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

被引：14
|
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
收藏
页码：339 / 348
页数：10
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