Dark calling Dark: Interaction in the dark sector in presence of neutrino properties after Planck CMB final release

Abstract

We investigate a well known scenario of interaction in the dark sector where the vacuum energy is interacting with cold dark matter throughout the cosmic evolution in light of the cosmic microwave background (CMB) data from final Planck 2018 release. In addition to this minimal scenario, we generalize the model baseline by including the properties of neutrinos, such as the neutrino mass scale ($M_{\nu }$) and the effective number of neutrino species ($N_{\mathrm{eff}}$) as free parameters, in order to verify the possible effects that such parameters might generate on the coupling parameter, and vice versa. As already known, we again confirm that in light of the Planck 2018 data, such dark coupling can successfully solve the $H_0$ tension (with and without the presence of neutrinos). Concerning the properties of neutrinos, we find that $M_{\nu }$ may be wider than expected within the $\Lambda$CDM model and $N_{\mathrm{eff}}$ is fully compatible with three neutrino species (similar to $\Lambda$CDM prevision). The parameters characterizing the properties of neutrinos do not correlate with the coupling parameter of the interaction model. When considering the joint analysis of CMB from Planck 2018 and an estimate of $H_0$ from Hubble Space Telescope 2019 data, {\it we find an evidence for a non-null value of the coupling parameter at more than 3$\sigma$ confidence-level.} We also discuss the possible effects on the interacting scenario due to the inclusion of baryon acoustic oscillations data with Planck 2018. Our main results updating the dark sectors' interaction and neutrino properties in the model baseline, represent a new perspective in this direction. Clearly, a possible new physics in light of some dark interaction between dark energy and dark matter can serve as an alternative to $\Lambda$CDM scenario to explain the observable Universe, mainly in light of the current tension on $H_0$.

arXiv comment13 pages, 6 tables (3 tables in the main text and 3 tables in the appendix), 3 captioned figures; accepted for publication in JCAP

References in corpus (96)

• Planck 2015 results. XIII. Cosmological parameters
• 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 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Coupled Quintessence
• 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 vs. Conformal Newtonian Gauge
• Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
• Massive neutrinos and cosmology
• Holographic dark energy and cosmic coincidence
• Cosmological perturbations
• Transition of the dark energy equation of state in an interacting holographic dark energy model
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• An improved upper limit on the neutrino mass from a direct kinematic method by KATRIN
• 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
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Cosmology with Interaction between Phantom Dark Energy and Dark Matter and the Coincidence Problem
• Indications of a late-time interaction in the dark sector
• Super-acceleration as Signature of Dark Sector Interaction
• Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
• Cosmological Evolution With Interaction Between Dark Energy And Dark Matter
• Cosmologies with Energy Exchange
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• 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
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension
• Reconciling CMB and structure growth measurements with dark energy interactions
• Gauss-Bonnet Quintessence: Background Evolution, Large Scale Structure and Cosmological Constraints
• Dark coupling
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• On the improvement of cosmological neutrino mass bounds
• Interacting Dark Energy -- constraints and degeneracies
• New constraints on interacting dark energy from cosmic chronometers
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• Updated results on neutrino mass and mass hierarchy from cosmology with Planck 2018 likelihoods
• Interacting models may be key to solve the cosmic coincidence problem
• Toward a solution of the coincidence problem
• Cosmological constraints in extended parameter space from the Planck 2018 Legacy release
• Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data
• Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios
• Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models
• Observational constraints on sign-changeable interaction models and alleviation of the $H_0$ tension
• Effective Theory of Interacting Dark Energy
• Adiabatic initial conditions for perturbations in interacting dark energy models
• An analytic model for interacting dark energy and its observational constraints
• A new interacting two fluid model and its consequences
• Astronomical bounds on a cosmological model allowing a general interaction in the dark sector
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Disformal couplings and the dark sector of the universe
• Impact of neutrino properties on the estimation of inflationary parameters from current and future observations
• Interacting quintessence from a variational approach Part II: derivative couplings
• Dark sectors with dynamical coupling
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Testing coupled dark energy with large scale structure observation
• Interacting quintessence from a variational approach Part I: algebraic couplings
• A model with interaction of dark components and recent observational data
• Quantum Field Theory of Interacting Dark Matter/Dark Energy: Dark Monodromies
• Effects of neutrino mass hierarchies on dynamical dark energy models
• 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
• Effects of Anisotropic Stress in Interacting Dark Matter - Dark Energy Scenarios
• Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models
• Bias due to neutrinos must not uncorrect'd go
• Constraining a dark matter and dark energy interaction scenario with a dynamical equation of state
• Dynamics of interacting quintessence
• Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?
• In search of the dark matter dark energy interaction: a kinematic approach
• Scalar-field dark energy nonminimally and kinetically coupled to dark matter
• Post-$Planck$ constraints on interacting vacuum energy
• 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
• Dynamics of nonlinear interacting dark energy models
• Cosmological constraints on an exponential interaction in the dark sector
• 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
• A cosmographic analysis of holographic dark energy models
• Search for sterile neutrinos in a universe of vacuum energy interacting with cold dark matter
• Matter bounce cosmology with a generalized single field: non-Gaussianity and an extended no-go theorem
• Dark matter-dark energy interaction for a time-dependent equation of state
• Will there be again a transition from acceleration to deceleration in course of the dark energy evolution of the universe?
• Exacerbating the cosmological constant problem with interacting dark energy
• Dynamics of coupled phantom and tachyon fields
• Hiding neutrino mass in modified gravity cosmologies
• The cosmology of minimal varying Lambda theories
• Exploring neutrino mass and mass hierarchy in interacting dark energy models
• Probing the properties of relic neutrinos using the cosmic microwave background, the Hubble Space Telescope and galaxy clusters
• Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
• Forecast on lepton asymmetry from future CMB experiments

