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.
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页码：339 / 348
页数：10
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