Non linear equation of state and effective phantom divide in brane models

Abstract

Here, DGP model of brane-gravity is analyzed and compared with the standard general relativity and Randall-Sundrum cases using non-linear equation of state. Phantom fluid is known to violate the weak energy condition. In this paper, it is found that this characteristic of phantom energy is affected drastically by the negative brane-tension $\lambda$ of the RS-II model. It is found that in DGP model strong energy condition(SEC) is always violated and the universe accelerates only where as in RS-II model even SEC is not violated for $1<\rho /\lambda <2$ and the universe decelerates.

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Cited by in corpus (2)

• Electron mass variation from dark sector interactions and compatibility with cosmological observations
• Late time accelerated scaling attractors in DGP (Dvali-Gabadadze-Porrati) braneworld