期刊
CLASSICAL AND QUANTUM GRAVITY
卷 30, 期 6, 页码 -出版社
IOP Publishing Ltd
DOI: 10.1088/0264-9381/30/6/065018
关键词
-
类别
资金
- Department of Physics, University of Kurdistan, Sanandaj, Iran [27/13726]
We study the correspondence between the interacting viscous ghost dark energy model with the tachyon, K-essence and dilaton scalar field models in the framework of Einstein gravity. We consider a spatially non-flat FRW universe filled with interacting viscous ghost dark energy and dark matter. We reconstruct both the dynamics and potential of these scalar field models according to the evolutionary behavior of the interacting viscous ghost dark energy model, which can describe the accelerated expansion of the universe. Our numerical results show that the interaction and viscosity have opposite effects on the evolutionary properties of the ghost scalar field models.
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