Future Destiny of Quintessential Universe and Constraint on Model from Deceleration Parameter  

作　　者：ZHANG De-Hai 

机构地区：[1]Department of Physics, the Graduate School of the Chinese Academy of Sciences, P.O. Box 3908, Beijing 100039, China

出　　处：《Communications in Theoretical Physics》2002年第8期253-255,共3页理论物理通讯（英文版）

基　　金：国家自然科学基金，NKBRSF G

摘　　要：The evolution of the quintessence in various stages of the universe, i.e., the radiation-, matter-, andquintessence-dominated stages, is closely related with the tracking behavior and the deceleration parameter of theuniverse. We gave the explicit relation between the equation-of-state of the quintessence in the epoch of the matter-quintessence equality and the inverse power index of the quintessence potential, obtained the constraint on this potentialparameter comingfrom the present deceleration parameter, i.e., a low inverse power index.We point out that the lowinverse power-law potential with a single term cannot work for the tracking solution. In order to have both of the trackerand the suitable deceleration parameter it is necessary to introduce at least two terms in the quintessence potential. Wegive the future evolution of the quintessential universe.

关 键 词：quintessence  equation of state  INVERSE low index  tracker  DECELERATION parameter 

分 类 号：O4[理学—物理]