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• W2016839175 abstract "We study cosmological application of the holographic energy density in the Brans-Dicke theory. Considering the holographic energy density as a dynamical cosmological constant, it is more natural to study it in the Brans-Dicke theory than in general relativity. Solving the Friedmann and Brans-Dicke field equations numerically, we clarify the role of Brans-Dicke field during evolution of the universe. When the Hubble horizon is taken as the IR cutoff, the equation of state ($w_{Lmd}$) for the holographic energy density is determined to be 5/3 when the Brans-Dicke parameter $omg$ goes infinity. This means that the Brans-Dicke field plays a crucial role in determining the equation of state. For the particle horizon IR cutoff, the Brans-Dicke scalar mediates a transition from $w_{Lmd} = -1/3$ (past) to $w_{Lmd} = 1/3$ (future). If a dust matter is present, it determines future equation of state. In the case of future event horizon cutoff, the role of the Brans-Dicke scalar and dust matter are turned out to be trivial, whereas the holographic energy density plays an important role as a dark energy candidate with $w_{Lmd} =-1$." @default.
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• W2016839175 date "2005-11-01" @default.
• W2016839175 modified "2023-10-14" @default.
• W2016839175 title "Role of the Brans–Dicke scalar in the holographic description of dark energy" @default.
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• W2016839175 doi "https://doi.org/10.1016/j.physletb.2005.09.040" @default.
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