Growth of linear matter perturbations and current observational constraints

doi:10.1088/1674-1056/19/7/079801

Abstract We discuss, using a recently proposed parametrization for the growth index of linear matter perturbations, the observational constraints on the wCDM model and the Dvali—Gabadadze—Porrati (DGP) model with all current growth factor data. We find that the wCDM model is allowed by the observations at the 1$\sigma$ confidence level, while the DGP model is only consistent with observations at 2$\sigma$ confidence level.

Keywords: dark energy DGP model matter perturbations

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PACS:	95.35.+d	(Dark matter)
	95.36.+x	(Dark energy)
	98.80.Es	(Observational cosmology (including Hubble constant, distance scale, cosmological constant, early Universe, etc))
	95.30.Sf	(Relativity and gravitation)

Fund: Project supported by the National Natural Science Foundation of China (Grants Nos. 10775050, 10705055 and 10935013), the Specialized Research Fund for the Doctoral Program of Higher Education (Grant No. 20070542002), the Programme for the Key Discipline in Hunan Province of China, the Foundation for the Author of National Excellent Doctoral Dissertation of China (Grant No. 200922) and the New Century Educational Talents Plan of Chinese Education Ministry (Grant No. 09-0144).

Cite this article:

Fu Xiang-Yun(付响云), Wu Pu-Xun(吴普训), and Yu Hong-Wei(余洪伟) Growth of linear matter perturbations and current observational constraints 2010 Chin. Phys. B 19 079801

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Growth of linear matter perturbations and current observational constraints

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