Matter Bounce Scenario in Extended Symmetric Teleparallel Gravity
arXiv:2206.02783 · doi:10.1140/epjc/s10052-023-11266-8
Abstract
In this paper, we have shown the matter bounce scenario of the Universe in an extended symmetric teleparallel gravity, the f(Q) gravity. Motivated from the bouncing scenario and loop quantum cosmology (LQC), the form of the function has been obtained at the backdrop of Friedmann-Lemaitre-Robertson Walker (FLRW) space time. Considering the background cosmology dominated by dust fluid, the e-folding parameter has been expressed, which contains the nonmetricity term. Since the slow roll criterion in the bouncing context is not valid, we used a conformal equivalence between f(Q) and scalar-tensor model to apply the bottom-up reconstruction technique in the bouncing model. The dynamics of the model has been studied through the phase space analysis, where both the stable and unstable nodes are obtained. Also, the stability analysis has been performed with the first order scalar perturbation of the Hubble parameter and matter energy density to verify the stability of the model.
10 pages, 6 figures
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Cited by in corpus (19)
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- Attractor behaviour of modified gravity and the cosmic acceleration
- Dynamical system analysis in teleparallel gravity with boundary term
- Cosmological implications of the constant jerk parameter in gravity theory
- Energy condition bounds on model parameters in a curved FLRW universe
- Gravity Bouncing Universe with Cosmological Parameters
- Cosmological models in gravity and the dynamical system analysis
- The dynamics of matter bounce cosmology in Weyl-type gravity
- A new cosmological model with quadratic expansion
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