SO(1,1) dark energy model and the universe transition
文献类型:期刊论文
作者 | Wei, YH; Tian, Y; Wei, YH , Bohai Univ, Dept Phys, Liaoning 121000, Peoples R China. |
刊名 | CLASSICAL AND QUANTUM GRAVITY
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出版日期 | 2004 |
卷号 | 21期号:23页码:5347-5353 |
关键词 | Hubble-space-telescope High-redshift Supernovae Equation-of-state Phantom Energy Cosmology Quantum Matter Quintessence Constraints Field |
ISSN号 | 0264-9381 |
英文摘要 | We suggest the SO(1, 1) scalar field model of dark energy. In this model, the Lagrangian may be decomposed as that of the real quintessence model and the negative coupling energy term of Phi to a. The existence of the coupling term L-c leads to a wider range of w(Phi) and overcomes the problem of negative kinetic energy in the phantom universe model. We propose a power-law expansion kinetics model of the universe with time-dependent power, which can describe the universe transition from ordinary acceleration to super acceleration. We also give a simple discussion of the Big Rip, singularity, and point out the possibility that the universe driven by a phantom avoids it. |
学科主题 | Physics |
URL标识 | 查看原文 |
WOS记录号 | WOS:000225806700004 |
公开日期 | 2012-08-30 |
源URL | [http://ir.itp.ac.cn/handle/311006/13928] ![]() |
专题 | 理论物理研究所_理论物理所1978-2010年知识产出 |
通讯作者 | Wei, YH , Bohai Univ, Dept Phys, Liaoning 121000, Peoples R China. |
推荐引用方式 GB/T 7714 | Wei, YH,Tian, Y,Wei, YH , Bohai Univ, Dept Phys, Liaoning 121000, Peoples R China.. SO(1,1) dark energy model and the universe transition[J]. CLASSICAL AND QUANTUM GRAVITY,2004,21(23):5347-5353. |
APA | Wei, YH,Tian, Y,&Wei, YH , Bohai Univ, Dept Phys, Liaoning 121000, Peoples R China..(2004).SO(1,1) dark energy model and the universe transition.CLASSICAL AND QUANTUM GRAVITY,21(23),5347-5353. |
MLA | Wei, YH,et al."SO(1,1) dark energy model and the universe transition".CLASSICAL AND QUANTUM GRAVITY 21.23(2004):5347-5353. |
入库方式: OAI收割
来源:理论物理研究所
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