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- W2950243085 abstract "In this paper, we study the effects which are produced by the interaction between a brane Universe and the bulk in which the Universe is embedded. Taking into account the effects produced by the interaction between a brane Universe and the bulk, we derived the Equation of State (EoS) parameter $omega_D$ for three different models of Dark Energy (DE), emph{i.e.} the Holographic DE (HDE) model with infrared (IR) cut-off given by the Granda-Oliveros cut-off, the Modified Holographic Ricci DE (MHRDE) model and a DE model which is function of the Hubble parameter $H$ squared and to higher derivatives of $H$. Moreover, we have considered two different cases of scale factor (namely, the power law and the emergent ones). A nontrivial contribution of the DE is observed to be different from the standard matter fields confined to the brane. Such contribution has a monotonically decreasing behavior upon the evolution of the Universe for the emergent scenario of the scale factor, while monotonically increasing for the power-law form of the scale factor $a(t)$." @default.
- W2950243085 created "2019-06-27" @default.
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- W2950243085 date "2015-10-22" @default.
- W2950243085 modified "2023-09-27" @default.
- W2950243085 title "Consequences of three modified forms of holographic dark energy models in bulk-brane interaction" @default.
- W2950243085 hasPublicationYear "2015" @default.
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