Attractor behaviour of modified gravity and the cosmic acceleration
arXiv:2303.09076 · doi:10.1016/j.dark.2024.101461
Abstract
In this paper, we have performed the dynamical system analysis of gravity cosmological models at both background and perturbation levels. We have presented three models pertaining to three distinct functional forms of . The first form is that of the logarithmic form of the torsion scalar , the second one is in the power law form, and the third one is the combination of the first two forms. For all these three forms of , we have derived the corresponding cosmological parameters in terms of the dynamical variables. Subsequently, the critical points are obtained and the condition(s) of its existence has been derived. Critical points of each model have been analysed individually and the corresponding cosmology are derived. The stability behaviour of these critical points are discussed from the behaviour of the eigenvalues and the phase portraits. At least one stable node has been obtained in each of these models. Further from the evolution plots of the cosmological parameters, the accelerating behaviour of the cosmological models are also verified.
14 pages, 9 figures, Accepted version Physics of the Dark Universe
References in corpus (26)
- Dynamics of dark energy
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Extended Gravity Cosmography
- f(T) gravity mimicking dynamical dark energy. Background and perturbation analysis
- gravity and cosmology
- Teleparallel equivalent of Gauss-Bonnet gravity and its modifications
- Good and bad tetrads in f(T) gravity
- Growth factor in f(T) gravity
- Cosmological Solutions of Gravity
- Cosmology in gravity: A unified dynamical system analysis at background and perturbation levels
- Dynamical system analysis for accelerating models in non-metricity gravity
- Dynamical systems approach and generic properties of cosmology
- Dynamical Stability Analysis of Accelerating f(T) Gravity Models
- Stability of the flat FLRW metric in gravity
- No constraints for gravity from gravitational waves induced from primordial black hole fluctuations
- Gauge Structure of Teleparallel Gravity
- Quasinormal modes of black holes in f(T) gravity
- Dynamical systems analysis in gravity
- Matter Bounce Scenario in Extended Symmetric Teleparallel Gravity
- Analyzing the geometrical and dynamical parameters of modified Teleparallel-Gauss-Bonnet model
- Dynamical complexity of the Teleparallel gravity cosmology
- Cosmological models in gravity and the dynamical system analysis
- Generalized Teleparallel de Sitter geometries
- Teleparallel Robertson-Walker geometries and applications
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- Scalar field induced dynamical evolution in teleparallel gravity
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- Cosmological Dynamics in Interacting Scalar-Torsion f(T,) Gravity: Investigating Energy and Momentum Couplings
- Dynamical system analysis in modified Galileon cosmology
- Dynamical System Analysis for Scalar Field Potential in Teleparallel Gravity
- The scalar-torsion gravity corrections in the first-order inflationary models
- Late Time Phenomena in Gravity Framework: Role of Priors
- Exact Analytical Taub-NUT like Solution in f(T) Gravity
- Scalar Field Static Spherically Symmetric Solutions in Teleparallel Gravity