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• W3100110364 abstract "In this paper, we propose a new method to use the strong lensing data sets to constrain a cosmological model. By taking the ratio [Formula: see text] as cosmic observations, one can completely eliminate the uncertainty caused by the relation σ SIS = f E σ 0 which characterizes the relation between the stellar velocity dispersion σ 0 and the velocity dispersion σ SIS . Via our method, a relative tight constraint to the cosmological model space can be obtained, for the spatially flat ΛCDM model as an example [Formula: see text] in 3σ regions. And by using this method, one can also probe the nature of dark energy and the spatial curvature of our Universe." @default.
• W3100110364 created "2020-11-23" @default.
• W3100110364 creator A5018656868 @default.
• W3100110364 creator A5086045569 @default.
• W3100110364 date "2013-05-10" @default.
• W3100110364 modified "2023-10-18" @default.
• W3100110364 title "STRONG GRAVITATIONAL LENSING AND ITS COSMIC CONSTRAINTS" @default.
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• W3100110364 doi "https://doi.org/10.1142/s0217732313500570" @default.
• W3100110364 hasPublicationYear "2013" @default.
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