Exploring neutrino mass and mass hierarchy in interacting dark energy models

Abstract

We investigate how the dark energy properties impact the constraints on the total neutrino mass in interacting dark energy (IDE) models. In this study, we focus on two typical interacting dynamical dark energy models, i.e., the interacting $w$ cold dark matter (I$w$CDM) model and the interacting holographic dark energy (IHDE) model. To avoid the large-scale instability problem in IDE models, we apply the parameterized post-Friedmann approach to calculate the perturbation of dark energy. We employ the Planck 2015 cosmic microwave background temperature and polarization data, combined with low-redshift measurements on baryon acoustic oscillation distance scales, type Ia supernovae, and the Hubble constant, to constrain the cosmological parameters. We find that the dark energy properties could influence the constraint limits on the total neutrino mass. Once dynamical dark energy is considered in the IDE models, the upper bounds of $\sum m_{\nu }$ will be changed. By considering the values of ${\chi }_{\min }^2$, we find that in these IDE models the normal hierarchy case is slightly preferred over the inverted hierarchy case; for example, $\Delta {\chi }^2=2.720$ is given in the IHDE+$\sum m_{\nu }$ model. In addition, we also find that in the I$w$CDM+$\sum m_{\nu }$ model $\beta =0$ is consistent with current observational data inside the 1$\sigma$ range, and in the IHDE+$\sum m_{\nu }$ model $\beta >0$ is favored at more than 2$\sigma$ level.

arXiv comment9 pages, 3 figures

References in corpus (139)

