cosmic Microwave Background data from the \textit{Planck} satellite. We then generate luminosity distance measurements from $\mathcal{O}(10^3)$ mock Gravitational Wave events matching the expected sensitivity of the proposed Einstein Telescope. We use these to forecast how the addition of Gravitational Wave standard sirens data can improve current limits on the Dark Matter -- Dark Energy coupling strength ($\xi$). We find that the addition of Gravitational Waves data can reduce the current uncertainty by a factor of $5$. Moreover, if the underlying cosmological model truly features Dark Matter -- Dark Energy interactions with a value of $\xi$ within the currently allowed $1\sigma$ upper limit, the addition of Gravitational Wave data would help disentangle such an interaction from the standard case of no interaction at a significance of more than $3\sigma$.

arXiv comment16 pages, 3 tables, 4 figures; version published in JCAP

References in corpus (178)

• 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
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• f(R) theories
• Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
• Cosmology and the Fate of Dilatation Symmetry
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Coupled Quintessence
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Testing General Relativity with Present and Future Astrophysical Observations
• A gravitational-wave standard siren measurement of the Hubble constant
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Gravitational Wave Experiments and Early Universe Cosmology
• 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
• Using gravitational-wave standard sirens
• Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
• Black holes, gravitational waves and fundamental physics: a roadmap
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Scientific Objectives of Einstein Telescope
• Interacting Dark Matter and Dark Energy
• Dynamical systems applied to cosmology: dark energy and modified gravity
• A 2 per cent Hubble constant measurement from standard sirens within 5 years
• Can interacting dark energy solve the $H_0$ tension?
• Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy
• Large-scale instability in interacting dark energy and dark matter fluids
• Mimetic Dark Matter
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Neutrino masses and cosmology with Lyman-alpha forest power spectrum
• Short GRB and binary black hole standard sirens as a probe of dark energy
• Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics
• Inference of the cosmological parameters from gravitational waves: application to second generation interferometers
• Dynamics of interacting dark energy
• Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
• Ultra-high precision cosmology from gravitational waves
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Scalar-tensor theories and modified gravity in the wake of GW170817
• Mimetic gravity: a review of recent developments and applications to cosmology and astrophysics
• Cosmologies with Energy Exchange
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Thermodynamics of dark energy interacting with dark matter and radiation
• Precision of Hubble constant derived using black hole binary absolute distances and statistical redshift information
• Interactions in Scalar Field Cosmology
• Prospects for resolving the Hubble constant tension with standard sirens
• Echo of interactions in the dark sector
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Gravitational wave astronomy
• Dark coupling
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Inflation in $f(R,\varphi )$-theories and mimetic gravity scenario
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Screening Modifications of Gravity through Disformally Coupled Fields
• GW170817 Falsifies Dark Matter Emulators
• Growing Matter
• On the improvement of cosmological neutrino mass bounds
• Interacting Dark Energy -- constraints and degeneracies
• Gravitational waves from cosmological compact binaries
• Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy
• Dark Interactions and Cosmological Fine-Tuning
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Generalized framework for testing gravity with gravitational-wave propagation. II. Constraints on Horndeski theory
• New constraints on interacting dark energy from cosmic chronometers
• Testing the Interaction between Dark Energy and Dark Matter with Planck Data
• Limits on the number of spacetime dimensions from GW170817
• Interacting models may be key to solve the cosmic coincidence problem
• Vainshtein mechanism after GW170817
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Brane-world extra dimensions in light of GW170817
• $f(T)$ gravity after GW170817 and GRB170817A
• The Growth of Structure in Interacting Dark Energy Models
• Scaling attractors in interacting teleparallel dark energy
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• The fate of large-scale structure in modified gravity after GW170817 and GRB170817A
• Conformal-Frame (In)dependence of Cosmological Observations in Scalar-Tensor Theory
• Coupled dark matter-dark energy in light of near Universe observations
• Effective Theory of Interacting Dark Energy
• Adiabatic initial conditions for perturbations in interacting dark energy models
• Vainshtein Screening in Scalar-Tensor Theories before and after GW170817: Constraints on Theories beyond Horndeski
• Covariant Horava-like and mimetic Horndeski gravity: cosmological solutions and perturbations
• Scale-dependent galaxy bias, CMB lensing-galaxy cross-correlation, and neutrino masses
• An analytic model for interacting dark energy and its observational constraints
• Hořava Gravity after GW170817
• A new interacting two fluid model and its consequences
• Cosmological dynamics of mimetic gravity
• Signature of the interaction between dark energy and dark matter in observations
• Alive and well: mimetic gravity and a higher-order extension in light of GW170817
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• On the large-scale instability in interacting dark energy and dark matter fluids
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Interacting dark energy in $f(R)$ gravity
• Hearing the echoes of electroweak baryogenesis with gravitational wave detectors
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• Mimicking dark matter and dark energy in a mimetic model compatible with GW170817
• Evidence for interacting dark energy from BOSS
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• On phenomenological models of dark energy interacting with dark matter
• Recovering a MOND-like acceleration law in mimetic gravity
• A Field Theory Model for Dark Matter and Dark Energy in Interaction
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• Dark Coupling and Gauge Invariance
• The length of the low-redshift standard ruler
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• Testing coupled dark energy with large scale structure observation
• Cosmological Constraints on Horndeski Gravity in Light of GW170817
• A model with interaction of dark components and recent observational data
• Probing cosmic anisotropy with gravitational waves as standard sirens
• Scalar-Fluid theories: cosmological perturbations and large-scale structure
• Testing models of vacuum energy interacting with cold dark matter
• Reconstructing the dark sector interaction with LISA
• Covariantizing the interaction between dark energy and dark matter
• Constraining interacting dark energy models with latest cosmological observations
• Is cosmic acceleration proven by local cosmological probes?
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Cosmological constraints on parametrized interacting dark energy
• Constraining the dark energy equation of state using LISA observations of spinning Massive Black Hole binaries
• In search of the dark matter dark energy interaction: a kinematic approach
• Cosmological constraints on an exponential interaction in the dark sector
• Robust model comparison disfavors power law cosmology
• Cosmological constraints on coupled dark energy
• Observational constraints on dark matter-dark energy scattering cross section
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• A cosmographic analysis of holographic dark energy models
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
• Future CMB cosmological constraints in a dark coupled universe
• Gauge-Invariant Perturbations of Varying-Alpha Cosmologies
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Probing the imprints of generalized interacting dark energy on the growth of perturbations
• Constraining interacting dark energy with CMB and BAO future surveys
• Null test for interactions in the dark sector
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Dark matter-dark energy interaction for a time-dependent equation of state
• Cosmological Bound from the Neutron Star Merger GW170817 in scalar-tensor and $F(R)$ gravity theories
• Future weak lensing constraints in a dark coupled universe
• Constraints on $f(R)$ theories of gravity from GW170817
• Measurement of Hubble constant with stellar-mass binary black holes
• Quintessence with Yukawa Interaction
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Power law cosmology model comparison with CMB scale information
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models
• J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
• Dark energy with a gradient coupling to the dark matter fluid: cosmological dynamics and structure formation
• Revisiting f(R) gravity models that reproduce $\Lambda$CDM expansion
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• Avoiding selection bias in gravitational wave astronomy
• Cosmological singularities in interacting dark energy models with an $\omega (q)$ parametrization
• Dark energy and Dark matter interaction in light of the second law of thermodynamics
• Modified Brans-Dicke cosmology with matter-scalar field interaction
• Extended Phase Space Analysis of Interacting Dark Energy Models in Loop Quantum Cosmology
• Deep connection between f(R) gravity and the interacting dark sector model
• CMB and matter power spectra with non-linear dark-sector interactions
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Limiting curvature mimetic gravity and its relation to Loop Quantum Cosmology
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• Dark sectors of the Universe: A Euclid survey approach
• Two-field cosmological phase transitions and gravitational waves in the singlet Majoron model
• Testing Dark Matter Models with Radio Telescopes in light of Gravitational Wave Astronomy
• Gravity in mimetic scalar-tensor theories after GW170817
• Coupling dark energy to dark matter inhomogeneities
• Prospects of the local Hubble parameter measurement using gravitational waves from double neutron stars
• Precessing supermassive black hole binaries and dark energy measurements with LISA
• Exact cosmological solutions of models with an interacting dark sector
• Revisiting the Instability Problem of Interacting Dark Energy Model in the Parametrized Post-Friedmann Framework
• Exploring evidence of interaction between dark energy and dark matter

