Observational constraints on the interacting dark energy - dark matter (IDM) cosmological models

Abstract

Particle creation (or annihilation) mechanisms, described by either quantum field theoretical models, or by the thermodynamics of irreversible processes, play an important role in the evolution of the early Universe, like, for example, in the warm inflationary scenario. Following a similar approach, based on the thermodynamics of open systems, in the present work we investigate the consequences of the interaction, decay, and particle generation in a many-component Universe, containing dark energy, dark matter, radiation, and ordinary matter, respectively. In this model, due to the interaction between these components, and of the corresponding thermodynamical properties, the conservation equations of different cosmological constituents are not satisfied individually. We introduce a thermodynamic description of the Universe, in which two novel physical aspects, the particle number balance equations, and the creation pressures, are considered, thus making the cosmological evolution equations thermodynamically consistent. To constrain the free parameters of the model several observational data sets are employed, including the Planck data sets, Riess 2020, BAO, as well as Pantheon data. By using a scaling ansatz for the dark matter to dark energy ratio, and by imposing constraints from Planck+Riess 2020 data, this model predicts an acceptable value for the Hubble parameter, and thus it may provide a solution to the so-called Hubble tension problem, much debated recently.

29+1 pages, 9 figures including subfigures, 2 tables; Published version

References in corpus (89)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The Cosmological Constant and Dark Energy
• Cosmological Imprint of an Energy Component with General Equation of State
• Cosmological Constant - the Weight of the Vacuum
• 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
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• 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
• New Constraints on ${\Omega }_M$, ${\Omega }_{\Lambda }$, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
• Observational Probes of Cosmic Acceleration
• Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
• MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Beyond the Cosmological Standard Model
• Planck 2018 results. V. CMB power spectra and likelihoods
• Improved Dark Energy Constraints from ~100 New CfA Supernova Type Ia Light Curves
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• Two new diagnostics of dark energy
• Scaling solutions in general non-minimal coupling theories
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Dark Energy vs. Modified Gravity
• $f(Q,T)$ gravity
• Large-scale instability in interacting dark energy and dark matter fluids
• The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
• The Dark Matter Distribution in Disk Galaxies
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Thermodynamic interpretation of the generalized gravity models with geometry - matter coupling
• Dark matter and the early Universe: a review
• Dark Matter and Background Light
• Likely Values of the Cosmological Constant
• Hubble Sinks In The Low-Redshift Swampland
• Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant
• Effective Field Theory of Dark Energy: a Review
• Testing the Cosmic Coincidence Problem and the Nature of Dark Energy
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• Scaling Cosmology
• Scalar--Tensor Theories of Gravity with \PHI Dependent Masses
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Matter creation in a nonsingular bouncing cosmology
• Palatini formulation of $f(R,T)$ gravity theory, and its cosmological implications
• An Accelerating Cosmology Without Dark Energy
• Inflationary Models Driven by Adiabatic Matter Creation
• On phenomenological models of dark energy interacting with dark matter
• Unified dark energy thermodynamics: varying w and the -1-crossing
• Cosmological consequences of an adiabatic matter creation process
• Newtonian Perturbations on Models with Matter Creation
• $Om$ diagnostic applied to scalar field models and slowing down of cosmic acceleration
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Dark Energy Survey Year 3 Results: Clustering Redshifts -- Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS
• Covariantizing the interaction between dark energy and dark matter
• Brief Review of Recent Advances in Understanding Dark Matter and Dark Energy
• The Higgs Portal to Cosmology
• Phase structure of the massive chiral Gross-Neveu model from Hartree-Fock
• Inflation with a graceful exit and entrance driven by Hawking radiation
• In search of the dark matter dark energy interaction: a kinematic approach
• CMB constraints on interacting cosmological models
• The effect of Dark Matter and Dark Energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect
• Cosmological evolution and dark energy in osculating Barthel-Randers geometry
• Forecasting the Interaction in Dark Matter-Dark Energy Models with Standard Sirens From the Einstein Telescope
• Is the continuous matter creation cosmology an alternative to $\Lambda$CDM?
• Non-minimal geometry-matter couplings in Weyl-Cartan space-times: $f(R,T,Q,T_m)$ gravity
• New physics of strong interaction and Dark Universe
• Constraining the dark matter-vacuum energy interaction using the EDGES 21-cm absorption signal
• Probing superheavy dark matter with gravitational waves
• Velocity-dependent interacting dark energy and dark matter with a Lagrangian description of perfect fluids
• Non-minimal Derivative Coupling Scalar Field and Bulk Viscous Dark Energy
• Gravitationally Induced Particle Production through a Nonminimal Torsion-Matter Coupling
• Constraints on the dark matter and dark energy interactions from weak lensing bispectrum tomography
• Cosmological dynamics of interacting dark energy and dark matter in viable models of f(R) gravity
• Dark Matter-Dark Energy Interaction and the Shape of Cosmic Voids
• Hawking Radiation as a Mechanism for Inflation
• Irreversible thermodynamical description of warm inflationary cosmological models
• Dynamics of Dirac-Born-Infeld dark energy interacting with dark matter
• Continuous matter creation and the acceleration of the universe: the growth of density fluctuations
• Scalar perturbations in cosmological models with dark energy - dark matter interaction
• Does the diffusion DM-DE interaction model solve cosmological puzzles?
• Cosmological Constraints on Entropic Cosmology with Matter Creation
• On the Cosmological Models with Matter Creation
• Holographic field theory models of dark energy in interaction with dark matter
• Falsifying Cosmological Constant
• Gamma-Ray Bursts and Dark Energy - Dark Matter interaction
• Testing CCDM Cosmology with the Radiation Temperature-Redshift Relation

Cited by in corpus (8)

• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• A model of dark matter dark energy interaction with some cosmic consequences
• Observational Constraints on the Dark Energy with a Quadratic Equation of State
• Hybrid star within $f(\mathcal{G})$ gravity
• Anisotropic Conformal Dark Gravity on the Lorentz Tangent Bundle Spacetime
• Interacting Dark Energy and Its Implications for Unified Dark Sector