https://doi.org/10.1140/epjc/s10052-009-1104-1
Regular Article - Theoretical Physics
Cosmological evolution of interacting dark energy in Lorentz violation
1
Theoretical Physics Lab., THEPI Devision, Jl. Ganesha 10, Bandung, 40132, Indonesia
2
Indonesia Center for Theoretical and Mathematical Physics (ICTMP), Faculty of Mathematics and Natural Sciences, Institut Teknologi Bandung, Jl. Ganesha 10, Bandung, 40132, Indonesia
3
Department of Physics, Udayana University, Jl. Kampus Bukit, Jimbaran, Kuta-Bali, 80361, Indonesia
4
Department of Physics, Institut Teknologi Sepuluh November, Jl. Kampus Sukolilo, Surabaya, 60111, Indonesia
* e-mail: arianto@upi.edu
Received:
8
April
2009
Revised:
15
June
2009
Published online:
31
July
2009
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,
. 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
. In particular, we consider the simple case where
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.
Key words: 98.80.Cq / 98.80.-k
© Springer-Verlag , 2009