Probing the interaction between dark energy and dark matter with future fast radio burst observations

Abstract

Interacting dark energy (IDE) scenario assumes that there exists a direct interaction between dark energy and cold dark matter, but this interaction is hard to be tightly constrained by the current data. Fast radio bursts (FRBs) will be seen in large numbers by future radio telescopes, and thus they have potential to become a promising low-redshift cosmological probe. In this work, we investigate the capability of future FRBs of constraining the dimensionless coupling parameter $\beta$ in four phenomenological IDE models. If we fix the FRB properties, about $10^5$ FRB data can give constraints on $\beta$ tighter than the current cosmic microwave background data in the IDE models with the interaction proportional to the energy density of dark energy. In all the IDE models, about $10^6$ FRB data can achieve the absolute errors of $\beta$ to less than $0.10$, providing a way to precisely measure $\beta$ by only one cosmological probe. Jointly constraining the FRB properties and cosmological parameters would increase the constraint errors of $\beta$ by a factor of about 0.5-2.

arXiv comment19 pages, 8 figures; accepted for publication in JCAP

References in corpus (102)

• Efficient Computation of CMB anisotropies in closed FRW models
• 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
• 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
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Observational constraints on Cosmic Reionization
• A fast radio burst associated with a Galactic magnetar
• A bright millisecond-duration radio burst from a Galactic magnetar
• Scaling solutions in general non-minimal coupling theories
• A census of baryons in the Universe from localized fast radio bursts
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• New physics in light of the $H_0$ tension: an alternative view
• The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
• The First CHIME/FRB Fast Radio Burst Catalog
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• Probing the Coupling between Dark Components of the Universe
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries
• Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
• Locating the "missing" baryons with extragalactic dispersion measure estimates
• Cosmological implications of Fast Radio Burst / Gamma-Ray Burst Associations
• Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Interactions in Scalar Field Cosmology
• Dark Energy and Dark Matter
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Distance Priors from Planck Final Release
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• Interacting Dark Energy -- constraints and degeneracies
• Fast radio bursts as a cosmic probe?
• Probing interaction and spatial curvature in the holographic dark energy model
• The Physics of Fast Radio Bursts
• Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
• Statefinder diagnosis for the interacting model of holographic dark energy
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Testing the interaction between dark energy and dark matter via latest observations
• Fast Radio Burst/Gamma-Ray Burst Cosmography
• Parametrized Post-Friedmann Signatures of Acceleration in the CMB
• A measurement of Hubble's Constant using Fast Radio Bursts
• Strongly lensed repeating Fast Radio Bursts as precision probes of the universe
• The imprint of the interaction between dark sectors in large scale cosmic microwave background anisotropies
• An 8\% Determination of the Hubble Constant from localized Fast Radio Bursts
• Constraint on Coupled Dark Energy Models from Observations
• Future Cosmological Constraints from Fast Radio Bursts
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Fast Radio Bursts and cosmological tests
• Relieving the $H_0$ tension with a new interacting dark energy model
• Exploring the full parameter space for an interacting dark energy model with recent observations including redshift-space distortions: Application of the parametrized post-Friedmann approach
• Interacting model of new agegraphic dark energy: Cosmological evolution and statefinder diagnostic
• Testing models of vacuum energy interacting with cold dark matter
• Constraining interacting dark energy models with latest cosmological observations
• A new measurement of the Hubble constant using Fast Radio Bursts
• Revisit of the interacting holographic dark energy model after Planck 2015
• Running coupling: Does the coupling between dark energy and dark matter change sign during the cosmological evolution?
• CHIME/FRB Catalog 1 results: statistical cross-correlations with large-scale structure
• Extracting host galaxy dispersion measure and constraining cosmological parameters using fast radio burst data
• The Large Dispersion and Scattering of FRB 20190520B are Dominated by the Host Galaxy
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Cosmology-independent estimate of the fraction of baryon mass in the IGM from fast radio burst observations
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Dispersion Distance and the Matter Distribution of the Universe in Dispersion Space
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Cosmological parameter estimation for dynamical dark energy models with future fast radio burst observations
• Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Multi-interacting dark energy and its cosmological implications
• Testing interacting dark matter and dark energy model with cosmological data
• A New Method to Measure Hubble Parameter $H(z)$ using Fast Radio Bursts
• Fast radio bursts to be detected with the Square Kilometre Array
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• A path to precision cosmology: synergy between four promising late-universe cosmological probes
• Redshift drift exploration for interacting dark energy
• Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Revisiting the interacting model of new agegraphic dark energy
• Exploring interacting holographic dark energy in a perturbed universe with parameterized post-Friedmann approach
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Fast Radio Burst Distributions Consistent with the First CHIME/FRB Catalog
• Implications from simulated strong gravitational lensing systems: constraining cosmological parameters using Gaussian Processes
• Prospects of strongly lensed repeating fast radio bursts: complementary constraints on dark energy evolution
• Constraining the Evolution of the Baryon Fraction in the IGM with FRB and H(z) data
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Probing primordial non-Gaussianity with Fast Radio Bursts
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Effect of Redshift Distributions of Fast Radio Bursts on Cosmological Constraints
• Prospects of strongly lensed fast radio bursts: Simultaneous measurement of post-Newtonian parameter and Hubble constant
• Reconstruction of Baryon Fraction in Intergalactic Medium through Dispersion Measurements of Fast Radio Bursts
• FRB dark sirens: Measuring the Hubble constant with unlocalized fast radio bursts
• Improvement of cosmological constraints with the cross correlation between line-of-sight optical galaxy and FRB dispersion measure

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