中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
theeffectsofparametrizationofthedarkenergyequationofstate

文献类型:期刊论文

作者Ke Shi1; Huang Yongfeng1; Tan Lu2
刊名researchinastronomyandastrophysics
出版日期2011
卷号011期号:012页码:1403
ISSN号1674-4527
英文摘要We investigate in detail the influence of parametrizations of the dark energy equation of state on reconstructing dark energy geometrical parameters, such as the deceleration parameter q(z) and Om diagnostic. We use a type Ia supernova sample, baryon acoustic oscillation data, cosmic microwave background information along with twelve observational Hubble data points to constrain cosmological parameters. With the joint analysis of these current datasets, we find that the parametrizations of w(z) have little influence on the reconstruction result of q(z) and Ore. The same is true for the transition (cosmic deceleration to acceleration) redshift zt, for which we find that for different parametrizations of w(z), the best fitted values of zt are very close to each other (about 0.65). All of our results are in good agreement with the ACDM model. Furthermore, using the combination of datasets, we do not find any signal of decreasing cosmic acceleration as suggested in some recent papers. The results suggest that the influence of the prior w(z) is not as severe as one may anticipate, and thus we can, to some extent, safely use a reasonable parametrization of w(z) to reconstruct some other dark energy parameters (e.g. q(z), Ore) with a combination of datasets.
语种英语
源URL[http://libir.pmo.ac.cn/handle/332002/29650]  
专题中国科学院紫金山天文台
作者单位1.南京大学
2.中国科学院紫金山天文台
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Ke Shi,Huang Yongfeng,Tan Lu. theeffectsofparametrizationofthedarkenergyequationofstate[J]. researchinastronomyandastrophysics,2011,011(012):1403.
APA Ke Shi,Huang Yongfeng,&Tan Lu.(2011).theeffectsofparametrizationofthedarkenergyequationofstate.researchinastronomyandastrophysics,011(012),1403.
MLA Ke Shi,et al."theeffectsofparametrizationofthedarkenergyequationofstate".researchinastronomyandastrophysics 011.012(2011):1403.

入库方式: OAI收割

来源:紫金山天文台

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