中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Impact of a Locally Measured H-0 on the Interpretation of Cosmic-chronometer Data

文献类型:期刊论文

作者Wei, Jun-Jie; Melia, Fulvio; Wu, Xue-Feng
刊名ASTROPHYSICAL JOURNAL
出版日期2017
卷号835期号:2页码:270-
英文摘要Many measurements in cosmology depend on the use of integrated distances or time, but. galaxies evolving passively on a timescale much longer than their age difference allow us to determine the expansion rate H(z) solely as a function of the redshift-time derivative dz/dt. These model-independent "cosmic chronometers" can therefore be powerful discriminators for testing different cosmologies. In previous applications, the available sources strongly disfavored models (such as Lambda CDM) predicting a variable acceleration, preferring instead a steady expansion rate over the redshift range 0 less than or similar to z less than or similar to 2. A more recent catalog of 30 objects appears to suggest non-steady expansion. In this paper, we show that such a result is entirely due to the inclusion of a high, locally inferred value of the Hubble constant H-0 as an additional datum in a set of otherwise pure cosmic-chronometer measurements. This H-0, however, is not the same as the background Hubble constant if the local expansion rate is influenced by a Hubble Bubble. Used on their own, the cosmic chronometers completely reverse this conclusion, favoring instead a constant expansion rate out to z similar to 2.
语种英语
源URL[http://libir.pmo.ac.cn/handle/332002/17422]  
专题中国科学院紫金山天文台
推荐引用方式
GB/T 7714
Wei, Jun-Jie,Melia, Fulvio,Wu, Xue-Feng. Impact of a Locally Measured H-0 on the Interpretation of Cosmic-chronometer Data[J]. ASTROPHYSICAL JOURNAL,2017,835(2):270-.
APA Wei, Jun-Jie,Melia, Fulvio,&Wu, Xue-Feng.(2017).Impact of a Locally Measured H-0 on the Interpretation of Cosmic-chronometer Data.ASTROPHYSICAL JOURNAL,835(2),270-.
MLA Wei, Jun-Jie,et al."Impact of a Locally Measured H-0 on the Interpretation of Cosmic-chronometer Data".ASTROPHYSICAL JOURNAL 835.2(2017):270-.

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来源:紫金山天文台

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