Cited by in corpus (71)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
• 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
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• 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
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Interacting Dark Energy in a closed universe
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Dark sector interaction and the supernova absolute magnitude tension
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• All-inclusive interacting dark sector cosmologies
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal
• Soundness of Dark Energy properties
• Revealing the effects of curvature on the cosmological models
• Late time interacting cosmologies and the Hubble constant tension
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• 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
• A double take on early and interacting dark energy from JWST
• A fake Interacting Dark Energy detection?
• Understanding the phenomenology of interacting dark energy scenarios and their theoretical bounds
• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• Scaling solutions and weak gravity in dark energy with energy and momentum couplings
• Dynamical Dark sectors and Neutrino masses and abundances
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Metastable dark energy models in light of Planck 2018: Alleviating the $H_0$ tension
• Dynamics in Varying vacuum Finsler-Randers Cosmology
• Touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension
• Dark Energy as a Critical Phenomenon: a Resolution for Hubble Tension
• General formulation of cosmological perturbations in scalar-tensor dark energy coupled to dark matter
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Interacting quintessence in light of Generalized Uncertainty Principle: Cosmological perturbations and dynamics
• Probing Interacting Dark Energy and Scattering of Baryons with Dark Matter in Light of EDGES 21cm Signal
• J-PAS: forecasts on interacting vacuum energy models
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• Interacting dark sector from the trace-free Einstein equations: cosmological perturbations with no instability
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• 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
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• The Integrated Sachs-Wolfe Effect in Interacting Dark Matter-Dark Energy Models
• CMB lensing in a modified $\Lambda$CDM model in light of the $H_0$ tension
• Structure Formation in Various Dynamical Dark Energy Scenarios
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Late-time Background Constraints on Linear and Non-linear Interacting Dark Energy after DESI DR2
• Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae
• Global asymptotic dynamics of the cubic galileon interacting with dark matter
• Chaotic interactions between dark matter and dark energy
• Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity
• Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
• Variational symmetries and superintegrability in multifield cosmology
• Vainshtein screening in Horndeski theories nonminimally and kinetically coupled to ordinary matter
• 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
• Probing Interacting Dark Sectors with upcoming Post-Reionization and Galaxy Surveys
• Some Classes of Interacting Two-Fluid Model of the Expanding Universe