The universe content is considered as a non-perfect fluid with bulk viscosity and can be described by ageneral equation of state (endowed some deviation from the conventionally assumed cosmic perfect fluid model).Anex...The universe content is considered as a non-perfect fluid with bulk viscosity and can be described by ageneral equation of state (endowed some deviation from the conventionally assumed cosmic perfect fluid model).Anexplicitly bulk viscosity dark energy model is proposed to confront consistently with the current observational data setsby statistical analysis and is shown consistent with (not deviated away much from) the concordant Λ Cold Dark Matter(CDM) model by comparing the decelerating parameter.Also we compare our relatively simple viscosity dark energymodel with a more complicated one by contrast with the concordant ΛCDM model and find our model improves for theviscosity dark energy model building.Finally we discuss the perspectives of dark energy probes for the coming yearswith observations.展开更多
基金Supported by the National Natural Science Foundation of China under Grant No.10675062the Project of Knowledge Innovation Program (PKIP) of Chinese Academy of Sciences under Grant No.KJCX2.YW.W10
文摘The universe content is considered as a non-perfect fluid with bulk viscosity and can be described by ageneral equation of state (endowed some deviation from the conventionally assumed cosmic perfect fluid model).Anexplicitly bulk viscosity dark energy model is proposed to confront consistently with the current observational data setsby statistical analysis and is shown consistent with (not deviated away much from) the concordant Λ Cold Dark Matter(CDM) model by comparing the decelerating parameter.Also we compare our relatively simple viscosity dark energymodel with a more complicated one by contrast with the concordant ΛCDM model and find our model improves for theviscosity dark energy model building.Finally we discuss the perspectives of dark energy probes for the coming yearswith observations.
