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Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method
Wu, Puxun ; Yu, Hongwei
2010-05-06 ; 2010-05-06
关键词dark energy theory supernova type Ia HUBBLE-SPACE-TELESCOPE EXPANSION HISTORY CONSTRAINTS UNIVERSE REDSHIFT DENSITY RECONSTRUCTION QUINTESSENCE DISCOVERIES STATEFINDER Astronomy & Astrophysics Physics, Particles & Fields
中文摘要With a model independent method the expansion history H(z), the deceleration parameter q(z) of the universe and the equation of state w(z) for the dark energy are reconstructed directly from the 192 Sne Ia (type Ia supernovae) data points which are contained in the new ESSENCE (Equation of State: Supernovae Trace Cosmic Expansion) Sne Ia data and the high redshift Sne Ia data. We find that the evolving properties of q(z) and w(z) reconstructed from the 192 Sne Ia data seem to be weaker than those obtained from the Gold set, but stronger than those from the SNLS (Supernova Legacy Survey) set. With a combination of the 192 Sne Ia and BAO (Baryonic Acoustic Oscillation) data, a tight constraint on Omega(m0) is obtained. At the 1 sigma confidence level Omega(m0) = 0.278(-0.023)(+ 0.024), which is highly consistent with the values from the Gold + BAO and SNLS + BAO data.
语种英语 ; 英语
出版者IOP PUBLISHING LTD ; BRISTOL ; DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND
内容类型期刊论文
源URL[http://hdl.handle.net/123456789/14745]  
专题清华大学
推荐引用方式
GB/T 7714
Wu, Puxun,Yu, Hongwei. Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method[J],2010, 2010.
APA Wu, Puxun,&Yu, Hongwei.(2010).Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method..
MLA Wu, Puxun,et al."Probing the cosmic acceleration history and the properties of dark energy from the ESSENCE supernova data with a model independent method".(2010).
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