Bianchi Type-III Magnetized Wet Dark Fluid Cosmological Model in General Relativity

被引：15

作者：

Adhav, K. S. ^{[1
]}

Dawande, M. V. ^{[1
]}

Thakare, R. S. ^{[1
]}

Raut, R. B. ^{[1
]}

机构：

[1] SGB Amravati Univ, Dept Math, Amravati 444602, India

来源：

INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2011年 / 50卷 / 02期

关键词：

Bianchi type-III space-time; Magnetic field; Wet dark fluid; Dark energy; ENERGY-MODEL; UNIVERSE; FIELD; DYNAMICS; QUINTOM; CONSTANT; PHANTOM; LAW; AGE;

D O I：

10.1007/s10773-010-0530-z

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Bianchi type-III cosmological model of universe filled with dark energy from a wet dark fluid (WDF) in presence and absence of magnetic field is investigated in general theory of relativity. We assume that F (12) is the only non-vanishing component of F (ij) . We obtain exact solutions to the field equations using the condition that expansion is proportional to the shear scalar i.e. (B=C (n) ). The physical behavior of the model is discussed with and without magnetic field. We conclude that universe model do not approach isotropy through the evolution of the universe.

引用

页码：339 / 348

页数：10

共 89 条

[1] Cosmological dynamics of the tachyon with an inverse power-law potential [J].