LRS Bianchi type-V cosmological model in f (Q, T) theory of gravity with cold matter and holographic dark energy

被引：0

作者：

Solanke, Y. S. ^{[1
]}

Mhaske, S. ^{[1
]}

Dagwal, V. J. ^{[2
]}

Pawar, D. D. ^{[3
]}

机构：

[1] Mungasaji Maharaj Mahavidyalaya, Dept Math, Darwha 445202, Yavatmal, India

[2] Govt Coll Engn, Dept Math, Nagpur 441108, India

[3] Swami Ramanand Teerth Marathwada Univ, Sch Math Sci, Nanded 431606, India

来源：

ASTRONOMY AND COMPUTING | 2025年 / 52卷

关键词：

f(Q; T) theory of gravity; Cold dark matter; Holographic dark energy; LUMINOUS RED GALAXIES; T GRAVITY; ACCELERATING UNIVERSE; CONSTANT; CONSTRAINTS; TRANSITION; INFLATION;

D O I：

10.1016/j.ascom.2025.100961

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In the present work Bianchi type V cosmological model with cold dark matter and holographic dark energy with f(Q,T) theory of gravity is investigated, with f(Q,T)=alpha Q+beta T, where alpha and beta are constants. To find the solution of the field equation we have used the anisotropic relation. Various physical and geometrical properties of the model have been investigated graphically.

引用

页数：11

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