Stability of the Einstein Static Universe in Zero-Point Length Cosmology with Topological Defects
Kalyan Bhuyan, Mrinnoy M. Gohain

TL;DR
This paper investigates the stability of the Einstein static universe within zero-point length cosmology, considering topological defects, and analyzes how these factors influence the universe's transition to inflation through various perturbation stability tests.
Contribution
It introduces a generalized framework incorporating topological defects into zero-point length cosmology and analyzes their impact on the stability of the Einstein static universe.
Findings
Model parameters influence phase transition stability.
Mutual interplay between zero-point length and defect dimension affects stability.
ESU remains stable against vector and tensor perturbations.
Abstract
Recently, zero-point length cosmology has shown some positive insights into some non-singular aspects of the early Universe. In addition, topological defects are known to play a significant role by its presence as a part of the total energy in the very early Universe. We investigate the stability issue of the Einstein static phase in the emergent scenario of the Universe in a generalized framework of zero-point length cosmology in the presence of topological defects in the very early times. We derive the modified Friedmann equations, where the matter sector includes an extra energy density term arising from -dimensional topological defects. We have studied the possibility of graceful exit of emergent scenario and its stability using dynamical system analysis and against homogeneous scalar perturbation. We also analysed the stability against inhomogeneous density perturbation, vector…
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Taxonomy
TopicsCosmology and Gravitation Theories · advanced mathematical theories · Black Holes and Theoretical Physics
