Correction to Lagrangian for Bouncing Cosmologies in Gravity
arXiv:2304.10245 · doi:10.1140/epjc/s10052-023-11798-z
Abstract
Symmetric teleparallel gravity offers to reformulate the gravitational formalism without the presence of curvature and torsion with the help of non-metricity tensors. Interestingly, Symmetric teleparallel gravity can be formulated equivalently to teleparallel gravity or general relativity for an appropriate setup. In this study, our aim lies in exploring the bouncing cosmologies as an alternative to the initial singularity of the Universe in the background of modified symmetric teleparallel gravity. To explore this, we adopt the reconstruction technique to present the possible reconstructed Lagrangian for various cosmological bouncing solutions in a flat Friedmann-Lemaître-Robertson-Walker spacetime with a perfect fluid matter distribution. We study the reconstructed gravitational Lagrangians, which are capable of reproducing analytical solutions for \textit{symmetric bounce}, \textit{super-bounce}, \textit{oscillatory bounce}, \textit{matter bounce}, and \textit{exponential bouncing} model settings. Further, we examine the dark energy profiles of the models using reconstructed Lagrangians. In addition, we found that an additional term arises in each reconstructed Lagrangian compared to general relativity (GR). That extra term corrected the background GR to present bouncing cosmology in modified gravity. These newly motivated cosmological models may have an effect on gravitational phenomena at other cosmological scales.
EPJ C revised version
References in corpus (19)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Quantum Nature of the Big Bang: Improved dynamics
- Towards a Nonsingular Bouncing Cosmology
- Bouncing Universe with Quintom Matter
- Exploring Bouncing Cosmologies with Cosmological Surveys
- A geometric perspective on singularity resolution and uniqueness in loop quantum cosmology
- Consistency of holonomy-corrected scalar, vector and tensor perturbations in Loop Quantum Cosmology
- New models and Big Bang Nucleosynthesis constraints in gravity
- Matter creation in a nonsingular bouncing cosmology
- Cosmological bouncing solutions in f(T,B) gravity
- Barotropic index w-singularities in cosmology
- A designer approach to gravity and cosmological implications
- On the impact of gravity on the Large Scale Structure
- Isotropization of locally rotationally symmetric Bianchi-I universe in -gravity
- Reconstruction of CDM Universe in Gravity
- Crossing phantom divide in gravity
- How can holonomy corrections be introduced in gravity?
- Structure formation in gravity: A distinguishing probe between the dark energy and modified gravity
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- Modified gravity models and their cosmological consequences
- Tensor Perturbations from Bounce Inflation Scenario in f(Q) Gravity
- Constraining Exponential f(Q) Gravity with Cosmic Chronometers and Supernovae: A Data-Driven Analysis
- Reconstruction of the singularity-free gravity via Raychaudhuri equations
- Dynamical systems analysis of a cosmological model with interacting Umami Chaplygin fluid in adiabatic particle creation mechanism: Some bouncing features
- Vulnerability of f(Q) gravity theory and a possible resolution
- Beyond the Cosmological Constant: Breaking the Geometric Degeneracy of cosmology via Redshift-Space Distortions
- Scale-Invariant Bounce Cosmology in Weyl f(Q) Gravity with Quintom Signature