Bianchi Type-II Dark Energy Model in Scale Covariant Theory of Gravitation

被引：14
|
作者：
Singh, J. K. [1 ]
Sharma, N. K. [1 ]
机构：
[1] Univ Delhi, Netaji Subhash Inst Technol, Sch Appl Sci, Sect 3, New Delhi 110078, India
来源：
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS | 2014年 / 53卷 / 02期
关键词：
Bianchi type-II metric; Dark energy; Scale covariant theory;
D O I：
10.1007/s10773-013-1830-x
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Spatially Homogeneous and anisotropic Bianchi type-II space time with variable equation of state (EoS) parameter and constant deceleration parameter has been investigated in scale covariant theory of gravitation formulated by Canuto et al. (Phys. Rev. Lett. 39:429, 1977). With the help of special law of variation for Hubble's parameter proposed by Bermann (Nuovo Cimento 74B:182, 1983) a dark energy cosmological model is obtained in this theory. We use the power law relation between scalar field I center dot and scale factor R to find the solutions. Some physical and kinematical properties of the model are also discussed.
引用
收藏
页码：461 / 468
页数：8
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