Probing the interaction between dark matter and dark energy in the presence of massive neutrinos

Abstract

We consider the possibility of an interaction in the dark sector in the presence of massive neutrinos, and study the observational constraints on three different scenarios of massive neutrinos using the most recent CMB anisotropy data in combination with type Ia supernovae, baryon acoustic oscillations, and Hubble parameter measurements. When a sterile neutrino is introduced in the interacting dark sector scenario in addition to the standard model prediction of neutrinos, we find that the coupling parameter, characterizing the interaction between dark matter and dark energy, is non-zero at 2$\sigma$ confidence level. The interaction model with sterile neutrino is also found to be a promising one to alleviate the current tension on Hubble constant. We do not find the evidence for a coupling in the dark sector when the possibility of a sterile neutrino is discarded.

arXiv comment8 pages, 4 figures; Added new models based on neutrinos, and revised the whole paper accordingly

References in corpus (44)

• Planck 2015 results. XIII. Cosmological parameters
• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• A 2.4% Determination of the Local Value of the Hubble Constant
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Massive neutrinos and cosmology
• Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
• Cosmological perturbations
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Quasar-Lyman $\alpha$ Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations
• Neutrinos in cosmology
• Large-scale instability in interacting dark energy and dark matter fluids
• Reconciling Planck with the local value of $H_0$ in extended parameter space
• Indications of a late-time interaction in the dark sector
• Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure
• Evidence for massive neutrinos from CMB and lensing observations
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Can vacuum decay in our Universe?
• Reconciling CMB and structure growth measurements with dark energy interactions
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• New constraints on interacting dark energy from cosmic chronometers
• Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies
• Hints of dynamical vacuum energy in the expanding Universe
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Cosmological constraints on a decomposed Chaplygin gas
• On phenomenological models of dark energy interacting with dark matter
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• Inhomogeneous vacuum energy
• Testing models of vacuum energy interacting with cold dark matter
• Constraints on non-flat cosmologies with massive neutrinos after Planck 2015
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Cosmological constraints on coupled dark energy
• Distinguishing interacting dark energy from wCDM with CMB, lensing, and baryon acoustic oscillation data
• Dark matter-dark energy interaction for a time-dependent equation of state
• Galaxy clustering, CMB and supernova data constraints on $\varphi$CDM model with massive neutrinos
• Observational constraints on varying neutrino-mass cosmology
• Cosmology with interaction in the dark sector
• Matter Power Spectra in Viable $f(R)$ Gravity Models with Massive Neutrinos
• Exploring a new interaction between dark matter and dark energy using the growth rate of structure
• Interaction in the dark sector

