作者: K. Karami , M. Jamil , M. Roos , S. Ghaffari , A. Abdolmaleki
DOI: 10.1007/S10509-012-1020-Y
关键词: Physics 、 Deceleration parameter 、 Classical mechanics 、 Dark matter 、 Mathematical physics 、 Dark energy 、 Lambda-CDM model 、 Omega 、 Dark fluid 、 Scalar field dark matter 、 Thermodynamics of the universe
摘要: We study the entropy-corrected version of new agegraphic dark energy (NADE) model and matter in a spatially non-flat Universe framework Ho\v{r}ava-Lifshitz cosmology. For two cases containing noninteracting interacting NADE (ECNADE) models, we derive exact differential equation that determines evolution ECNADE density parameter. Also deceleration parameter is obtained. Furthermore, using parametrization state as $\omega_{\Lambda}(z)=\omega_0+\omega_1 z$, obtain both $\omega_0$ $\omega_1$. find presence interaction, this can cross phantom divide line which compatible with observation.