Incorporating holographic dark energy in the big rip cosmological model with f(R, Σ T) - Gravity

被引：0

作者：

Bakry, M. A. ^{[1
,3
]}

Alkaoud, A. ^{[2
]}

机构：

[1] Ain Shams Univ, Fac Educ, Dept Math, Cairo 11864, Egypt

[2] Imam Mohammad Ibn Saud Islamic Univ IMSIU, Coll Sci, Dept Phys, Riyadh, Saudi Arabia

[3] Cairo Univ, Egyptian Relat Grp ERG, Giza 12613, Egypt

来源：

INDIAN JOURNAL OF PHYSICS | 2025年 / 99卷 / 07期

关键词：

Modified field equations; Holographic dark energy; Big rip model; PROBE WMAP OBSERVATIONS; UNIVERSE; ANISOTROPY; DECELERATION; CONSTRAINTS; CONSTANT; TORSION; PARAMETER; REDSHIFT; FIELD;

D O I：

10.1007/s12648-024-03481-0

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The primary objective of this research is to investigate the behavior of the universe model in the presence of matter and holographic dark energy in f(R, Sigma, T) - Gravity. The study utilizes f(R, Sigma, T) strong gravity with torsion field equations to derive exact solutions for a Big Rip universe. The research also explores the physical and geometrical aspects of the universe, including the results obtained by Bakry and Shafeek (Indian J Phys 1, 2021). Additionally, the paper introduces a novel cosmological model for Dark energy based on an anti-gravity field scenario. This model may offer a viable solution to the dark energy problem due to the anti-gravity field's existence.

引用

页码：2695 / 2706

页数：12

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