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耦合为αHρ_φ+βHρ_m的k-essence暗能量模型相空间分析
Phase-space Analysis of K-essence Dark Energy Model with the Coupling αHρ_φ+βHρ_m
【摘要】 结合最近十年宇宙学中关于k-essence暗能量模型的多篇论文观点,本文适当选取F(X)=-X(1/2)+X构造拉格朗日量,同时尝试改进暗物质与暗能量的非零相互耦合0≠Q=αHρ_φ+βHρ_m,使其既与暗物质相关又与暗能量相关。进而推导出更普遍的相空间演化自洽微分方程组。最后在满足宇宙加速膨胀这一观测结果的前提下,设定参数α,β,λ的数值,并作出相空间演化图,标记出相空间演化的稳定点,定性地分析出宇宙演化晚期的几种可能结果。
【Abstract】 With the views from the papers for the last ten years about k-essence dark energy models,this paper chooses F( X) =-X(1/2)+ X to make the Lagrangian,and tries the coupling term 0≠Q = αHρ_φ+ βHρ_m between dark matter and dark energy,and it derives the general self-contain evolution differential equations. Finally,under the observation fact of accelerating expansion,three parameters α,β,λare set to draw the phase-space evolution pictures,and the stable points,including the critical points,are marked on the pictures to demonstrate the possible result of the late cosmology dynamical evolution.
- 【文献出处】 北华航天工业学院学报 ,Journal of North China Institute of Aerospace Engineering , 编辑部邮箱 ,2016年05期
- 【分类号】P159
- 【被引频次】1
- 【下载频次】15