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 | 2024年
关键词：
Modified field equations; Holographic dark energy; Big rip model; PROBE WMAP OBSERVATIONS; UNIVERSE; ANISOTROPY; DECELERATION; CONSTRAINTS; CONSTANT; TORSION; PARAMETER; REDSHIFT; MAPS;
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.
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页数：12
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