Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?

Abstract

We propose a revised cosmological scenario that extends the $\Lambda$ Cold Dark Matter ($\Lambda$CDM) framework by incorporating metric $f(R)$ gravity in the Jordan frame. In this model, the dark energy component arises from a non-minimally coupled scalar field, decomposed into a smooth background (set to unity to recover General Relativity) and a rapidly varying, massive fluctuation that decays into the dark matter sector. In the near-GR limit, this setup provides a phenomenological extension of $\Lambda$CDM characterized by two additional parameters: the present-day value of the scalar fluctuation and a normalized decay rate. Using a Markov Chain Monte Carlo analysis of low-redshift cosmological data, comprising Type Ia Supernovae, Baryon Acoustic Oscillation (BAO), and Cosmic Chronometer measurements, we find that the proposed model achieves a better overall fit than $\Lambda$CDM, while the Bayesian evidence remains statistically inconclusive given the inclusion of two extra parameters. The model predicts a moderate increase in the inferred value of $H_0$ and an improved consistency with DESI BAO data when adopting the SH0ES prior. Furthermore, describing dark matter particle creation as a transition phase in the late Universe offers an intriguing physical interpretation, potentially capturing features already present in current data and providing a promising avenue to explore extensions of the standard cosmological model within modified gravity frameworks.

arXiv comment15 pages, 2 figures

References in corpus (112)

• f(R) Theories Of Gravity
• Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
• Extended Theories of Gravity
• Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
• 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
• dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences
• In the Realm of the Hubble tension $-$ a Review of Solutions
• Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
• Multimodal nested sampling: an efficient and robust alternative to MCMC methods for astronomical data analysis
• Planck 2018 results. I. Overview and the cosmological legacy of Planck
• The Pantheon+ Analysis: Cosmological Constraints
• Tensions between the Early and the Late Universe
• Early Dark Energy Can Resolve The Hubble Tension
• Importance Nested Sampling and the MultiNest Algorithm
• The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
• Challenges for $\Lambda$CDM: An update
• The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Cosmology Intertwined II: The Hubble Constant Tension
• New physics in light of the $H_0$ tension: an alternative view
• The $H_0$ Olympics: A fair ranking of proposed models
• Can interacting dark energy solve the $H_0$ tension?
• On the Hubble constant tension in the SNe Ia Pantheon sample
• Post-Newtonian constraints on f(R) cosmologies in Palatini formalism
• Post-Newtonian constraints on f(R) cosmologies in metric formalism
• Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
• 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 gravity lagrangian according to solar system experiments
• Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix
• On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030
• Echo of interactions in the dark sector
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• New Early Dark Energy
• Reconciling CMB and structure growth measurements with dark energy interactions
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Reducing the $H_0$ and ${\sigma }_8$ tensions with Dark Matter-neutrino interactions
• Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant
• New constraints on interacting dark energy from cosmic chronometers
• Is there an early Universe solution to Hubble tension?
• A Vacuum Phase Transition Solves $H_0$ Tension
• Dark Energy with Phantom Crossing and the $H_0$ tension
• Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
• Massive gravitational waves from f(R) theories of gravity: Potential detection with LISA
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• Assessing observational constraints on dark energy
• Constraints on the Coupling between Dark Energy and Dark Matter from CMB data
• Relaxing cosmological tensions with a sign switching cosmological constant
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Interpreting DESI's evidence for evolving dark energy
• Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
• Beyond $\Lambda$CDM with Low and High Redshift Data: Implications for Dark Energy
• Quintessential interpretation of the evolving dark energy in light of DESI
• Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension
• Dark Energy at early times and ACT: a larger Hubble constant without late-time priors
• Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0{w}_a$CDM cosmological parameterization result
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Finite-time Cosmological Singularities and the Possible Fate of the Universe
• Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
• Relieving the $H_0$ tension with a new interacting dark energy model
• Dark sector interaction and the supernova absolute magnitude tension
• All-inclusive interacting dark sector cosmologies
• An overview of what current data can (and cannot yet) say about evolving dark energy
• Evidence of a decreasing trend for the Hubble constant
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
• Sensitivity of the Hubble Constant Determination to Cepheid Calibration
• Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Omnipotent dark energy: A phenomenological answer to the Hubble tension
• The Hubble Tension Revisited: Additional Local Distance Ladder Uncertainties
• Late time transitions in the quintessence field and the $H_0$ tension
• $f(R)$ gravity in the Jordan Frame as a Paradigm for the Hubble Tension
• Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy
• Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae
• A double take on early and interacting dark energy from JWST
• Dark degeneracy I: Dynamical or interacting dark energy?
• Hot New Early Dark Energy
• A fake Interacting Dark Energy detection?
• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• Interacting dark energy: clarifying the cosmological implications and viability conditions
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• Composite Dark Energy and the Cosmological Tensions
• Inflation, the Hubble Tension and Early Dark Energy: an alternative overview
• Gauge invariant formulation of gravitational waves in metric $f(R)$ gravity
• Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
• Metric $f(R)$ gravity with dynamical dark energy as a scenario for the Hubble tension
• Phenomenological emergent dark energy in the light of DESI Data Release 1
• Slow-rolling scalar dynamics and as solution for the Hubble tension
• Dynamical dark energy in the light of DESI 2024 data
• Minimal dark energy: key to sterile neutrino and Hubble constant tensions?
• Dynamical dark energy confronted with multiple CMB missions
• Cold New Early Dark Energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients
• Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters
• Cosmological implications of an interacting model of dark matter \& dark energy
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Observational Constraints on Dark Energy Models with $\Lambda$ as an Equilibrium Point
• Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
• Dynamical Dark Energy in the Crosshairs: A Joint Analysis with DESI, Pantheon plus, and TDCOSMO Constraints
• Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
• Modified gravity in the presence of matter creation: scenario for the late Universe
• Reassessing the Constraints from SH0ES Extragalactic Cepheid Amplitudes on Systematic Blending Bias
• Perturbations of Single-field Inflation in Modified Gravity Theory
• The effective running Hubble constant in SNe Ia as a marker for the dark energy nature
• Quantum Dynamics of the Isotropic Universe in the Metric f(R) Gravity
• Two Dynamical Scenarios for Binned Master Sample Interpretation
• Decay of dark energy into dark matter in a metric $f(R)$ gravity: effective running Hubble constant
• On the emergence of a classical Isotropic Universe from a Quantum $f(R)$ Bianchi Cosmology in the Jordan Frame

Cited by in corpus (5)

• Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions
• Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity
• Hubble Tension and Dark Energy in Teleparallel Gauss-Bonnet Gravity: New Constraints from DESI BAO, Pantheon${}^{+}$ and Hubble Data
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Running Hubble Constant with the Redshift as a Marker of Evolutionary Dark Energy