期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 346, 期 1, 页码 273-278出版社
SPRINGER
DOI: 10.1007/s10509-013-1428-z
关键词
Reconstruction; Holographic dark energy; Modied f (R); Horava-Lifshitz gravity
资金
- Higher Education Commission, Islamabad, Pakistan
- Department of Science and Technology, Govt. of India [SR/FTP/PS-167/2011]
This paper is devoted to the study of holographic reconstruction of the modified f(R) Horava-Lifshitz gravity in the flat universe. For this purpose, we assume a scale factor in the form of exact power-law solution. A reconstructed model is obtained which may provide reasonable qualitative description of some cosmological era satisfying the sufficient condition for a realistic model. We represent the graphical description of this model exhibiting increasing behavior. We also discuss the evolution of the accelerated expansion of the universe through equation of state parameter (EoS) for the reconstructed model. Its graphical representation depicts about a quintessence dominated era in near future. The stability of the model is observed initially, however it becomes unstable after a small interval of time.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据