Future Constraints on Dynamical Dark-Energy using Gravitational-Wave Standard Sirens

Abstract

The detection of gravitational waves (GW) by the LIGO and Virgo collaborations offers a whole new range of possible tests and opens up a new window which may shed light on the nature of dark energy and dark matter. In the present work we investigate how future gravitational waves data could help to constrain different dynamical dark energy models. In particular, we perform cosmological forecastings of a class of well known and most used dynamical dark energy models using the third-generation gravitational wave detector, the Einstein Telescope. We have considered 1000 simulated GW events in order to constrain the parameter space of the dynamical dark energy models. Our analyses show that the inclusion of the GW data from the Einstein Telescope, significantly improves the parameter space of the dynamical dark energy models compared to their constraints extracted from the standard cosmological probes, namely, the cosmic microwave observations, baryon acoustic oscillations distance measurements, Supernove type Ia, and the Hubble parameter measurements.

arXiv comment27 pages, 10 tables and 13 figures, version accepted for publication in Physical Review D

References in corpus (75)

• 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
• 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
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Exploring the Expansion History of the Universe
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• Accelerating Universes with Scaling Dark Matter
• GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
• TianQin: a space-borne gravitational wave detector
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
• Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
• The Simons Observatory: Science goals and forecasts
• GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• 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
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Cosmological perturbations
• Efficient sampling of fast and slow cosmological parameters
• Scientific Objectives of Einstein Telescope
• Reconciling Planck with the local value of $H_0$ in extended parameter space
• Future Supernovae observations as a probe of dark energy
• Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies
• Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
• Ultra-high precision cosmology from gravitational waves
• A parametric model for dark energy
• Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations
• Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z)\ge -1$ are tighter than those obtained in $\Lambda$CDM
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Dark energy in Horndeski theories after GW170817: A review
• Gravitational Lensing as a Probe of Quintessence
• Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope
• Gravitational waves from cosmological compact binaries
• Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy
• How many dark energy parameters?
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
• Observational constraints on one-parameter dynamical dark-energy parametrizations and the $H_0$ tension
• Gravitational Wave Decay into Dark Energy
• Brane-world extra dimensions in light of GW170817
• Constraints on Einstein-aether theory after GW170817
• First predictions of the angular power spectrum of the astrophysical gravitational wave background
• Can luminosity distance measurements probe the equation of state of dark energy
• Stochastic Gravitational-Wave Background from Binary Black Holes and Binary Neutron Stars and Implications for LISA
• Alive and well: mimetic gravity and a higher-order extension in light of GW170817
• Mimicking dark matter and dark energy in a mimetic model compatible with GW170817
• New observational constraints on $f(T)$ gravity through gravitational-wave astronomy
• Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology
• Dark energy after GW170817, revisited
• Probing cosmic anisotropy with gravitational waves as standard sirens
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Constraining the time variation of Newton's constant $G$ with gravitational-wave standard sirens and supernovae
• Testing Brans-Dicke gravity using the Einstein telescope
• Observational Constraints on Oscillating Dark-Energy Parametrizations
• Signatures of extra dimensions in gravitational waves from black hole quasi-normal modes
• Improving cosmological parameter estimation with the future gravitational-wave standard siren observation from the Einstein Telescope
• Model-independent Curvature Determination from Gravitational-Wave Standard Sirens and Cosmic Chronometers
• Latest astronomical constraints on some nonlinear parametric dark energy models
• Waveforms of compact binary inspiral gravitational radiation in screened modified gravity
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• A synthetic model of the gravitational wave background from evolving binary compact objects
• Gravitational wave forms, polarizations, response functions and energy losses of triple systems in Einstein-Aether theory
• Euclid space mission: a cosmological challenge for the next 15 years
• First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant
• Biased Cosmology: Pivots, Parameters, and Figures of Merit

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• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
• Revisiting a negative cosmological constant from low-redshift data
• Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
• The Gravitational-Wave Physics II: Progress
• Do we have any hope of detecting scattering between dark energy and baryons through cosmology?
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Revealing the effects of curvature on the cosmological models
• Constraining the Hubble constant to a precision of about 1% using multi-band dark standard siren detections
• Forecasting constraints on deviations from general relativity in $f(Q)$ gravity with standard sirens
• Dark degeneracy I: Dynamical or interacting dark energy?
• Constraints on the distance duality relation with standard sirens
• Constraining the cosmological parameters using gravitational wave observations of massive black hole binaries and statistical redshift information
• The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
• A preliminary forecast for cosmological parameter estimation with gravitational-wave standard sirens from TianQin
• 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
• 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
• 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 $z$
• Imprints of an extended Chevallier-Polarski-Linder parametrization on the large scale of our universe
• 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
• Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications
• Searching for modified gravity in the astrophysical gravitational wave background: Application to ground-based interferometers
• Forecast constraints on Anisotropic Stress in Dark Energy using gravitational-waves
• Exploring bulk viscous unified scenarios with Gravitational Waves Standard Sirens
• Will Gravitational Wave Sirens Determine the Hubble Constant?
• Rapid identification of time-frequency domain gravitational wave signals from binary black holes using deep learning
• Investigating the dynamical models of cosmology with recent observations and upcoming gravitational-wave data
• Combining strongly lensed and unlensed fast radio bursts: To be a more precise late-universe probe
• 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
• How will our knowledge of short gamma-ray bursts affect the distance measurement of binary neutron stars?
• Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
• Search for exotic gravitational wave signals beyond general relativity using deep learning
• Forecast cosmological constraints from the number counts of Gravitational Waves events
• Prospects for joint multiband detection of intermediate-mass black holes by LGWA and the Einstein Telescope
• Rings of light caused by gravitational waves