Constraining dark energy using observational growth rate data | |
Shi, K.1,2; Huang, Y. F.1,2; Lu, T.3,4![]() | |
刊名 | PHYSICS LETTERS B
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2012-10-31 | |
卷号 | 717期号:4-5页码:299-306 |
关键词 | Cosmological parameters Dark energy Large-scale structure of universe |
英文摘要 | Observational growth rate data had been derived from observations of redshift distortions in galaxy redshift surveys. Here we use the growth rate data to place constraints on the dark energy model parameters. By performing a joint analysis with the Type la supernova, baryon acoustic oscillation and cosmic microwave background data, it is found that the growth rate data are useful for improving the constraints. The joint constraints show that the ACDM model is still in good agreement with current observations, although a time-variant dark energy still cannot be ruled out. It is argued that the growth rate data are helpful for understanding the dark energy. With more accurate data available in the future, we will have a powerful tool for constraining the cosmological and dark energy parameters. (C) 2012 Elsevier B.V. All rights reserved. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Physics, Multidisciplinary |
研究领域[WOS] | Physics |
关键词[WOS] | EQUATION-OF-STATE ; BARYON ACOUSTIC-OSCILLATIONS ; REDSHIFT-SPACE DISTORTIONS ; PROBE WMAP OBSERVATIONS ; LUMINOUS RED GALAXIES ; GAMMA-RAY BURSTS ; COSMOLOGICAL CONSTANT ; PERTURBATIONS ; SUPERNOVAE ; COMPONENT |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000310863300003 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/15539] ![]() |
专题 | 紫金山天文台_院士文集_陆埮 |
作者单位 | 1.Nanjing Univ, Dept Astron, Nanjing 210093, Jiangsu, Peoples R China 2.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China 3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 4.Nanjing Univ, Purple Mt Observ, Joint Ctr Particle Nucl Phys & Cosmol, Nanjing 210093, Jiangsu, Peoples R China |
推荐引用方式 GB/T 7714 | Shi, K.,Huang, Y. F.,Lu, T.. Constraining dark energy using observational growth rate data[J]. PHYSICS LETTERS B,2012,717(4-5):299-306. |
APA | Shi, K.,Huang, Y. F.,&Lu, T..(2012).Constraining dark energy using observational growth rate data.PHYSICS LETTERS B,717(4-5),299-306. |
MLA | Shi, K.,et al."Constraining dark energy using observational growth rate data".PHYSICS LETTERS B 717.4-5(2012):299-306. |
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