Holographic dark energy with linearly varying deceleration parameter and escaping big rip singularity of the Bianchi type-V universe

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• 作者：Sanjay Sarkar (1)
  
• 关键词：Bianchi type ; V line element ; Linearly varying deceleration parameter ; Holographic dark energy ; Black hole ; Wormhole ; Big rip and big trip singularity
• 刊名：Astrophysics and Space Science
• 出版年：2014
• 出版时间：August 2014
• 年：2014
• 卷：352
• 期：2
• 页码：859-866
• 全文大小：394 KB
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• 作者单位：Sanjay Sarkar (1)
  
  1. Department of Mathematics, Kaziranga English Academy, Garchuk, Guwahati, 35, India
  
• ISSN：1572-946X

文摘

The present work deals with the accretion of two minimally interacting fluids: dark matter and a hypothetical isotropic fluid as the holographic dark energy components onto black hole and wormhole in a spatially homogeneous and anisotropic Bianchi type-V universe. To obtain an exact solution of the Einstein’s field equations, we use the assumption of linearly varying deceleration parameter. Solution describes effectively the actual acceleration and indicates a big rip type future singularity of the universe. We have studied the evolution of the mass of black hole and the wormhole embedded in this anisotropic universe in order to reproduce a stable universe protected against future-time singularity. It is observed that the accretion of these dark components leads to a gradual decrease and increase of black hole and wormhole mass respectively. Finally, we have found that contrary to our previous case (Sarkar in Astrophys. Space. Sci. 341:651, 2014a), the big rip singularity of the universe with a divergent Hubble parameter of this dark energy model may be avoided by a big trip.