摘要
We investigate the interacting new holographic dark energy （HDE） with viscosity. Specifically, we not only study the dynamical evolutions of the new HDE with viscosity and the influences of viscosity as well as the coupling constant on the equation of state for the new HDE, but also establish the correspondence between the new HDE with viscosity and variable generalized Chaplygin gas （VGCG） models in the fiat Friedmann-Robertson-Walker universe. Furthermore, we also reconstruct the potential and the dynamics of VGCG as the scalar field. By analysis we show that for the new holographic Chaplygin gas model, if the related parameters to the potential satisfy some constraints, the accelerated expansion can be achieved. These research results can reduce to the ones without viscosity.
We investigate the interacting new holographic dark energy （HDE） with viscosity. Specifically, we not only study the dynamical evolutions of the new HDE with viscosity and the influences of viscosity as well as the coupling constant on the equation of state for the new HDE, but also establish the correspondence between the new HDE with viscosity and variable generalized Chaplygin gas （VGCG） models in the fiat Friedmann-Robertson-Walker universe. Furthermore, we also reconstruct the potential and the dynamics of VGCG as the scalar field. By analysis we show that for the new holographic Chaplygin gas model, if the related parameters to the potential satisfy some constraints, the accelerated expansion can be achieved. These research results can reduce to the ones without viscosity.
基金
Supported by the National Natural Science Foundation of China under Grant Nos 11175077 and 11205078, the PhD Programs Foundation of Ministry of Education of China under Grant No 20122136110002, the Natural Science Foundation of Liaoning Province under Grant No L2011189, and the Project of Key Discipline of Theoretical Physic of Department of Education in Liaoning Province under Grant Nos 905035 and 905061.
