中国科学院机构知识库网格
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Dark energy and fate of the Universe

文献类型:期刊论文

作者Huang, QG; Li, M
刊名SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
出版日期2012
卷号55期号:7页码:1330-1334
关键词SUPERNOVA LEGACY SURVEY HUBBLE-SPACE-TELESCOPE DYNAMICS PARAMETRIZATIONS CONSTRAINTS
ISSN号1674-7348
通讯作者Zhang, X (reprint author), Northeastern Univ, Dept Phys, Coll Sci, Shenyang 110004, Peoples R China.
英文摘要We explore the ultimate fate of the Universe by using a divergence-free parametrization for dark energy w(z)=w (0)+w (a) [ln(2 + z) / (1 + z) - ln 2]. Unlike the Chevallier-Polarski-Linder parametrization, this parametrization has well behaved, bounded behavior for both high redshifts and negative redshifts, and thus can genuinely cover many theoretical dark energy models. After constraining the parameter space of this parametrization by using the current cosmological observations, we find that, at the 95.4% confidence level, our Universe can still exist at least 16.7 Gyr before it ends in a big rip. Moreover, for the phantom energy dominated Universe, we find that a gravitationally bound system will be destroyed at a time , where P is the period of a circular orbit around this system, before the big rip.
学科主题Physics
收录类别SCI
资助信息Project of Knowledge Innovation Program of Chinese Academy of Sciences; National Natural Science Foundation of China [11105053, 10705041, 10975032, 11175042, 10535060, 10975172, 10821504]; National Ministry of Education of China [NCET-09-0276, N100505001]; National Basic Research Program of China [2007CB815401]
原文出处http://dx.doi.org/10.1007/s11433-012-4748-z
语种英语
WOS记录号WOS:000305419500029
公开日期2014-04-25
源URL[http://ir.itp.ac.cn/handle/311006/15074]  
专题理论物理研究所_理论物理所1978-2010年知识产出
推荐引用方式
GB/T 7714
Huang, QG,Li, M. Dark energy and fate of the Universe[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2012,55(7):1330-1334.
APA Huang, QG,&Li, M.(2012).Dark energy and fate of the Universe.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,55(7),1330-1334.
MLA Huang, QG,et al."Dark energy and fate of the Universe".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 55.7(2012):1330-1334.

入库方式: OAI收割

来源:理论物理研究所

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