中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Relic abundance of asymmetric Dark Matter in quintessence

文献类型:期刊论文

作者Iminniyaz, Hoernisa1; Chen, Xuelei2,3
刊名ASTROPARTICLE PHYSICS
出版日期2014-02-01
卷号54页码:125-131
关键词Dark Matter Asymmetry Relic abundance Quintessence Cosmology
英文摘要We investigate the relic abundance of asymmetric Dark Matter particles in quintessence model with a kination phase. The analytic calculation of the asymmetric Dark Matter in the standard cosmological scenario is extended to the nonstandard cosmological scenario where we specifically discuss the quintessence model with a kination phase. We found that the enhancement of Hubble rate changes the relic density of particles and anti-particles. We use the present day Dark Matter abundance to constrain the Hubble rate in quintessence model with a kination phase for asymmetric Dark Matter. (C) 2013 Elsevier B.V. All rights reserved.
收录类别SCI
语种英语
WOS记录号WOS:000332434700016
源URL[http://ir.bao.ac.cn/handle/114a11/6614]  
专题国家天文台_星系宇宙学研究部
作者单位1.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China
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Iminniyaz, Hoernisa,Chen, Xuelei. Relic abundance of asymmetric Dark Matter in quintessence[J]. ASTROPARTICLE PHYSICS,2014,54:125-131.
APA Iminniyaz, Hoernisa,&Chen, Xuelei.(2014).Relic abundance of asymmetric Dark Matter in quintessence.ASTROPARTICLE PHYSICS,54,125-131.
MLA Iminniyaz, Hoernisa,et al."Relic abundance of asymmetric Dark Matter in quintessence".ASTROPARTICLE PHYSICS 54(2014):125-131.

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来源:国家天文台

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