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• In the Realm of the Hubble tension $-$ a Review of Solutions
• Non-minimal dark sector physics and cosmological tensions
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Revisiting a negative cosmological constant from low-redshift data
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• The Gravitational-Wave Physics II: Progress
• Nonlinear interacting cosmological models after Planck 2018 legacy release and the $H_0$ tension
• Field theoretic interpretations of interacting dark energy scenarios and recent observations
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Probing observational bounds on scalar-tensor theories from standard sirens
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Dark sectors with dynamical coupling
• All-inclusive interacting dark sector cosmologies
• Reconciling $H_0$ tension in a six parameter space?
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
• Cosmological parameter estimation with future gravitational wave standard siren observation from the Einstein Telescope
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Forecast constraints on $f(T)$ gravity with gravitational waves from compact binary coalescences
• Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds
• Dynamics of a two scalar field cosmological model with phantom terms
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Dynamical Dark sectors and Neutrino masses and abundances
• Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• Forecasts on the speed of gravitational waves at high $z$
• Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
• Exploiting the Einstein Telescope to solve the Hubble tension
• Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• A model-independent reconstruction of dark sector interactions
• Probing Interacting Dark Energy and Scattering of Baryons with Dark Matter in Light of EDGES 21cm Signal
• Interacting quintessence in light of Generalized Uncertainty Principle: Cosmological perturbations and dynamics
• Testing f(R) gravity with the simulated data of gravitational waves from the Einstein Telescope
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Constraining $\Lambda$CDM cosmological parameters with Einstein Telescope mock data
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• Addressing Cosmological Tensions by Non-Local Gravity
• A test of the standard dark matter density evolution law using galaxy clusters and cosmic chronometers
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• Forecast Analysis on Interacting Dark Energy Models from Future Generation PICO and DESI Missions
• No slip gravity in light of LISA standard sirens
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Addressing the High-$f$ Problem in Pseudo-Nambu-Goldstone Boson Dark Energy Models with Dark Matter - Dark Energy Interaction
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Probing the dark matter density evolution law with large scale structures
• Generalized Model of Interacting Dark Energy and Dark Matter : Phase Portrait Analysis of Evolving Universe
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Exploring the potentiality of standard sirens to probe cosmic opacity at high redshifts
• Quasinormal Modes and Greybody Factors of Charged Symmergent Black Hole
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations
• Interacting Dark Energy: New parametrization and observational constraints
• Gravitational wave signatures from dark sector interactions
• Gravitational wave probes of Barrow cosmology with LISA standard sirens
• Measuring the primordial gravitational waves from cosmic microwave background and stochastic gravitational wave background observations
• Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
• Primordial blackhole formation: Exploring chaotic potential with a sharp step via the GLMS perspective
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Accelerating scaling solutions from dark matter particle creation
• Rings of light caused by gravitational waves