A cosmological model with time dependent ?, G and viscous fluid in general relativity

被引：2
作者：
Tiwari, Rishi Kumar [1 ]
Alfedeel, Alnadhief H. A. [2 ]
Sofuoglu, Deger [3 ]
Abebe, Amare [4 ,5 ]
Hassan, Eltegani I. [2 ]
Shukla, B. K. [1 ]
机构：
[1] Govt Model Sci Coll Rewa, Dept Math, Rewa, Madhya Pradesh, India
[2] Imam Mohammad Ibn Saud Islamic Univ IMSIU, Dept Math & Stat, Riyadh, Saudi Arabia
[3] Istanbul Univ, Dept Phys, Istanbul, Turkey
[4] North West Univ, Ctr Space Res, Mahikeng, South Africa
[5] Natl Inst Theoret & Computat Sci NITheCS, Cape Town, South Africa
来源：
FRONTIERS IN ASTRONOMY AND SPACE SCIENCES | 2022年 / 9卷
关键词：
time dependent G and boolean AND; bianchi metric; viscous fluid; anisotropy; cosmological parameter; F(R) THEORIES; LAMBDA; SUPERNOVAE; UNIVERSE; OMEGA;
D O I：
10.3389/fspas.2022.965652
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
neutrinos disengage from of galaxies formation our cosmos (Hu et al., been many attempts to models involving viscous recently studied various field equations for model physical parameters or imposing any extra constraints, as others do. Instead, we will recast the geovering equations for the Bianchi type - V model as adimension less, non-linear, first order, coupling differential equation for cosmological observations h(z), SZm(z), SZA, SZx, and SZ,, then integrate them in parallel to
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页数：8
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