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Freddy P. Zen Arianto Bobby E. Gunara Triyanta A. Purwanto 《The European Physical Journal C - Particles and Fields》2009,63(3):477-490
The cosmological evolution of an interacting scalar-field model in which the scalar field interacts with dark matter, radiation,
and baryons via Lorentz violation is investigated. We propose a model of interaction through the effective coupling,
[`(b)]\bar{\beta}
. Using dynamical system analysis, we study the linear dynamics of an interacting model and show that the dynamics of critical
points are completely controlled by two parameters. Some results can be mentioned as follows. Firstly, the sequence of radiation,
the dark matter, and the scalar-field dark energy exist and baryons are subdominant. Secondly, the model also allows for the
possibility of having a universe in the phantom phase with constant potential. Thirdly, the effective gravitational constant
varies with respect to time through
[`(b)]\bar{\beta}
. In particular, we consider the simple case where
[`(b)]\bar{\beta}
has a quadratic form and has a good agreement with the modified ΛCDM and quintessence models. Finally, we also calculate the first post-Newtonian parameters for our model. 相似文献
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