FRW Cosmology with a Varying Cubic Deceleration Parameter

Q2 Physics and Astronomy Letters in High Energy Physics Pub Date : 2022-08-20 DOI:10.31526/lhep.2023.330
Leishingam Kumrah, S. S. Singh, L. Devi, Md Khurshid Alam
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引用次数: 0

Abstract

In this work a new law of varying deceleration parameter of third degree have been proposed. The solutions of the modified field equations have been derived under the newly proposed law of the deceleration parameter. Model exhibits the Big-bang singularity at cosmic time ($t=0$) and shows Big Rip at ($t=n$) then it re-enter the phase of initial singularity at $t=2n$ and ends its cyclic behavior at $t=3n$. The evolution of the physical and dynamical parameters of the Universe have been studied and the graphical representation has also been shown. Further $Om(z)$ diagnostic parameter and the energy conditions have also been studied together with their graphical representations.
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变三次减速参数的FRW宇宙学
本文提出了一种新的三次减速参数变律。在新提出的减速参数规律下,导出了修正后的场方程的解。模型在宇宙时间($t=0$)处显示大爆炸奇点,在($t=n$)处显示大撕裂,然后在$t=2n$处重新进入初始奇点阶段,并在$t=3n$处结束循环行为。研究了宇宙的物理和动力学参数的演变,并给出了图形表示。进一步研究了$Om(z)$诊断参数和能量条件,并给出了它们的图形表示。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Letters in High Energy Physics
Letters in High Energy Physics Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
1.20
自引率
0.00%
发文量
4
审稿时长
12 weeks
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