Domain Walls and Quark Matter Cosmological Models in f(R, T) = R + αR2 + λT Gravity

被引:0
|
作者
Bishi, Binaya K. [1 ,2 ]
Beesham, Aroonkumar [1 ,3 ]
Mahanta, K. L. [4 ]
机构
[1] Univ Zululand, Dept Math Sci, Private Bag X1001, ZA-3886 Kwa Dlangezwa, South Africa
[2] Lovely Profess Univ, Dept Math, Jalandhar 144401, Punjab, India
[3] Mangosuthu Univ Technol, Fac Nat Sci, Jacobs, South Africa
[4] CV Raman Global Univ, Dept Math, Bhubaneswar 752054, Orissa, India
来源
IRANIAN JOURNAL OF SCIENCE AND TECHNOLOGY TRANSACTION A-SCIENCE | 2021年 / 45卷 / 05期
基金
新加坡国家研究基金会; 芬兰科学院;
关键词
FLRW spacetime; f; (R; T) = R + alpha R-2 + lambda T; Domain wall; Quark matter; SYMMETRIC SPACE-TIME; STRING CLOUD; BRANS-DICKE; F R; GRAVITY; CONSTANT; DYNAMICS; FIELD;
D O I
10.1007/s40995-021-01113-4
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The manuscript deals with the study of the FLRW universe together with domain walls and quark matter in f(R, T) gravity where R is the Ricci scalar and T is the trace of the energy momentum tensor. We choose f (R, T) = R + alpha R-2 + lambda T. Exact solutions are obtained under the assumptions: (1) a constant and variable deceleration parameter of the form q = m - 1 and q = - alpha(3)/t(2) + beta - 1, alpha(3) not equal 0 and (2) an equation of the state of the form p(m) = (gamma - 1)rho(m) and p(m) = 1/3 (rho(m) - 4B(c)). The physical quantities involved in the cosmological models are obtained and analysed graphically. The solutions obtained here are most general which reduce to the solutions in general relativity, f(R, T) theory and higher derivative theory with suitable choices of the parameters.
引用
收藏
页码:1825 / 1835
页数:11
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