Cited by in corpus (164)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Early Dark Energy Can Resolve The Hubble Tension
• Cosmology Intertwined II: The Hubble Constant Tension
• New physics in light of the $H_0$ tension: an alternative view
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• 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
• Echo of interactions in the dark sector
• Prospects for resolving the Hubble constant tension with standard sirens
• New Early Dark Energy
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Revisiting a negative cosmological constant from low-redshift data
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• Reducing the $H_0$ and ${\sigma }_8$ tensions with Dark Matter-neutrino interactions
• Structure formation in $f(T)$ gravity and a solution for $H_0$ tension
• A Vacuum Phase Transition Solves $H_0$ Tension
• Dark Energy with Phantom Crossing and the $H_0$ tension
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• Exploring Cosmic Origins with CORE: Cosmological Parameters
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Scalar-tensor theories of gravity, neutrino physics, and the $H_0$ tension
• A new interacting two fluid model and its consequences
• 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
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Dark sectors with dynamical coupling
• Dark sector interaction and the supernova absolute magnitude tension
• All-inclusive interacting dark sector cosmologies
• A model with interaction of dark components and recent observational data
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• New constraints on interacting dark energy from DESI DR2 BAO observations
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• Tension of the $E_G$ statistic and RSD data with Planck/$\Lambda$CDM and implications for weakening gravity
• Cosmic voids in modified gravity models with massive neutrinos
• Measurements of $H_0$ and reconstruction of the dark energy properties from a model-independent joint analysis
• Late time transitions in the quintessence field and the $H_0$ tension
• Soundness of Dark Energy properties
• Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe
• Late time interacting cosmologies and the Hubble constant tension
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• Dark Neutrino interactions phase out the Hubble tension
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• Unbiased Hubble constant estimation from binary neutron star mergers
• Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints
• Constraints on interacting dark energy models through cosmic chronometers and Gaussian process
• Dynamics of nonlinear interacting dark energy models
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• Quantifying the $S_8$ tension and evidence for interacting dark energy from redshift-space distortion measurements
• Dark degeneracy I: Dynamical or interacting dark energy?
• A double take on early and interacting dark energy from JWST
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Observational constraints on dark matter-dark energy scattering cross section
• Probing elastic interactions in the dark sector and the role of $S_8$
• A fake Interacting Dark Energy detection?
• Cosmological bounds on dark matter-photon coupling
• Large-scale (in-) stability Analysis of an Exactly Solved Coupled Dark-Energy Model
• Emergent Dark Energy, neutrinos and cosmological tensions
• On structure formation from a small-scales-interacting dark sector
• Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• 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
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• Late time acceleration due to generic modification of gravity and Hubble tension
• Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• A model of interacting dark fluids tested with supernovae and Baryon Acoustic Oscillations data
• The cosmological impact of future constraints on $H_0$ from gravitational-wave standard sirens
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Weak cosmic growth in coupled dark energy with a Lagrangian formulation
• Smoothing the $H_0$ tension with a dynamical dark energy model
• Dynamical systems methods and statefinder diagnostic of interacting vacuum energy models
• No H_0 Assistance from Assisted Quintessence
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• Models of vacuum energy interacting with cold dark matter: Constraints and comparison
• Non-parametric reconstruction of interaction in the cosmic dark sector
• Strong Bounds on Sum of Neutrino Masses in a 12 Parameter Extended Scenario with Non-Phantom Dynamical Dark Energy ($w(z)\ge -1$)
• Constraining the dark-energy equation of state with cosmological data
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Dynamical analysis of interacting dark energy model in the framework of particle creation mechanism
• General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories
• Quintessential Cosmological Tensions
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Testing the warmness of dark matter
• Clustering and redshift-space distortions in modified gravity models with massive neutrinos
• Alleviating $H_0$ tension in Horndeski gravity
• Can phantom transition at $z\sim 1$ restore the Cosmic concordance?
• J-PAS: forecasts on interacting vacuum energy models
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Constraints on Newton's Constant from Cosmological Observations
• Cascading Dark Energy
• Dark matter solution to the $H_0$ and $S_8$ tensions, and the integrated Sachs-Wolfe void anomaly
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids
• Gravitational Baryogenesis in Running Vacuum models
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Alleviating $H_0$ tension in scalar-tensor and bi-scalar-tensor theories
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• On sign-changeable interaction in FLRW cosmology
• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• In search of an interaction in the dark sector through Gaussian Process and ANN approaches
• FLRW accelerating universe with interactive dark energy
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• On the interacting dark energy scenarios $-$ the case for Hubble constant tension
• Early Dark Energy from a Higher-dimensional Gauge Theory
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• An FLRW interacting dark energy model of the Universe
• Non-thermal neutrino-like hot dark matter in light of the $S_8$ tension
• Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Do we need wavelets in the late Universe?
• Constraints On Dark Energy Models From Galaxy Clusters and Gravitational Lensing Data
• Observational constraints on interactions between dark energy and dark matter with momentum and energy transfers
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• Coupled dark energy model inspired from general conformal transformation
• Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy
• Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
• Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
• Modified Equations of State for Dark Energy and Observational Limitations
• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Dark Energy and Modified Scale Covariant Theory of Gravitation
• Implications for cosmology from Ground-based Cosmic Microwave Background observations
• Effects of anisotropy in an anisotropic extension of $w$CDM model
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• Universe consisting of diffusive dark fluids: thermodynamics and stability analysis
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Phantom Dirac-Born-Infeld Dark Energy
• Measuring neutrino mass in light of ACT DR6 and DESI DR2
• Reconstructing the dark matter and dark energy interaction scenarios from observations
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• Interacting Dark Energy and Its Implications for Unified Dark Sector
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Interacting tachyon with varying mass dark matter
• Cosmological constraints on mass-varying dark matter
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe
• Self-interaction in a cosmic dark fluid: The four-kernel rheological extension of the equations of state
• Crunching, Bouncing, and Cyclical Cosmologies from Dark Sector Interactions
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Is the $\Lambda$CDM Model in Crisis?