Saved in:
Bibliographic Details
Main Authors: Amani, Alireza, Kubeka, A. S., Mahichi, E.
Format: Preprint
Published: 2023
Subjects:
Online Access:https://arxiv.org/abs/2308.05130
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866910015729696768
author Amani, Alireza
Kubeka, A. S.
Mahichi, E.
author_facet Amani, Alireza
Kubeka, A. S.
Mahichi, E.
contents In this paper, we model the bounce phase, stability, and the reconstruction of the universe by non-minimal kinetic coupling. In the process, we obtained importance information about the energy density and the matter pressure of the universe in relation to the previous universe through the bounce quantum phase. The novelty of the work is that the scale factor is obtained directly from the model and is fitted with an exponential function, with this view we explore the process of the early universe even the bounce phase. After that, we plot the cosmological parameters in terms of time evolution. In what follows, we investigate the stability of the model by dynamical system analysis in a phase plane. Finally, we examine the stability of the universe, especially in the inflationary period, by using the phase-space trajectories.
format Preprint
id arxiv_https___arxiv_org_abs_2308_05130
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Cosmological Evolution and Stability of a Bouncing Universe with Non-Minimal Kinetic Coupling Gravity
Amani, Alireza
Kubeka, A. S.
Mahichi, E.
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this paper, we model the bounce phase, stability, and the reconstruction of the universe by non-minimal kinetic coupling. In the process, we obtained importance information about the energy density and the matter pressure of the universe in relation to the previous universe through the bounce quantum phase. The novelty of the work is that the scale factor is obtained directly from the model and is fitted with an exponential function, with this view we explore the process of the early universe even the bounce phase. After that, we plot the cosmological parameters in terms of time evolution. In what follows, we investigate the stability of the model by dynamical system analysis in a phase plane. Finally, we examine the stability of the universe, especially in the inflationary period, by using the phase-space trajectories.
title Cosmological Evolution and Stability of a Bouncing Universe with Non-Minimal Kinetic Coupling Gravity
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2308.05130