Particle Production Scenario in an Algebraically Coupled Quintessence Field with a Dark Matter Fluid
arXiv:2403.10215 · doi:10.1016/j.cjph.2025.06.009
Abstract
We investigate the dynamics of an algebraically coupled quintessence field with a dark matter fluid, focusing on particle production through the action principle via a modified interaction Lagrangian. The interaction parameter serves as the source of dark matter particle production and entropy generation. As particle creation occurs due to the interaction between the field and fluid sectors, the system exhibits additional pressure. Our analysis includes studying the system's dynamics by considering an exponential type of interaction corresponding to the field's exponential potential. We assess the system's background dynamics using the dynamical system stability technique to derive the constraints on the model parameters. Additionally, we determine the best-fit values of the model parameters against two combinations of data sets: (i) CC+Pantheon+SH0ES, and (ii) CC+Pantheon+SH0ES+SDSS BAO+ DESI BAO. By employing a comprehensive data analysis technique, we compare the evidence of our models to flat CDM. Based on the Akaike Information Criterion (AIC) and Bayesian Information Criterion (BIC), one of the models emerges as a robust alternative to CDM when considering the joint data sets.
arXiv comment32 pages, 16 figures, and 5 tables. Accepted for the publication in Chinese Journal of Physics
References in corpus (97)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- emcee: The MCMC Hammer
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- f(R) Theories Of Gravity
- Cosmological Constant - the Weight of the Vacuum
- An alternative to quintessence
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- In the Realm of the Hubble tension a Review of Solutions
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- Essentials of k-essence
- Coupled Quintessence
- f(T) teleparallel gravity and cosmology
- Exponential potentials and cosmological scaling solutions
- Kinetically Driven Quintessence
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- The Pantheon+ Analysis: Cosmological Constraints
- Bayes in the sky: Bayesian inference and model selection in cosmology
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Coincident General Relativity
- The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
- The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
- Gauss-Bonnet dark energy
- Scaling solutions in general non-minimal coupling theories
- Interacting quintessence solution to the coincidence problem
- New physics in light of the tension: an alternative view
- Interacting Dark Matter and Dark Energy
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Action functionals for relativistic perfect fluids
- Non-minimal dark sector physics and cosmological tensions
- Large-scale instability in interacting dark energy and dark matter fluids
- Tale of stable interacting dark energy, observational signatures, and the tension
- Nonminimal coupling of perfect fluids to curvature
- Bulk Viscous Cosmology
- Hubble Parameter and Baryon Acoustic Oscillation Measurement Constraints on the Hubble Constant, the Deviation from the Spatially-Flat cdm Model, The Deceleration-Acceleration Transition Redshift, and Spatial Curvature
- Aspects of the cosmological "coincidence problem"
- Linear and non-linear perturbations in dark energy models
- Hydrodynamical N-body simulations of coupled dark energy cosmologies
- Dos and don'ts of reduced chi-squared
- Observational constraints on an interacting dark energy model
- Interacting Dark Energy -- constraints and degeneracies
- Statefinder parameters for interacting dark energy
- Update on Coupled Dark Energy and the tension
- Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements
- Is there an early Universe solution to Hubble tension?
- A New Perspective on Cosmic Coincidence Problems
- Cosmological coincidence problem in interacting dark energy models
- Coupled Quintessence in a Power-Law Case and the Cosmic Coincidence Problem
- Late time acceleration in Brans Dicke Cosmology
- Cosmological constraints on Brans-Dicke theory
- Brans-Dicke gravity with a cosmological constant smoothes out CDM tensions
- String-inspired cosmology: Late time transition from scaling matter era to dark energy universe caused by a Gauss-Bonnet coupling
- Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation
- Observational constraints on sign-changeable interaction models and alleviation of the tension
- Adiabatic initial conditions for perturbations in interacting dark energy models
- Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835
- Cosmological particle production, causal thermodynamics, and inflationary expansion
- Constraints on Dark Energy from Supernovae, Gamma Ray Bursts, Acoustic Oscillations, Nucleosynthesis and Large Scale Structure and the Hubble constant
- New Cosmic Accelerating Scenario without Dark Energy
- On phenomenological models of dark energy interacting with dark matter
- Cosmological models and centre manifold theory
- Cosmological consequences of an adiabatic matter creation process
- Relativistic fluid dynamics: physics for many different scales
- Scalar-Fluid theories: cosmological perturbations and large-scale structure
- Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum
- On the homogeneity of SnIa absolute magnitude in the Pantheon+ sample
- On the dynamics of perfect fluids in non-minimally coupled gravity
- Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
- Phantom dark energy with varying-mass dark matter particles: acceleration and cosmic coincidence problem
- Can redshift errors bias measurements of the Hubble Constant?
- Late time interacting cosmologies and the Hubble constant tension
- Scalar-field dark energy nonminimally and kinetically coupled to dark matter
- Quantifying the tension and evidence for interacting dark energy from redshift-space distortion measurements
- Model-independent limits and constraints on extended theories of gravity from cosmic reconstruction techniques
- Nonsingular Decaying Vacuum Cosmology and Entropy Production
- Thermodynamical aspects of running vacuum models
- Testing Gravity on Cosmic Scales: A Case Study of Jordan-Brans-Dicke Theory
- First Detection of the BAO Signal from Early DESI Data
- Scaling solutions from interacting fluids
- Dark energy with a gradient coupling to the dark matter fluid: cosmological dynamics and structure formation
- Cosmological particle production and generalized thermodynamic equilibrium
- Dynamical stability of K-essence field interacting non-minimally with a perfect fluid
- Challenging matter creation models in the phantom divide
- Dynamics of non-minimally coupled perfect fluids
- Dynamical systems analysis of tachyon dark energy model from a new perspective
- Dynamical stability in models where dark matter and dark energy are non-minimally coupled to curvature
- Dynamical Stability in presence of non-minimal derivative dependent coupling of -essence field with a relativistic fluid
- Constraining constant and tomographic coupled dark energy with low-redshift and high-redshift probes
- Phase-space of flat Friedmann-Robertson-Walker models with both a scalar field coupled to matter and radiation
- Cosmological Constraints on the Coupling Model from Observational Hubble Parameter and Baryon Acoustic Oscillation Measurements
- Scaling solutions in quintessential inflation
- Stability analysis of warm quintessential dark energy model
- Investigating The Hubble Tension Through Hubble Parameter Data
- On the Cosmological Models with Matter Creation
- On a class of scaling FRW cosmological models