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耦合为αHρ_φ+βHρ_m的k-essence暗能量模型相空间分析 被引量:1

Phase-space Analysis of K-essence Dark Energy Model with the Coupling αHρ_φ+βHρ_m
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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。 With the views from the papers for the last ten years about k-essence dark energy models, this paper chooses F(X) = - √X + X to make the Lagrangian, and tries the coupling term 0≠Q=αHρφ+βHρm 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,λ are 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.
出处 《北华航天工业学院学报》 CAS 2016年第5期23-26,共4页 Journal of North China Institute of Aerospace Engineering
基金 北华航天工业学院科研项目(KY-2012-12 BKY-2014-10)
关键词 暗能量耦合 K-ESSENCE 相空间 coupling of dark energy, k-essence, phase - space
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