Phase space analysis of an exponential model in gravity including linear dark-sector interactions
arXiv:2510.12020 · doi:10.1140/epjc/s10052-026-15313-y
Abstract
We present a cosmological analysis of an exponential gravity model, within the dynamical systems formalism. Following the method introduced by Böhmer \textit{et al} [Universe \textbf{9} no.4, 166 (2023)], the modified Friedmann modified equations are successfully reduced to an autonomous system. Given the exponential form of , the equilibrium conditions result in transcendental equations, which we approximate to identify the critical points. We therefore perform a general stability analysis of these points in terms of the model parameters. Finally, we extend the model by including a linear dark energy-dark matter interaction, where the equilibrium points are found with their stability properties. The model exhibits the three main domination epochs in the Universe, as well as a non-trivial impact on the late-time de Sitter attractor.
22 pages, 12 figures
References in corpus (42)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- The Case for a Positive Cosmological Lambda-term
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- The Pantheon+ Analysis: Cosmological Constraints
- Coincident General Relativity
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Conditions for the cosmological viability of f(R) dark energy models
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- Cosmology in geometry
- Teleparallel Gravity: From Theory to Cosmology
- Dynamical systems applied to cosmology: dark energy and modified gravity
- Cosmological solutions and growth index of matter perturbations in gravity
- First evidence that non-metricity f(Q) gravity could challenge CDM
- The Null Energy Condition and its violation
- Signatures of -gravity in cosmology
- Observational constraints on cosmological solutions of theories
- Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
- Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry
- Cosmology in gravity: A unified dynamical system analysis at background and perturbation levels
- Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data
- New models and Big Bang Nucleosynthesis constraints in gravity
- Is exponential gravity a viable description for the whole cosmological history?
- Cosmological observational constraints on the power law type modified gravity theory
- Phantom cosmological model with observational constraints in gravity
- Phase-space analysis of a novel cosmological model in theory
- Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions
- Dynamical systems analysis of gravity
- Cosmological dynamical systems in modified gravity
- Flat FLRW Universe in logarithmic symmetric teleparallel gravity with observational constraints
- Exploring the stability of cosmology near general relativity limit with different connections
- A new cosmological model with quadratic expansion
- Cosmological constraints on dynamical dark energy model in gravity
- Structure growth in cosmology
- Modified gravity with an exponential function of curvature
- Cosmological dynamics and observational constraints on a viable non-metric gravity model
- Analysis of the cosmological evolution parameters, energy conditions, and linear matter perturbations of an exponential-type model in gravity
- How Much NEC Breaking Can the Universe Endure?
- A Unified Dynamical Systems Framework for Cosmology in Gravity: Generic Features Beyond the Coincident Gauge