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Minimally interacting holographic dark energy model in a five dimensional spherically symmetric space-time in Saez–Ballester theory of gravitation
- 作者:P. Raju ; K. Sobhanbabu ; D. R. K. Reddy
- 关键词:Scalar–tensor theory ; Holographic dark energy ; Spherically symmetric space ; time
- 刊名:Astrophysics and Space Science
- 出版年:2016
- 出版时间:February 2016
- 年:2016
- 卷:361
- 期:2
- 全文大小:656 KB
- 参考文献:Adhav, K.S., et al.: Astrophys. Space Sci. 353, 249 (2014) CrossRef ADS
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- 作者单位:P. Raju (1)
K. Sobhanbabu (1) D. R. K. Reddy (2)
1. Dept. of Mathematics, J.N.T.U. College of Engineering, Vizianagaram, India 2. Dept. of Applied Maths, Andhra University, Visakhapatnam, India
- 刊物类别:Physics and Astronomy
- 刊物主题:Physics
Astronomy
- 出版者:Springer Netherlands
- ISSN:1572-946X
文摘
Five-dimensional spherically symmetric space-time filled with two minimally interacting fields, matter and holographic dark energy components, is investigated in a scalar tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). An explicit solution of the field equations is obtained. Some physical and kinematic properties of the model are also studied.
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