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A Parametric Dynamic Model of Dark Energy
作者姓名:邓雪梅  吴亚波  赵国明
作者单位:Department of Physics, Liaoning Normal University, Dalian 116029
基金项目:Supported by the National Natural Science Foundation of China under Grant No 10475036, the Natural Science Foundation of Liaoning Province under Grant No 20032102, and the Scientific Research Foundation of the Higher Education Institute of Liaoning Province under Grant No 05L215.
摘    要:The double complex symmetric gravitational theory is extended to the parametric symmetric gravitational theory by introducing a parameter β. Hence parametric Friedmann-Robertson-Walker equations are obtained and some characters of dark energy in corresponding spaces are discussed by taking different values of β. In our method some previous results can be included as the special case of our results. It is worth noting that some characters of dark energy can be more intuitively described in our model. By analysis, we can predict that the fate of universe would be a Big Rip in the future, and also find that the state parameters for the two different constraint conditions wФ are consistent with the present cosmological observations.

关 键 词:参数动力学模型  暗能量  重力均衡理论  Friedmann-Robertson-Walker方程  理论物理
收稿时间:2006-01-17
修稿时间:2006-01-17

A Parametric Dynamic Model of Dark Energy
DENG Xue-Mei,WU Ya-Bo,ZHAO Guo-Ming.A Parametric Dynamic Model of Dark Energy[J].Chinese Physics Letters,2006,23(6):1655-1658.
Authors:DENG Xue-Mei  WU Ya-Bo  ZHAO Guo-Ming
Institution:Department of Physics, Liaoning Normal University, Dalian 116029
Abstract:
Keywords:98  80  -k  04  20  -q
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