• Cosmological parameters from CMB and other data: a Monte-Carlo approach
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• 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
• A Model of Holographic Dark Energy
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Massive neutrinos and cosmology
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Final Results from phase II of the Mainz Neutrino Mass Search in Tritium $\beta$ Decay
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Search for neutrinoless double beta decay with enriched 76Ge in Gran Sasso 1990-2003
• Holographic Dark Energy
• Constraints on holographic dark energy from type Ia supernova observations
• Unveiling $\nu$ secrets with cosmological data: neutrino masses and mass hierarchy
• Large-scale instability in interacting dark energy and dark matter fluids
• Probing the Coupling between Dark Components of the Universe
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Indications of a late-time interaction in the dark sector
• Neutrino mass limit from tritium beta decay
• Evidence for massive neutrinos from CMB and lensing observations
• Holographic dark energy models: A comparison from the latest observational data
• Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
• 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
• Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
• Echo of interactions in the dark sector
• Neutrino mass from Cosmology
• $\nu \Lambda$CDM: Neutrinos help reconcile Planck with the Local Universe
• Sterile neutrinos in cosmology
• Towards a cosmological neutrino mass detection
• Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
• Reconstructing holographic quintessence
• Stability of the curvature perturbation in dark sectors' mutual interacting models
• Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12
• The $H_0$ tension in light of vacuum dynamics in the Universe
• Probing interaction and spatial curvature in the holographic dark energy model
• Hints of dynamical vacuum energy in the expanding Universe
• Possible signals of vacuum dynamics in the Universe
• Light sterile neutrinos
• Statefinder diagnosis for the interacting model of holographic dark energy
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Neutrino cosmology and Planck
• Parametrized Post-Friedmann Signatures of Acceleration in the CMB
• Reconstructing the interaction between dark energy and dark matter using Gaussian Processes
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• A new life for sterile neutrinos: resolving inconsistencies using hot dark matter
• Holographic tachyon model
• Neutrinos help reconcile Planck measurements with both Early and Local Universe
• Neutrino Mass Hierarchy
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• Holographic dark energy in a cyclic universe
• Parametrized Post-Friedmann Framework for Interacting Dark Energy
• Large-scale stable interacting dark energy model: Cosmological perturbations and observational constraints
• Comparison of dark energy models: A perspective from the latest observational data
• Search for sterile neutrinos in holographic dark energy cosmology: Reconciling Planck observation with the local measurement of the Hubble constant
• Constraining early and interacting dark energy with gravitational wave standard sirens: the potential of the eLISA mission
• Measuring neutrino masses with a future galaxy survey
• The KATRIN Neutrino Mass Experiment
• 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
• The strongest bounds on active-sterile neutrino mixing after Planck data
• 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
• Effects of neutrino mass hierarchies on dynamical dark energy models
• Testing models of vacuum energy interacting with cold dark matter
• Constraining interacting dark energy models with latest cosmological observations
• Covariantizing the interaction between dark energy and dark matter
• No new cosmological concordance with massive sterile neutrinos
• Comparison of dark energy models after Planck 2015
• Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
• 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?
• Heal the world: Avoiding the cosmic doomsday in the holographic dark energy model
• Impacts of dark energy on weighing neutrinos: mass hierarchies considered
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Additional Light Sterile Neutrinos and Cosmology
• Constraints on the neutrino mass and mass hierarchy from cosmological observations
• Impacts of dark energy on weighing neutrinos after Planck 2015
• Revisit of the Interaction between Holographic Dark Energy and Dark Matter
• Light sterile neutrinos after BICEP-2
• Coupled dark energy with perturbed Hubble expansion rate
• Weighing neutrinos in the scenario of vacuum energy interacting with cold dark matter: application of the parameterized post-Friedmann approach
• A search for sterile neutrinos with the latest cosmological observations
• Holographic dark energy in a universe with spatial curvature and massive neutrinos: a full Markov Chain Monte Carlo exploration
• Constraints on neutrino masses from Planck and Galaxy Clustering data
• Cosmological constraints on neutrinos after BICEP2
• Possible theoretical limits on holographic quintessence from weak gravity conjecture
• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Exploring neutrino mass and mass hierarchy in the scenario of vacuum energy interacting with cold dark matter
• Probing the imprint of interacting dark energy on very large scales
• Holographic Ricci dark energy: Interacting model and cosmological constraints
• Implications of observed neutrinoless double beta decay
• Probing the interaction between dark energy and dark matter with the parametrized post-Friedmann approach
• Gravitational clustering of cosmic relic neutrinos in the Milky Way
• Interacting model of new agegraphic dark energy: observational constraints and age problem
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Constraining neutrino mass and extra relativistic degrees of freedom in dynamical dark energy models using Planck 2015 data in combination with low-redshift cosmological probes: basic extensions to $\Lambda$CDM cosmology
• Neutrino constraints: what large-scale structure and CMB data are telling us?
• Cosmic age problem revisited in the holographic dark energy model
• Effects of time-varying $\beta$ in SNLS3 on constraining interacting dark energy models
• Prospects for Measurement of the Neutrino Mass Hierarchy
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Constraints on the sum of neutrino masses using cosmological data including the latest extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Constraining dynamical dark energy with a divergence-free parametrization in the presence of spatial curvature and massive neutrinos
• Redshift drift exploration for interacting dark energy
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• A closer look at interacting dark energy with statefinder hierarchy and growth rate of structure
• A model of interacting dark fluids tested with supernovae and Baryon Acoustic Oscillations data
• Weighing neutrinos in dynamical dark energy models
• Observational constraints on cosmic neutrinos and dark energy revisited
• Couplings between holographic dark energy and dark matter
• Relic Right-handed Dirac Neutrinos and Implications for Detection of Cosmic Neutrino Background
• Observational constraints on varying neutrino-mass cosmology
• 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
• Breaking parameter degeneracy in interacting dark energy models from observations
• Constraints on neutrino masses from the study of the nearby large-scale structure and galaxy cluster counts
• Statistical tests of sterile neutrinos using cosmology and short-baseline data
• Cosmological model of the interaction between dark matter and dark energy
• Measuring growth index in a universe with sterile neutrinos
• Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure
• New holographic dark energy model with non-linear interaction
• CMB and matter power spectra with non-linear dark-sector interactions
• New cosmological constraints with extended-Baryon Oscillation Spectroscopic Survey DR14 quasar sample
• Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
• Discriminating between Thermal and Nonthermal Cosmic Relic Neutrinos through Annual Modulation at PTOLEMY
• Tilt of primordial gravitational wave spectrum in a universe with sterile neutrinos
• The late Universe with non-linear interaction in the dark sector: the coincidence problem
• More on the holographic Ricci dark energy model: smoothing Rips through interaction effects?
• Constraining dynamical neutrino mass generation with cosmological data
• Constraints on neutrino masses from the lensing dispersion of Type Ia supernovae
• Interacting dark energy in the dark $SU(2{)}_R$ model
• Constraints on Cosmological Models from Hubble Parameters Measurements
• Observational constraints on running vacuum model

Cited by in corpus (32)

• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• The Gravitational-Wave Physics II: Progress
• Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
• Prospects for Constraining Interacting Dark Energy Models with 21 cm Intensity Mapping Experiments
• Constraints on active and sterile neutrinos in an interacting dark energy cosmology
• Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
• Probing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data
• Using a multi-messenger and multi-wavelength observational strategy to probe the nature of dark energy through direct measurements of cosmic expansion history
• 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
• Forecasting Interacting Vacuum-Energy Models using Gravitational Waves
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
• A forecast of using fast radio burst observations to constrain holographic dark energy
• Forecast for weighing neutrinos in cosmology with SKA
• Impacts of dark energy on constraining neutrino mass after Planck 2018
• Constraints on neutrino mass in the scenario of vacuum energy interacting with cold dark matter after Planck 2018
• Cosmological search for sterile neutrinos after Planck 2018
• IDECAMB: an implementation of interacting dark energy cosmology in CAMB
• Dark energy versus modified gravity: Impacts on measuring neutrino mass
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• Reconstructing a non-linear interaction in the dark sector with cosmological observations
• Prospects for weighing neutrinos in interacting dark energy models using joint observations of gravitational waves and $\gamma$-ray bursts
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Prospects for searching for sterile neutrinos with gravitational wave and $\gamma$-ray burst joint observations
• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Evolution of cosmological perturbations in the models with interacting dynamical dark energy
• Measuring neutrino mass in light of ACT DR6 and DESI DR2